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secondary education in five year plan
ond five-year plan. The major recom-mendations include: 1. Language and Culture I & II may be met in high school and are not included in this 4-year plan. The educational foundations and computing courses are designed for those entering the education field. At INR 2.70 lakh crore, it constitutes 20% of […] in Secondary Education is a combined undergraduate-graduate five year degree program (bachelors + masters + teaching license) designed for students who are pursuing a bachelor's degree in the College of Arts and Sciences and who also wish to … 11th Five Year Plan. Eleventh Five Year Plan: Inclusive Growth, 2007-12. ˚ e Five-Year Master's Plan is a pathway to earning two powerful credentials, a Bachelor of Arts degree and a Master of Arts in Teaching degree, in just ˜ ve years. Rebecca Keatley and Mr Smith are down on the farm, learning about equal and unequal groups, multiplication and arrays. Eleventh Five Year Plan: Social Sector, 2007-12. Addressing the convocation, the Prime Minister said the 11th five year plan presents a comprehensive strategy for strengthening the education sector covering all segments of the education pyramid. When you complete the Middle-Secondary Education degree from Marian University, you will not only be ready for licensure […] foundations in microbiology secondary vocational schools twelfth five year plan standard teaching material chinese edition Oct 03, 2020 Posted By Frank G. Slaughter Ltd TEXT ID d12259a1d Online PDF Ebook Epub Library microbiology 10th edition pdf book description foundations in microbiology is a allied health microbiology text using a taxonomic approach to this disorder chapters were Students should consult with their adviser to … STRATEGIC DIRECTION 5: Prepare math majors to be successful in graduate school and in careers in secondary education… The Action Plan for Education 2017 is an important document, marking the first annual action plan under the broader strategic framework of the Action Plan for Education 2016-2019 which was published in September 2016. About. As a part of the tenth Five-year Plan (2002–2007), the central government of India outlined an expenditure of 65.6% of its total education budget of ₹ 438 billion (US$6.1 billion) i.e. The 11th Plan, approved at the meeting of the National Development Council in December 2007, places the highest priority on education as a centred instrument for achieving rapid and inclusive growth. Multi-purpose secondary schools, to add agriculture, technical subjects, and commerce to the present curriculum. The theme of it is, "Nurturing Industrialization for Economic Transformation and Human Development" with the main objective of enhancing the pace of progress towards the Tanzania Development Vision 2025. The secondary programs are designed for those wanting to teach content to middle school and/or high school students. Monday 30 November: A new numeracy Live Lesson for 5-7 year-olds. Please see requirement details. 4 ASEAN 5-Year Work Plan on Education Strategic Direc on for ASEAN Coopera on in Educa on The development of the ASEAN 5-Year WPE (2011-2015) drew impetus from the decision of the Fourth ASEAN Educa on Ministers Mee ng (4th ASED) held on 5-8 April 2009 in Phuket. Education Strategic Plan 2018–2030 v 4.2 Cost projections 72 4.3 External support for the ESP 86 5 M&E framework 89 5.1 Basic education indicators 89 5.2 Secondary education indicators 93 5.3 TVET indicators 96 5.4 NFE indicators 97 5.5 Inclusive and special education indicators 99 5.6 Tertiary education indicators 101 On December 1, the Ministry of Education held a press conference. The program also focuses on supporting under-represented students (e.g. Our resources are designed to work together from Year 7 to Year 11, providing a coherent 5-year curriculum and consistent assessment framework. The IES includes a five-year Outbound Student Mobility Pilot program which will help post-secondary students with the costs of study or work abroad. A 4-3-4-3 system: primary, middle, sec-ondary, and college stages. Kindergarten education in Hong Kong is for children from 3 to 6 years old. English Major - Secondary Education Concentration Suggested Four-Year Plan Based on course availability and student needs and preferences, the selected sequences will probably vary from those presented below. 21516-2192 1 REVISED FIVE-YEAR STRATEGIC PLAN 2015/16-2019/20 MARCH 2016. programs in either Secondary, students must apply to the Professional Teacher Education Program (master's portion of the program) within their majors. New factories were opened, especially in the east. On 4 th October, the government of India approved the 12th five year plan (2012-17) that aims to achieve annual average economic growth rate of 8.2 per cent, down from 9 per cent (Eleventh plan 2007-12).. DEPARTMENT OF BASIC EDUCATION REVISED FIVE-YEAR STRATEGIC PLAN 2015/16-2019/20. PLANNING COMMISSION HRD DIVISION 2. Five Year Development Plan, 2016/17- 2020/21 is the principal and shared tool in the realisation of these objectives. Indicator: Increase number of full-time Instructors by 1 each year until there are 15. Your child's secondary education goes from Year 9 to Year 13 (around 13-17 years of age). Choose a two- or three-year KS3 pathway to suit your needs. Many children go to a … The instructor ranks should stabilize at 15 after 5 years. Local non-profit-making kindergartens joining the kindergarten education scheme are provided with direct government subsidy. 3. 1.1.4 The Eleventh Plan must also pay attention to the problems in the higher education sector, where there is a need to expand the system and also to improve quality. More railways were built to transport the goods produced such as steel, coal, iron, and oil. Every year the amount of steel, coal, iron and oil that was produced rose. The following School Improvement Plan describes the current status of Sample Christan School and provides a five year plan to ensure the school's viability in the future. There is a 4 year lower secondary education programme that concludes with students taking 'O' level examinations and then, for a small proportion, 2 further years of Students who are interested in pursuing the combined 5-year B.S./M.Ed. 2 STRATEGIC PLAN FOREWORD BY THE MINISTER OF BASIC EDUCATION Basic Education is a concurrent function in Government and as the sectoral departments whose functions are of delivery require According to Ren Youqun, Director of the Department of Teacher Work of the Ministry of Education, during the "13th Five-Year Plan" period, the number of teachers has increased from 15.39 million at the end of the "12th Five-Year Plan" to 17.32 million today, an increase of 12.5%, which strongly supports the world's largest educati ₹ 12.5 billion (US$180 million) on adult education; 9.5% i.e. The Master of Education (M.Ed.) Prime Minister Manmohan Singh has termed the 11th five year plan as "India's educational plan". Also I like to try and plan the unit at a relevant time (Basketball around March Madness or during Basketball Season… Soccer around the World Cup or during soccer season) You can see a video of my entire process below. Overview The CIF (Curriculum, Instruction, & Foundations) program includes elementary, secondary, educational foundations, and educational computing for pre-service teachers. Public sector schools form the majority in the 6-year primary and 6-year secondary basic education… SCHOOL EDUCATION SECTOR School Education Sector covers:1.Pre-primary Education2.Primary Education ( Class I-V)3.Upper Primary Education ( Class VI-VIII)3.Secondary Education (Class IX-X)4.Higher Secondary Education ( Class XI-XII)5.Vocational Education6.Adult Education ( Literacy) 2 ˚ e Five-Year Master's Plan can help you develop a highly marketable and ˛ exible skill set that will equip you to work in … ₹ 43.25 billion (US$610 million) on secondary education; 2.9% i.e. The education system for schools is made up of 13 Year levels. The Biden plan will invest $18 billion in grants to these four-year schools, equivalent to up to two years of tuition per low-income and middle class student, including DREAMers and students who transfer to a four-year HBCU, TCU, or MSI from a tuition-free community college. Local schools. Eleventh Five Year Plan: Education, 2007-12. Flexible resources that work for your setting . It's a bit long, but I did plan the whole year in under 15 minutes, so I'd call it a win. ₹ 288 billion (US$4.0 billion) on elementary education; 9.9% i.e. The Marian University Bachelor of Science in Middle-Secondary Education program will give you the skills and knowledge to cultivate the educational and personal growth of youth ages 10-18 in grades 5-12. First Plan (1951–1956) The first Indian prime minister, Jawaharlal Nehru, presented the First Five-Year Plan to the Parliament of India and needed urgent attention. In addition to the test score requirement for admission into the program, all Secondary Education and Teaching majors must meet all Praxis requirements prior to the semester you anticipate Residency I of the year-long teacher residency. School Education and Literacy in the 12th Plan (2012 - 2017) 1. Third Five Year Plan (1965-70) It recognized "the concept of education as a vital national investment and a major determination of the nation's economic growth." The Third Plan aimed at widening the base of primary education and proposed to increase the primary enrollment rate from 45 to 70 per cent in 1970. Find out how we can support your school. We encourage you to follow this plan to help you stay track to graduate on time. Grades 1 & 2, followed by 5 years of junior education after which all students sit for the national grade 7 examinations. *This is a suggested curriculum plan to complete this degree program in four years. Get Classroom Experience Starting Freshman Year. Your child's primary education starts at Year 1 and goes to Year 8 (around 5-12 years of age). The Action Plan for Education 2016-2019 articulates the ambition, values and goals Your 5 Year Agreement (5YA) funding is based on a formula. The plan was created by the School Improvement Committee in collaboration with Sample Christian School's faculty and administration. The First Five-year Plan was launched in 1951 which mainly focused in development of the primary sector.The First Five-Year Plan was based on the Harrod–Domar model with few modifications. There is a minimum budget set so that all schools have enough 5YA funding to do their essential work. Working Group on Secondary and Vocational Education: 11th Five Year Plan, 2007 to 2012 As a board of trustees, you need to decide how to allocate your 5YA funding in your 10 Year Property Plan (10YPP) following certain rules on how to spend this funding. NOTE: Students may apply for admission to the Professional Teacher Education Programs only once. Foreword by the Secretary of State for Education and Skills 3 Executive Summary 6 Chapter 1: Introduction 12 Chapter 2: Early Years 20 Chapter 3: Primary Schools 32 Chapter 4: Independent Specialist Schools 44 Chapter 5: Personalisation and choice in the secondary years 58 Chapter 6: 14–19 Education and Training 68 Chapter 7: Adult Skills 80 and education. We've mapped out a 4-year plan for our Secondary Education and Teaching majors. 2. a Mission for Secondary Education is essential to consolidate the gains of SSA and to move forward in establishing a knowledge society. The five year plan also resulted in many peasants leaving the countryside to work in towns or industrial centers.
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secondary education in five year plan 2020


Islamic Spirituality is based upon the assumption that what appears to us mystery revealed itself as being God. The Qur'an is this revelation. The Qur'an Instructs us in the foundational importance of awareness of God and the proper response to God. The Sunnah (lifestyle or practice) of Muhammad expresses and exemplifies this Qur'anic awareness of, and response to God within actual, historical phenomenal reality. This is the heart and foundation and raison d'etre of Islamic spirituality. Muhammad is considered to be a "walking Qur'an". Islamic spirituality fosters God-consciousness, called taqwa, in and through add daily activities in addition to activities we usually identify as 'spiritual" such as fasting and prayer. It shuns any extermes. Islamic spirituality is active in all four aspects of human experience. It thus avoids extremes of interiority and does not portray the physical or the social as being contra the spirtual.
Dr. YA Sabba is a highly educated scholar and academic adept in Urdu, Hindi and Persian having MA, PhD form Delhi University. He is an Associate Professor teaching in the University. He sincerely devoted to his time teaching and writing related to his field ad had also writing related to his field and had also attended several seminars and symposium on the subject.
The Quadiriyyah Order -- Pg. 25 3.


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Terahertz laser source at room temperature
Source: PhysOrg.com.
"There is a growing interest in utilizing terahertz radiation, or T-rays, for a variety of applications," Mikhail Belkin, a scientist at Harvard University, says. "The terahertz region is a part of the electromagnetic spectrum that lies between the radio waves and infrared/visible light."
Producing light in the terahertz range gets tricky, though: "Currently, the way to generate this radiation at room temperature involves solid state lasers that are bulky and energy consuming." In order to facilitate the creation of practical terahertz devices and systems, Belkin points out that "we want to create a compact electrically-pumped terahertz source, similar to semiconductor lasers in infrared and visible that you can fit in a laser pointer, and to be able to operate it at room temperature."
The applications for a laser device operating in the terahertz range include security screening, radio astronomy, biomedical imaging, and spectroscopy. "The main funding for our work comes from the security aspect," Belkin explains. "Terahertz rays can penetrate through cardboard, plastic, clothing, and many other materials, so that we can image a concealed weapon, or detect chemical and biological agents through sealed packages."
Along with colleagues at Texas A&M University and the Swiss Federal Institute of Technology, Zürich, Belkin believes a first step has been made in developing a practical room-temperature electrically-pumped semiconductor laser device that produces terahertz radiation. The key is to combine, in one device, a dual-wavelength infrared semiconductor laser and giant optical nonlinearity for difference-frequency mixing. Their current device produces approximately 300nW of 5THz radiation at room temperature. The findings are published in the article "Room temperature terahertz quantum cascade laser source based on intracavity difference-frequency generation" in the May 19 issue of Applied Physics Letters.
"We undertook an unusual approach to the problem, going around with a dual-wavelength quantum cascade laser operating at room-temperature in mid-infrared and utilizing a nonlinear optical process of difference-frequency generation inside the laser cavity to produce terahertz radiation," explains Belkin, expounding via email.
He continues: "In order to make the concept work, we needed to integrate giant optical nonlinearity inside the laser cavity. This has been done by growing a structure containing a stack of ultra-thin atomic layers of semiconductor materials on top of each other. This approach allowed us to adjust the energy levels in the structure to create an artificial medium with very large optical nonlinearity."
Right now, Belkin admits, the terahertz power output of their current devices is smaller that he and his colleagues would like. However, they have demonstrated the first room-temperature electrically-pumped semiconductor laser source of terahertz radiation. Additionally, the team is already making changes to the design to improve the terahertz power output. "We are confident that the power output of our devices can be improved several orders of magnitude when the structure is fully optimized," Belkin says.

redpajama_set_name: RedPajamaCommonCrawl


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Production Design For Variety, Nonfiction, Event or Award Special
Casting For A Limited Series, Movie Or A Special
Cinematography For A Single-Camera Series
Costumes For A Contemporary Series, Limited Series or Movie
Costumes For A Period | Fantasy Series, Limited Series Or Movie
Costumes For A Variety, Nonfiction or Reality Programming
Directing For Nonfiction Programming
Writing For Nonfiction Programming
Electronic Production
Lighting Design | Lighting Direction For A Variety Series
Lighting Design | Lighting Direction For A Variety Special
Technical Direction, Camerawork, Video Control For A Limited Series, Movie Or A Special
Creative Achievement In Interactive Media - Multiplatform Storytelling (Juried)
Creative Achievement In Interactive Media - Original Interactive Program (Juried)
Creative Achievement In Interactive Media - Social TV Experience (Juried)
Creative Achievement In Interactive Media - User Experience And Visual Design (Juried)
Prosthetic Makeup For A Series, Limited Series, Movie Or Special
Music Composition For A Limited Series, Movie Or Special (Original Dramatic Score)
Picture Editing For An Unstructured Reality Programming
Single-Camera Picture Editing For A Limited Series Or A Movie
Sound Mixing For A Limited Series Or A Movie
Special Class Programs
Stunt Coordination For A Comedy Series Or A Variety Program
Stunt Coordination For A Drama Series, Limited Series Or Movie
Outstanding Single-Camera Picture Editing For A Limited Series Or Movie - 2016
"Waiting for Dutch"
Skip Macdonald, ACE
"Did You Do This? No, You Did It!"
Curtis Thurber
The People v. O.J. Simpson: American Crime Story
"From The Ashes Of Tragedy"
Adam Penn
"The Verdict"
Stewart Schill, ACE
"The Race Card"
C. Chi-Yoon Chung
2014 - 66th2015 - 67th2016 - 68th2017 - 69th2018 - 70th
Outstanding Documentary Or Nonfiction Series


Artonic was honored to be contacted for the Adrian Graduate Studies website design. Working closely with graduate professors and team members within the grad studies programs, Artonic created a website prototype, search engine optimized content, and a user-friendly design. The finished website showcases custom photography from Adrian College's photographer. The design is beautiful, modern, and sophisticated.
This website design project was multifaceted with detailed brand guidelines, numerous contacts within the college, and a tight deadline. We worked with each professor at the Graduate College to complete a personal profile and an up-to-date programs page. The final website design is one of Artonic's favorites!


business - Recipe for Disaster?
Recent storms serve as reminders to review your homeowners policy--or regret it later.
When natural disasters strike, the most important consideration is survival. It isn't until after the hurricane winds stop blowing, the tor-nado stops twisting, or the earth stops quaking that the financial wounds become apparent. They can, though, be almost as painful as physical ones. Just ask the hundreds of thousands of Americans whose homes or businesses recently took a hit from Hurricanes Charley, Frances and Ivan. Damage from those three storms could reach tens of billions of dollars by the time the counting is done-much of which won't be covered by insurance.
Americans who live along the hurricane zones of the Southeast, the Tornado Alley of the Plains, or the tectonic fault lines of the Pacific Coast have obvious reasons to worry about natural disasters. But no matter where you live, events like the three hurricanes mentioned above provide reason enough to take a quick peek at your homeowners policy. Better yet, make it an annual tradition to review the insurance that protects one of the biggest investments you'll ever make.
A standard homeowners policy covers a house, its contents, landscaping and outbuildings, along with any visitors to the property. Damage from a number of situations-fire, hailstorm, falling trees and so on-will typically be insured against. Other potentially costly problems, though, tend to be omitted. Earthquakes? Not usually covered. Floods? From broken pipes, yes, but not from rising water courtesy of Mother Nature. Mold infestations? If at all, with a limit so low it won't help much if mold is actually discovered.
Much of the language in a homeowners policy is boilerplate written by and for lawyers, which means it's unintelligible to the rest of us. If nothing else, though, read the exclusions section of your policy. You'll find it in the "conditions and coverages" section. For most people, what they read there is enough to keep them awake at night. It's a nightmare list of all the disasters that could befall your house, leaving you a financial wreck, homeless and maybe even bankrupt.
Armed with that list, decide what risks you are-and are not-willing to accept. It isn't just disasters, either. Don't forget to consider excluded items such as high-value jewelry. Keep in mind, too, pets that might limit or void your policy. Faced with an increasing number of dog-bite claims, for example, many insurance companies are refusing to sell or renew policies to homeowners with Doberman pinschers, pit bulls, Rottweilers and some other breeds. Check your policy for pet limits or exclusions. Then head to an insurance agent to get quotes on policy amendments or additional coverage that might fill in the gaps.


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Former NHL goalie shares struggles with mental illness, addiction | CBC News Loaded
Former NHL goalie shares struggles with mental illness, addiction
Former NHL goaltender Clint Malarchuk has gone through both physical and mental trauma in his life and, after two brushes with death, he's sharing his story and advocating for better mental health support.
Addiction affects the whole family but 'we close our eyes to it,' says Clint Malarchuk
Clare Hennig · CBC News · Posted: Apr 14, 2018 9:00 AM EDT | Last Updated: April 14, 2018
Clint Malarchuk, seen playing goal for Buffalo in 1990, is sharing his story to help reduce the stigma surrounding mental health. (Rick Stewart/Getty Images)
Malarchuk endured one of the most horrific injuries in NHL history in 1989 when he was playing goal for the Buffalo Sabres. The skate of an opposing player clipped his throat and severed his jugular vein.
Ex-NHL goalie Clint Malarchuk opens up on mental illness in 'The Crazy Game'
"That was the beginning of a real spiral downward because of trauma, which now they call PTSD," he told Gloria Macarenko, guest host of CBC's The Early Edition. "It really set me off in a lot of bad ways."
Malarchuk was back on the ice 10 days after his injury and continued to be professionally involved in hockey for many years after.
But he faced a long battle with obsessive compulsive disorder, depression, anxiety, panic attacks and nightmares, Malarchuk said.
"I self-medicated with alcohol to try and calm my anxiety or pick me up when I was depressed," he said. "Addiction and mental illness, it almost goes hand in hand for so many of us."
At his lowest, Malarchuk attempted suicide.
"Being a suicide survivor, I'm a big advocate for helping people on addiction," he said. "There is no way I would have pulled that trigger had I been sober."
Malarchuk returned to the ice within days of the accident that nearly took his life. (Rick Stewart /Allsport)
Impact of addiction
He's taking part in an event this weekend in Surrey about the impact of addiction on families.
"Addiction is so out there, we close our eyes to it a lot of times and it affects the whole family," he said. "They see it, they live it. How do you handle it?"
Malarchuk's own story begins in a family where his father battled alcohol addiction, he said.
Still haunted
Even long after the initial trauma, the effects linger and memories can be triggered, he said.
"It still haunts me," Malarchuk said.
Malarchuk said his mental health suffered a severe setback in 2008 when Florida Panthers player Richard Zednik suffered a similar injury to the one he had.
Tragedies like last week's crash between the Humboldt Broncos team bus and a semi-trailer can also have an impact.
No need to suffer alone with PTSD, former NHL goalie Clint Malarchuk tells first responders
Former NHL player Clint Malarchuk talks PTSD, addiction in Saskatoon
"Anybody in Canada, or even North America, can really be thrown through a loop on that, but somebody like myself who has struggled with trauma, it affected me," he said.
Malarchuk is speaking at the free event in Surrey, called How Addiction Affects Families, on Saturday, April 14.
If you or someone you know needs help, contact The Crisis Intervention and Suicide Prevention Centre of B.C. by phone at 1-800-SUICIDE or online.
With files from The Early Edition.


Do you have friends who might want to join you in this free webinar? Easily share it using any of the buttons below.
Save the date Thursday, April 11th at 8pm ET on your calendar and look out for an email from me in the next few minutes with next steps.


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» Forum » Motorsport » Canadian GP
#1 | Canadian GP Fri Jun 09, 2017 11:52 pm
jpp47
Kimi Raikkonen set the pace in the second Formula 1 practice session for the Canadian Grand Prix.
The Finn clocked a 1m12.935s at the Circuit Gilles Villeneuve in Montreal to finish 0.215 seconds clear of Lewis Hamilton's Mercedes.
Championship leader Sebastian Vettel and Valtteri Bottas were third and fourth respectively with the top four separated by 0.375s.
The super-soft was the tyre of choice for the early running, before teams turned their attention to the ultra-softs for qualifying simulations.
Vettel was among the first to do his low-fuel run and promptly went quickest, with team-mate Raikkonen slotting into second.
Raikkonen then improved to go fastest, with Hamilton moving up into second and Vettel demoted to third.
Max Verstappen was the leading Red Bull in fifth, 0.453s off the pace, but his session was curtailed 20 minutes early when he stopped out on track with a gearbox problem.
The session was red-flagged while the teenager's car was recovered from the side of the track between Turns 7 and 8.
It compounded a frustrating afternoon for the team, with Daniel Ricciardo spending most of the session in the garage after suffering an engine problem.
Felipe Massa was sixth, but he was nearly seven tenths further back in the Williams, with Fernando Alonso bouncing back from a late start to the session to go seventh at the chequered flag.
Esteban Ocon, Daniil Kvyat and Sergio Perez completed the top 10.
Romain Grosjean was 11th after he endured a frustrating session, spinning twice at Turn 6 and once at Turn 1 before ranting on the radio to his team about the situation.
He was just one of a series of drivers, that included Vettel, Bottas, Kvyat (pictured) and Perez, who spun during the session.
Carlos Sainz Jr recovered from failing to set a timed lap in FP1 to rack up more than 40 laps in the Toro Rosso, ending the day 13th-fastest.
Near the back of the field, Stoffel Vandoorne failed to set a representative qualifying simulation time after spinning at the final chicane on his new-tyre run.
FP2 TIMES
POS	DRIVER	CAR	TIME	GAP	LAPS
1	Kimi Raikkonen	Ferrari	1m12.935s	-	41
2	Lewis Hamilton	Mercedes	1m13.150s	0.215s	41
3	Sebastian Vettel	Ferrari	1m13.200s	0.265s	41
4	Valtteri Bottas	Mercedes	1m13.310s	0.375s	42
5	Max Verstappen	Red Bull/Renault	1m13.388s	0.453s	25
6	Felipe Massa	Williams/Mercedes	1m14.063s	1.128s	38
7	Fernando Alonso	McLaren/Honda	1m14.245s	1.310s	19
8	Esteban Ocon	Force India/Mercedes	1m14.299s	1.364s	46
9	Daniil Kvyat	Toro Rosso/Renault	1m14.461s	1.526s	38
10	Sergio Perez	Force India/Mercedes	1m14.501s	1.566s	41
11	Romain Grosjean	Haas/Ferrari	1m14.566s	1.631s	33
12	Nico Hulkenberg	Renault	1m14.604s	1.669s	38
13	Carlos Sainz	Toro Rosso/Renault	1m14.621s	1.686s	43
14	Kevin Magnussen	Haas/Ferrari	1m14.676s	1.741s	35
15	Daniel Ricciardo	Red Bull/Renault	1m15.072s	2.137s	8
16	Jolyon Palmer	Renault	1m15.127s	2.192s	40
17	Lance Stroll	Williams/Mercedes	1m15.240s	2.305s	40
18	Marcus Ericsson	Sauber/Ferrari	1m15.611s	2.676s	31
19	Stoffel Vandoorne	McLaren/Honda	1m15.624s	2.689s	20
20	Pascal Wehrlein	Sauber/Ferrari	1m16.308s	3.373s	31
#2 | RE: Canadian GP Fri Jun 09, 2017 11:54 pm
Ferrari team principal Maurizio Arrivabene says he was "laughing a bit" at suggestions the team is favouring Sebastian Vettel over Kimi Raikkonen in the 2017 Formula 1 title battle.
Raikkonen had taken pole ahead of his team-mate at the Monaco Grand Prix and the Finn had led until the pitstops, with Vettel's later stop allowing him to take the lead and go on to win the race.
Vettel's victory meant he extended his championship lead over Hamilton to 25 points, and the Ferrari driver has finished ahead of Raikkonen in all the races this season.
Arrivabene insisted Vettel is not the number one driver in the Ferrari line-up, claiming that the team's priority is the constructors' standings.
"I was reading after Monaco and hearing all the speculation about number one and number two, I always said that the situation is that we are looking forward in the championship, to do all our best for the constructors' championship," Arrivabene said in Canada.
"If you do well in the constructors' championship, you need two drivers and this is better at the moment for Ferrari. It is the only trophy that if you win, it stays at home. The drivers' trophy goes to the drivers, of course."
Hamilton's seventh place finish in Canada meant his points defecit to Vettel increased from six points to 25, and he argued after the race that Ferrari was "clearly" favouring Vettel - although the two Ferrari drivers dismissed such suggestions.
Arrivabene said both Ferrari drivers were well aware of the team's current policy.
"I was very clear since the beginning of the season. Until the numbers are going in one direction or the other direction in the championship, there will be no team orders.
"I am very, very clear. The drivers know all about this, they accept it. I think, what has happened in Monaco - I was a bit laughing when I heard the stories. It is not the reality.
"We are looking for the constructors' championship, but in the drivers' championship they are free to do it until the numbers are clear in one direction or the other."
What kind of liar he is,,,,,,,,,,,
#4 | RE: Canadian GP Sat Jun 10, 2017 9:48 pm
Quote: jpp47 wrote in post #3
I think they read a lot of critics in the last weeks, thats why he need to talk it down.
There are rumors that Ferrari offer Kimi a contract for 2018. Let´s see what he will do
P4 in quali
Raikkonen says he paid the price for a mistake in F1 qualifying
Kimi Raikkonen said he "paid the price" for a mistake when it counted in the closing moments of Formula 1 qualifying for the Canadian Grand Prix.
The Finn, who set the pace during Friday practice, had to settle for fourth on the grid, and he believes he was capable of more than that if he hadn't made an error on his final run.
"There was a lot of speed on the last lap, but I made a mistake in corner two," said Raikkonen.
"I improved a little bit, but I couldn't make the lap very good, and I paid the price for it.
"It was a little bit more tricky today than yesterday just to get a good feeling with the tyres, but that's how it goes."
While his Ferrari team-mate Sebastian Vettel ended up three tenths of a second adrift of an inspired Lewis Hamilton in the fight for pole, Raikkonen was nearly eight tenths back, which he described as "not a surprise".
"At places like this, if you get one corner wrong, you're going to lose massive lap time," he said.
"Our car has been good, but for whatever reason we've struggled a bit in qualifying."
However, Raikkonen believes the race "will be a different story", with the Montreal venue traditionally throwing up unexpected circumstances and incident-packed grands prix.
"Often it's quite a hectic race here, a lot of things happen," he said.
"You never know here, it's one of those places things can change quite quickly.
"We'll try again, we'll see what happens. We should have good speed."
http://www.autosport.com/news/report.php...e-in-qualifying
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#7 | RE: Canadian GP Sat Jun 10, 2017 10:04 pm
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#8 | RE: Canadian GP Sun Jun 11, 2017 10:26 pm
Strange race
A long fight back for Seb to finish fourth and Kimi seventh
Montreal – The toughest Grand Prix of the year ended with Seb in fourth place and Kimi in seventh. Given how things went on the opening lap, with both cars damaged and a front wing to change, a strategy to rejig, overtaking moves to make, it was a demonstration of courage and determination from drivers and team. Sebastian still leads the Drivers' championship on 141 points, 13 more than Hamilton.
Gusty conditions, dust flying around the track and even a few black but harmless clouds all served to ramp up the tension before the start. Verstappen's blistering start meant that Seb, who had got off the line well, had to lift off. He thus found himself back in fourth, but further back, a collision between Massa and Sainz immediately brought out the Safety Car. Max's move had damaged the right front wing end plate on Sebastian's car. Rather than risk further problems, he pitted for a new nose and a change to Supersofts. Unfortunately, the SF70H had additional damage to the floor. Meanwhile, Kimi lost ground in the duel with Ricciardo and found himself sixth and a trip across the grass also caused him some damage.
Verstappen's race ended at the side of the track at Turn 3 and out came the safety car again, albeit this time a virtual one. The race resumed on lap 14 and that number also represented Seb's position, but he soon dispensed with Grosjean. On lap 18, Kimi, who was having a tricky time of it, pitted and fitted the red-banded tyres and by this point Seb was already up to eleventh. He then passed Hulkenberg to move into the points before pulling off a passing move on Stroll at the chicane. Kimi got ahead of Alonso to go sixth, with Sebastian now just two places further back having come out on top of duels with Magnussen and Fernando.
Life wasn't easy with two damaged cars: on lap 42, Kimi pitted for fresh rubber, the super-quick Ultrasofts. Seb stayed out until lap 50, dealing with traffic ahead of him, but he would also have to rescue his race with the purple tyres, with which Kimi was now flying. Seb started to demolish the lap times, getting under the 1'15" mark with 10 laps to go. He passed Kimi who had a brake control issue. At the start of lap 66, Seb pulled off a miracle, risking everything to pass Ocon who was also using the DRS. Perez was now in his sights and he slipped by at the start of the penultimate lap, so that his race ended just off the podium. KImi brought his wounded No 7 car home in seventh spot. "Thanks guys" was the immediate message from Maurizio. That said it all.
http://formula1.ferrari.com/en/canadian-...to-be-proud-of/
DCEIp0HWAAAnShE.jpg - Bild entfernt (keine Rechte)
#9 | RE: Canadian GP Sun Jun 11, 2017 10:29 pm (Last edited: Sun Jun 11, 2017 10:30 pm)
DCDd1A2XYAItsEH.jpg - Bild entfernt (keine Rechte)
DCDebpsXcAAzkoK.jpg - Bild entfernt (keine Rechte)
Best part of the race
DCELpCDW0AIbtg3.jpg - Bild entfernt (keine Rechte)
DCEKnC5XcAAIS-x.jpg - Bild entfernt (keine Rechte)
#10 | RE: Canadian GP Mon Jun 12, 2017 8:24 pm
sad race for me. problems for kimi seem to have kept him behind the pink cars
F1 GP Monaco 2017 » « F1 GP Azerbaijan 2017


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Another local elementary school is holding their annual Easter egg hunt for teachers/staff this morning! They have it out on their playground and prizes in the eggs include candy, gift cards, jeans passes, early dismissal pass, free day off pass, etc.
I am throwing an Easter Sunday Sale! Be sure to hop on over to my store to get 20% off everything!


text:
\section{Introduction}

The string-theory-inspired TeV-Gravity models \cite{TVG},
where matter lives on a 3-brane embedded into a
$D$-dimensional space-time with the extra $D-4$ dimensions
compactified on a manifold of the inverse size $\sim 1\div 10 {\rm TeV}$,
opened a potential possibility to observe non-trivial
gravitational effects in accelerator \cite{acc},
cosmic ray \cite{mmt} and neutrino \cite{nuMBH} experiments.
So far, attention in this field was restricted to effects, associated with
the possible production of mini-black-holes (MBH), which
can be {\it massively} produced already at LHC if TeV-Gravity models
are true. These MBH are supposed to evaporate
instantaneously (see, however, \cite{Fron}),
but -- since Hawking radiation does not
distinguish between the sorts of particles and space directions --
can cause energy and momentum redistribution between the products
of reaction, which is potentially observable (though not
too pronounced -- as usual for the TeV-energy experiments).\footnote{We need
to mention here that while discussing experimental evidence of
the black hole evaporation one has to look after various conservation
laws like baryon number conservation. In particular, we believe that the
probability of black hole formation by quarks within a proton with a
subsequent evaporation, i.e. a proton decay into mesons and, possibly,
leptons is vanishing. Basing on some arbitrary assumptions about what
quantum gravity is, \cite{protonHaw}, one may estimate \cite{proton2}
the proton lifetime to be $M_{Pl}^{d+4}/m_p^{d+5}$ ($4+d$ is the number of
dimensions where quarks propagate) which is unacceptable large for
Tev-Gravity models. Note, however, that this is completely {\it quantum}
gravity (whatever it means) effect, while forming black holes in
accelerators is completely {\it classical} and, therefore, say, arguments in
\cite{Stoj} are absolutely misleading.}

It is natural to assume that the story should not be restricted
to MBH: once Pandora box
of gravitational effects on particle physics is open, all of its
content can show up. This implies that other types of
multi-dimensional gravitational configurations could also be born,
along with the MBH. Since much less is known about
such configurations, except that they appear on equal footing
with black holes in general relativity, we can just {\it assume}
that the same is true in particle theory: namely,
that, like MBH, they are created in particle collisions
{\it classically}, with the cross-sections,
defined by their geometrical sizes, with only a modest damping caused
by radiation of gravitational waves, and decay almost instantly,
either classically or due to some analogue of Hawking radiation.
If one agrees to accept this assumption,
the question arises whether any such configurations can leave traces
in the properties of particle collisions,
essentially different from those of mini-black-holes.

The most interesting from this perspective are the
(mini-)black-\-rings \cite{br} and, especially,
(mini-)time-\-machines (MTM): geometries with existing closed time-like
worldlines. There is a long story of discussions around
time-machines in general relativity \cite{tm}, we agree with
the recent conclusion of \cite{viss,Ori,kr1},
that no reasons were found to forbid their existence.\footnote{
Touching the subject of time machines, one, probably, should not avoid
comment on the celebrated grandfather, known also as butterfly or,
in scientific literature, as
Polchinski \cite{Polch}, paradox: what if, while traveling to the
past, one affects or even destroys the preconditions for its own creation.
Here one should be careful in distinguishing between ``affects" and ``destroys".
In the {\it former} case, there is no trouble: one should just modify the
relation between initial and final conditions (causes and corollaries),
remembering also that solutions to differential equations on spaces
with non-trivial topology are uniquely defined by initial conditions
for non-compact directions {\it and} by ``zero-modes" for compact ones (in other
words, the ``residents" of the time-machine should be included into
formulation of the Cauchy problem). In the {\it latter} case,
the ``problem" is actually a one of a G\"odel- or Echer-style
``impossible things": describing in a Human-created language
a non-existing entity. In quantum theory, one should sum over
all possible {\it globally defined} histories (world lines), and the
paradox normally describes in words a (self-contradictory) history,
which actually does not exist:
if {\it somebody} killed your grandfather, then
his world line terminated and could not lead to your birth-day, thus,
that {\it somebody} was not you. Hence, there is no continuous world line,
satisfying the conditions of the paradox, and the
{\it non-realizable} history of {\it you}
killing {\it your} grandfather does not
contribute to the functional integral. It is kinematically,
not dynamically, forbidden. Thus, the scientific problem related to grandfather
paradox is that of classical determinism and of accurate formulation of
Cauchy-like problems, existence and uniqueness of its solution,
in the presence of time machines. It is sometime a difficult, but in no
way a paradoxical problem. See \cite{gfp} for more considerations.}
Thus we suggest to switch the direction of the
discussion: from whether time-machines are allowed to exist
and be observable
(not separated from us by any sort of impenetrable horizon like
in the case of non-traversable wormhole, say, the Einstein-Rosen
bridge, \cite{Wheeler}), to whether we can notice them.
As explained above, the TeV-gravity models allow one to shift
this discussion to the solid ground of particle physics and
perhaps even to forthcoming accelerator experiments.
In this context the basic question is: can massively produced and
quickly ``evaporating" mini-time-machines
leave traces, somehow different from those of pure-particle-physics
processes (with no gravity effects) and from those caused by
mini-black-holes?
We do not say that discussion of mini-time-machines production rates
are not important -- quite the opposite, we shall see that these
rates can essentially affect the answer and need be evaluated, --
just, given all the experience of discussion of
``chronology protection principle" \cite{Haw}, we believe that one can
try to overstep this controversial subject and see what happens:
if something interesting occurs, then we can come back with more
enthusiasm and devotion.

One more word of caution is needed, this time not from the
general-relativity, but from the particle-theory side.
The best one can technically do at the moment is to consider MBH and MTM,
once they are created, as classical backgrounds and see what
happens to particles embedded into them. In MBH case it was
sufficient to accept the existence of Hawking radiation,
in the MTM case we discuss below a some more delicate
aspects of particle propagation. Strictly speaking, such consideration
is safe when the scale of the background exceeds the particle's
Compton wavelength -- what is hardly true for
MBH and MTM, created in high-energy collisions (though one of the
two parameters of the MTM -- duration $T$ -- can actually be large).
We {\it assume} that qualitative effects can still be evaluated
in above ``approximation", like it is assumed about the Hawking
radiation of MBH, but more justification is needed here.

Surprisingly small is known about the testable properties of
time machines: most discussions seem to concentrate on philosophical
issues and not much is done in estimation (and even definition)
of concrete quantities.
In the rest of this paper, we try to list possible qualitative effects
in particle physics that could be of interest for further
quantitative investigation.

\section{Basic assumptions \label{s2}}

\subsection{On MTM-induced corrections to scattering probabilities}

In quantum theory of fields $\phi(t,\vec x)$ the mini-time-machines
modify probabilities of scattering processes in the following way:
\ba
\sum_{\rm over\ geometries}
\rho_{\rm geometry}
\left|\big< \phi(t_1,\vec x_1)\ldots \phi(t_n,\vec x_n)
\big>_{\rm geometry}\right|^2
\label{f0}
\ea
This formula
reflects the fact that the story is about {\it classical}
gravity: only matter fields are quantum, and no interference is
considered between different geometries, say, between mini-time-machines
with different duration of time loops.

\subsection{On probability of MTM creation in particle collisions}

The probability $\rho_{\rm geometry}$ of given geometry to contribute
characterizes the probability to the corresponding object
(mini-\-black-\-hole, mini-\-black-\-ring, mini-\-time-\-machine etc)
to be created at accelerator (or in cosmic ray event) at energy ${\cal E}$.
Like in the mini-\-black-\-hole case we assume that this probability is
basically defined by the geometrical size ${\cal R}$ of the object
(Schwarzschild radius or a size of the time-machine mouth) and the threshold
energy ${\cal E}_{threshold}$:
\ba
\rho_{\rm geometry} \sim
{\cal R}^2\theta\left({\cal E} - {\cal E}_{threshold}({\cal R})\right),
\label{crepro}
\ea
where $\theta(x)$ is the Heaviside step-function. Of course this is a
disputable formula (``chronology protection principle", if true, would simply
put $\rho$ for time-machines equal zero, and even the analogue of this
formula for mini-black-holes caused long discussion
\cite{mbhcs}), but we just state
that at the moment nothing forbids one to {\it assume} that (\ref{crepro})
{\it can} be adequate. It just reflects the assumption that mini-time-machines
can be created {\it classically} in particle collisions,
with no quantum damping (which would characterize {\it quantum} creation of a
{\it coherent} classical, i.e. consisting of {\it many} particles,
object from {\it a few} colliding particles) and the obvious existence of some
minimal energy needed for strong deformations of flat space-time to occur.
As known from considerations of {MBH}%{mini-\-black-\-hole}, the cross-section (\ref{crepro}) with
${\cal R}$ and ${\cal E}_{threshold}({\cal R}) \sim {\cal R}m^2_{Pl}$,
allowed by TeV-gravity models (i.e. with $m_{Pl} \sim 1\div 10\ {\rm TeV}$),
is enough to make LHC a {\it factory}, producing an {MBH}%{mini-\-black-\-hole}\ every second,
and we can imagine that the rate of {MTM}%{mini-\-time-\-machine}\ production can be comparably high.
This feeling that time machines are often associated with the black holes,
so that the probabilities of their existence can be indeed comparable,
both in the Universe and in accelerator processes, starts to get some support
in the general-relativity literature of the last years \cite{tmbh}.
Of course, there is a more delicate dependence on the parameters of MTM}%{mini-\-time-\-machine\
 in the proportionality coefficient, implied in (\ref{crepro}), and it is
important for any kind of numerical and even qualitative estimates, but it
is hard to evaluate without addressing concrete models of MTM}%{mini-\-time-\-machine.

\subsection{\label{mtmg} On MTM geometries}

A typical example of time-machine geometry is
obtained by cutting two $4d$ balls out of Minkowski space and identifying
(gluing) the boundaries of emerged holes (``mouths"). If one of the balls is inside
the light-cone of another, we obtain a time-machine Wheeler's wormhole, see Fig.1
(otherwise it would be a Wheeler's wormhole with no closed time-like curves).
This particular construction of the space with closed time-like curves
was originally proposed in \cite{Deu,Pol1}.
As seen from Fig.1 the MTM has two essentially different parameters:
the size of the mouth (length of the cut) ${\cal R}$ and duration
(distance between
the cuts) $T$. Note that in (\ref{crepro}) we assume that in the first
approximation the probability of MTM creation does not depend on $T$, in
particular large $T$ may not be damped as strongly as large ${\cal R}$, and
$T$ can essentially exceed
${\cal R} \sim {\cal E}/m_{Pl}^2
$.
This is a disputable assumption, but it is supported by some studies of
time machines in general relativity, implying that $T$ is indeed a soft
(nearly zero-) mode (even negative in same cases) of the time machine solutions
\cite{tzm,tmbh}.

Another popular
construction of the time-machine is a traversable wormhole suggested in
\cite{Th}, see also \cite{whole}. Important addition to Fig.1 is a tube,
connecting the balls boundaries (instead of gluing them directly,
as in Fig.1), and appearance of a new parameter: time-loop duration $T$
can generically exceed the time-machine time-life $\cal T$.
On a general class of wormhole geometries, see \cite{genwh}; on the stability
of wormholes, see \cite{morewh}; on the gravitating matter creating wormholes, see
\cite{kdv}; on rotating wormholes solutions which are presumably more stable, see
\cite{rwh}.
Other constructions of time machines can be found in \cite{tm}.
One can think about other ways to construct time-machine geometries.
We do not discuss classification of time-machine
geometries and their differences, example of Fig.1,
sometime with addition of additional parameter $T \geq {\cal T}$  will be sufficient
for our purpose of listing some interesting phenomena in particle physics,
induced by the presence of time-machines.

\begin{figure}[ht]
\epsfxsize 450pt
\begin{center}
\epsffile{fig1abt.eps}
\end{center}
\caption{\footnotesize A time-machine wormhole, represented by flat space
with cuts (with their sides appropriately identified).
The second picture shows topology of emerged space
(geometrically it can still be flat almost everywhere).
The tube in the second picture can easily change its width
far from its ends, and this allows to distinguish between the
characteristic time loop duration $T$ and the time-machine life-time
(in laboratory frame) ${\cal T}$. Both $T$ and ${\cal T}$ can be
soft modes and do not need to be restricted by collision energy as
strongly as the cut length (ball size) ${\cal R}$.}
\end{figure}

\subsection{On MTM evaporation (decay)}

If MTM contains strong gravitational fields and gravitational horizons,
they can lose energy by a direct analogue of the Hawking radiation
\cite{Kraeva}.
Remarkably, the same can be true if gravitational fields are small and no
event horizons\footnote{
Of course, a Cauchy horizon, separating the domain where initial
conditions at remote past
are not enough to fix the solutions of evolution equations
uniquely, is obligatory present in any time machine.
} are formed,
like in our flat-space-time wormhole in Fig.1.
Then time-machine's energy is fully carried by its "residents" --
particles, which move along closed world lines (or zero-modes of fields
in another formulation). Virtual-pair creation can produce an antiparticle
to annihilate any given resident, then the other element of the pair can
escape out of the time machine, thus forcing it to loose its residents
and thus the energy.
This process is possible because the finite size of the time machine
makes -- through quantum zero fluctuations -- the particles inside,
even in their classically stable ground states,
slightly more energetic than outside, what favors their escape,
whenever possible.
Properties of such evaporation should be, indeed, similar to the Hawking
radiation, in particular, it should also be thermal because of
uncertainty in the non-controllable state of the residents.

\subsection{On second quantization formalism: the key one for particle-theory
causality and unitarity}

Individual correlators in (\ref{f0}) can be represented in
two essentially different ways: in second and first quantization formalisms.
In the former case the correlator is given by a functional integral over
fields,
\ba
\int D\phi\ e^{iS\{\phi\}} \phi(t_1,\vec x_1)\ldots \phi(t_n,\vec x_n),
\label{f1}
\ea
and Feynman diagrams are made out of propagators, which are obtained
by solving Klein-Gordon and Dirac equations in the space with non-trivial
topology, like in Fig.1.
It is a non-trivial problem to find explicit expressions for
such functions, as everybody knows from the study of oversimplified
examples in electrostatics or in the theory of Riemann surfaces.
Even for Fig.1, and even for the case when spheres are deformed into
straight cuts and even in $2d$ instead of $4d$ it is quite a problem to
write an adequate Green function explicitly.\footnote{In $2d$ one
readily writes down a {\it Euclidean} Green function
$$\log \left(\vartheta(\Big|z-z'\Big|\tau)|^2
\exp\pi\frac{{\rm Im}(z-z')^2}{{\rm Im}\ \tau} \right) + {\rm
contribution\ of\ the\ {zero-mode} }$$ with $\tau$ in the argument
of Jacobi theta-function defined through the ratio $T/{\cal R}$ and
$$
z\equiv\int^x \frac{dx}{\sqrt{\left(x^2-{R^2+T^2\over 4}\right)^2+T^2x^2}}
$$
is obtained by the Jacobi map.
However, this formula actually describes a Green function after
compactification of a plane to $CP^1$ and can not be directly used
for analytical continuation into non-compact Minkowski space with appropriate
boundary conditions. } If known, such expressions could be used to
somehow extract the commutators\footnote{For example, the
equal-time commutator for $t'=t$ can be found with the help of the
BJL theorem \cite{BDL}: picking up the coefficient in front of
$\omega^{-1}$ after Fourier transformation in time direction.
However, even in this case there can be problems with making Fourier
transformation in time-machine geometry, where the time $t$ is not
globally defined.} $\Big< [\phi(x,t),
\phi(x',t')]\Big>$ and check if they vanish outside the light-cone
-- and thus study the naive particle-physics causality in the
time-machine geometry. Unfortunately, because of problems with
explicit expressions, not much can be done with the
causality-related problems in the second quantization formalism.

\subsection{On first-quantization formalism}

The first-quantization formalism is much better suited to study
(counter-)intuitive problems. It represents propagators as sums over
all {\it possible} world-lines of a particle in the space-time, leading from
initial to the final point. Interactions are taken into account by
forming usual Feynman diagrams out of these propagators.
A non-trivial problem, however, arises with what are ``possible"
world-lines in Minkowski space-time.
In non-relativistic quantum mechanics \cite{FH} the sum is over all world
lines of the type $\vec x(t)$ with $-\infty < x_j(t) < +\infty$ and
$t_i< t < t_f$ and $\vec x(t_i) = \vec x_i$, $\vec x(t_f) = \vec x_f$,
i.e. one allows classical equations of motion to be broken, but
time-ordering is preserved.
In relativistic situation where the typical particle action is
$S\{\vec x(t)\} = m\int \sqrt{1 - \dot{\vec x}^2}dt$, one can impose
additional constraint $\left|\dot{\vec x}\right| \leq 1$ -- particles
can not travel faster than light. The sum over world-lines with
this restriction would provide the ``causal particle propagator"
\ba
g(\vec x_f,t_f|\vec x_i,t_i) =
\int \left\{D\vec x(t)
\prod_{t=t_i}^{t_f} \theta\left(1-\dot{\vec x}^2\right)\right\}
\exp\left(
im \int_{t_i}^{t_f} \sqrt{1 - \dot{\vec x}^2}dt\right)
\label{cpp}
\ea
-- an obviously causal quantity in Minkowski space.
However, for geometrical intuition
this object does not look very natural if space and time are to be treated
on equal footing. From that point of view, instead of  summing over all
functions $\vec x(t)$ in (\ref{cpp}) one would rather sum over all
curves $\vec x(s), t(s)$ in the space time. The difference is two-fold,
see Fig.2:
first, not all curves are inverse images of projections onto the time
segments $(t_i,t_f)$; second, not all curves satisfy the restriction
that velocities never exceed unity (the speed of light).
\begin{figure}[ht]
\epsfxsize 350pt
\begin{center}
\epsffile{fig6t.eps}
\end{center}
\caption{\footnotesize
Difference between a particle world line (a), generic path (b)
and a singular path (c), implied in the definition of Feynman propagator.
The last one consists of pieces, which look like particle/antiparticle
world lines, i.e. belong everywhere to the light cones,
are invertibly projected on the time axis and projection
preserves/inverts the direction.}
\end{figure}
The latter subject is in fact a delicate one, related to analytical
continuations and other peculiarities of Polyakov's method
to handle non-polynomial actions \cite{Poly},
while the former difference is taken into account by
composition of any space-time curve from a sequence of well-projectable
fragments, going along and backwards in time. The full integral over
all curves -- the Feynman's propagator $G(\vec x_f,t_f|\vec x_i,t_i)$ --
is a multi-linear  combination of $g$ and $\bar g$, interpreted as
propagators of particles and anti-particles \cite{FAP}, depending on
the sign of $dt/ds$:
\ba
G(\vec x_f,t_f|\vec x_i,t_i)=g(\vec x_f,t_f|\vec x_i,t_i)+
\int_{|\vec x_f-\vec x|\le t_f-t,\ |\vec x_i-\vec x|\le t-t_i}
\bar g(\vec x_f,t_f|\vec x,t) g(\vec x,t|\vec x_i,t_i)+\ldots
\ea

\begin{figure}[ht]
\epsfxsize 300pt
\begin{center}
\epsffile{fig5t.eps}
\end{center}
\caption{\footnotesize A typical contribution to the Feynman "propagator"
outside the light-cone. Both particle and antiparticle travel inside
their light cones and no causality violation takes place. However, this
{\it correlator} does not describe {\it propagation} of any physical entity:
it is instead an amplitude to create and annihilate a pair.
This obvious fact makes interpretation of amplitudes (especially, the loop
diagrams), evaluated with the help of Feynman propagators somewhat tricky.
}
\end{figure}

As clear from Fig.3, the Feynman ``propagator" does not
vanish outside the light-cone (still, and
somewhat ironical, it is often called ``causal"), and does not need to vanish,
see, e.g., \cite{props}. Better understanding of
these problems seem important for clarification of physics of time machines,
and they seem to remain under-investigated.

\section{Particles in time-machine}

The typical world-line of a particle, traveling through time machine
of Fig.1 is shown in Fig.4.

\begin{figure}[ht]
\epsfxsize 450pt
\begin{center}
\epsffile{fig3abt.eps}
\end{center}
\caption{\footnotesize A particle, traveling $n=3$ times through a time machine
with the time loop of length $T$. In the left-side picture also two
photons are shown, radiated by the particle. The one which escapes
immediately after being emitted looks for a distant observer as coming
from the place where no particle was present and can cause
non-locality of effective theory.}
\end{figure}

It passes $n$ times through the time-machine and finally escapes.
In laboratory frame all $n$ walks do not take any time, but in the
particle's own frame the situation is different: $nT$ units of its
proper time pass before it escapes. If the particle could decay or
radiate (in Fig.4 the radiation case is shown), it was doing so
during all its life in time-machine and comes out much older
-- by $nT$ -- than its twin particle, which never was in the time
machine (note, that
in special relativity, the traveling twin returns younger than the one
who stayed at home, but in the case of time machine, as well as of
a travel in strong gravitational field, things are different:
the traveler gets older). We now list some effects obvious from Fig.4,
together with their possible implications for observations.
In every case it is important to figure out, whether an
effect can occur

-- without any gravitational effects,

-- also in the presence of {MBH}%{mini-\-black-\-hole},

-- in presence of any kind of wormholes (i.e. effect does not distinguish between
space- and time-like wormholes),

-- only for time-machine geometries.

\subsection{Frequency filtration}

The field, describing a particle with frequency $\omega$, acquires
a phase factor $e^{i\omega T}$ every time it makes a cycle along
the time loop of duration $T$ in time machine. After $n$ cycles
the wave function will be proportional to
$$
\sum_{k=0}^n e^{ik\omega T}
\longrightarrow \sum_m \delta\left(\omega - \frac{2\pi m}{T}\right)
$$
for large enough $n$. Of course, one should take into account the
space-dependence of the wave function, but the phenomenon is already
clear from above oversimplified formula: original frequency spectrum
at the entrance into the time-machine is re-shaped, mostly
frequencies which are integer multiples of $\frac{2\pi}{T}$ will
penetrate through the time machine. This frequency filtration
implies that gravitational effects can modify the original
spectra of particles, calculated in neglect of them. Actually, such
modifications are caused both by {MTM}%{mini-\-time-\-machine}s and {MBH}%{mini-\-black-\-hole}s. Though
effect of particular MTM}%{mini-\-time-\-machine\ is quite specific: frequency filtration
(and nothing equally specific would be caused by particular MBH}%{mini-\-black-\-hole),
it is obscured by averaging over various time-loop durations $T$ in
formula (1).

\subsection{Unexpectedly energetic particles}

It was noted in \cite{Haw} that the gravitational field
in a time machine could provide a particle\footnote{In \cite{Haw} it was
a photon traveling along the first closed null-curve to come into existence
as the time-machine is formed. This photon is blue-shifted every time
it makes a closed loop inside the time machine. See also \cite{Kras}.
}
with additional energy each time it passes through the time machine,
so that it can acquire a lot during a period of time which is nearly
zero in laboratory frame. This would
cause another peculiar type of modification of spectrum,
providing some particles with a large excess of energy at expense
of the other particles:
the latter are produced in evaporation of the MTM, which
lost part of its gravitational energy to acceleration of the former.
This effect is again specific
for time machines (as compared to the MBH}%{mini-\-black-\-hole\ and space-like wormholes),
but again, since
spectrum modification involves a lot of averaging, it can be not
too pronounced in actual experiments.

As usual, one should add a word of caution.
Already in \cite{Haw} it was argued, that the time machines
with accelerating ability can be not observable for one or another reason
(they can decouple from our universe or instead quickly renormalize the
accelerating gravitational field down to zero).
Furthermore, in \cite{Haw} it was noted that the geometry in a tube region
around the closed curved acts as ``a diverging lens" \cite{viss},
which disperses {\it energy}, even if it concentrates the {\it energy density}.
Thus, if a point particle is substituted by a wave packet, its total
energy can actually decrease instead of increasing.
According to \cite{Haw} this is indeed the case for the wormholes of \cite{Th}.
A more careful analysis for (quantum) point-like particles is still needed.

\subsection{Accelerated aging, intensification of decay and oscillation
 processes}

If a particle travels $n$ times along a time loop of duration $T$, its
proper-time (age) exceeds the laboratory time by $nT$.
This means that from the point of view of laboratory observer such
particle ages much faster than it would in the absence of time machine.
In particular, if the particle decays and probability of its existence
decreases as $e^{-\Gamma t}$, the presence of time-machine seemingly
accelerates the decay for the outside observer:
$e^{-\Gamma t} \longrightarrow e^{-\Gamma (t+nT)}$.
Note that $nT$ can considerably exceed the characteristic time ${\cal T}$
of evaporation of mini-time-machine (which can be smaller than $10^{-28}$ s
for MTM possibly created at LHC and is negligible as compared to life-time
of all ordinary particles), both because $T$ can be much greater
than ${\cal T}$ and because $n$ can be large.

Similar phenomenon will take place with the loss of energy due to
radiation. As shown in Fig.4, the radiated photons can have
different fates -- they can escape from the time machine immediately
or can continue to make time loops in it,-- this does not affect the
radiation rate of original particle. Other effects, related to the
age of particles, like kaon or neutrino oscillations will also be
seemingly accelerated in the presence of MTM.

\subsection{Effective non-locality, possible $CPT$ and unitarity
violation}

As shown in Fig.4, a photon, emitted by a particle when it was
traveling inside the time machine, can escape, but its emission
point will have nothing to do with that of the escaping particle itself
(if escaping photon was emitted not at the last, but at some
intermediate travel of the particle along the time loop, and if
we notice that trajectories of these travels in space can differ
from time to time -- as shown in Fig.4).
This means that from the point of view of external observer
a kind of non-local emission of photon took place: a potentially
non-local effective interaction is generated by time machine.
This opens a room for $CPT$-violation, though more detailed
analysis is needed to decide whether it can indeed be caused by
{MTM}%{mini-\-time-\-machine}\ (see also \cite{HawH} for a toy two-dimensional model discussion
of the issue)\footnote{For possible CPT violation effects due to non-trivial topology
see, e.g., a recent paper \cite{Klin} and references therein.}.

Naive unitarity violation in time-machine geometries
is considered very probable \cite{unit}, because of
existence of the Jinnee-type world histories \cite{LN}, shown in Fig.5,
which are not fully controlled by initial conditions at remote past
and should be somehow averaged over.
Of course, after evaporation of MTM the {\it formal} unitarity
should be recovered,
like it happens in the case of evaporating black holes \cite{evabh}
(or molecular theory).
However, physically relevant thermalization-style effects
remain and can probably be observed.

\begin{figure
\epsfxsize 500pt
\begin{center}
\epsffile{fig8abct.eps}
\end{center}
\caption{\footnotesize Encounters of external particle with
the ``residents" of the time machine,
nicknamed "Jinn" in ref.\cite{LN}. They can interfere with
the incoming and outgoing particles and are well observable, but
they are not controlled by specification of {\it in} or {\it out}
states, what requires a more accurate formulation of unitarity
when particle theory is considered in the time-machine geometries.
{\bf (a)} Vertical lines (classically unobservable Jinn-at-rest)
can be added in any number at any place of
the cuts. This represents the ambiguity in the world-history of a
particle traveling through the time machine. In the picture it is
assumed that particles interact as in central collisions of tiny balls:
they exchange momentum and energy in every act of interaction.
{\bf (b)} A non-trivial meeting with Jinnee.
Encounter with the Jinnee is not controlled by the initial
condition at remote past.
One and the same pattern (which contributes exactly once to
the functional integral) allows different {\it interpretations}:
one can say that a particle gets through the time-machine without
interaction with the Jinnee living inside or that a particle itself
passes along a time-loop inside time machine and escapes, with
changes in its motion, caused by self-interaction.
{\bf (c)} Here the aging (dissipating) Jinnee is shown: as time goes,
our particle can radiate (or decay or dissipate energy in other ways).
The remaining kinetic energy and thus the age of the particle is
characterized by the angle between the world line and time-axis.
It is clear from the picture that as result of encounter with the
Jinnee the particle becomes older -- in accordance with the second
interpretation in (b): that it have spent extra proper time inside
the time machine.
The typical (proper-time) history of a "wild" Jinnee is as follows
(see \cite{LN} for discussion of artificially created Jinn).
Radiation can cause incoming particle to be trapped inside the
time machine and become a Jinnee. After that the aging Jinnee looses
energy and becomes sterile Jinnee-at-rest, which has no more energy
to loose and can no longer radiate. Still, since the energy of
resting Jinnee can exceed its mass due to zero-fluctuation effects
in the time-machine of a finite size, the quantum
interaction with virtual pairs can allow the Jinnee to escape:
this effect contributes to quantum evaporation of time-machines
(gravitational fields, if any, can also be considered as a sort of
Jinn).
}
\end{figure}

\subsection{Collective effects}

Fig.4 shows that a time-machine converts, at some stages of
evolution, a single particle into an ensemble of co-existing
particles. Moreover, the particles in the ensemble are copies and
thus are strongly correlated. This opens a room for various
collective effects to occur, if interaction is taken into account,
up to bose-condensation, superfluidity and superconductivity of
copies inside the time-machine. Since phase transitions may affect
the behavior of particles, including, say, their decay rates and
radiation distributions, they may affect the outcome of particle
collisions. This kind of collective effects, caused by cloning of a
single particle, seems to be absolutely peculiar for time machines.

\subsection{Extra production of antiparticles at intermediate stage}

As clear from the presentation of wormhole geometry in the right-hand-parts
of Figs.1 and 4, while traveling through the time-machine, a probe particle
will sometime move
backwards in time from the point of view of the laboratory frame.
Probably, at this part of its history it can be considered as
antiparticle. In other words, the {MTM}%{mini-\-time-\-machine}\ seem to temporarily
convert particles into antiparticles, however, as clear from Fig.6,
for external observer the decay products of {\it these} antiparticles are
indistinguishable from those of original particles, at least in the
theory without CP-violation. Thus, experimental consequences of temporal
presence of antiparticles are obscure.

\begin{figure}[ht]
\epsfxsize 400pt
\begin{center}
\epsffile{fig7t.eps}
\end{center}
\caption{\footnotesize
Irrespective of time-directions in which the particle $A$
can move inside a time-machine (and its possible conversion into
anti-particle $\bar A$), the observer at remote future will see
only $B$ and $C$ (and not $\bar B$ or $\bar C$) in the products
of $A$ decay.
{\bf (a)} A particle $A$ can emit $B$ and turn into $C$.
{\bf (b)} When moving backwards in time, $C$ looks like a normally moving
anti-particle $\bar C$, which turns into $\bar A$ after collision with
$\bar B$.
{\bf (c)} Alternatively, $\bar C$ can convert into $\bar A$ by emission of
$B$.}
\end{figure}

If $CP$ is violated, a more interesting
question arises: antiparticles should have
coupling constants, which are complex conjugate of their particle's
counterparts ($CP$-violating mass terms, e.g.
$i\mu(K_0^2-\bar K_0^2)$ as opposed to the ordinary $m^2K_0\bar K_0$,
are usually considered as additional valence-two vertices in
Feynman diagrams).
In the first quantization formalism this means that
when moving backwards in time the particle should have different
parameters. Such abrupt change is not a problem in the formalism,
involving singular paths of Fig.3c, where world lines of
particles and antiparticles lie inside light cones and are well
separated. However, adequate description in terms of
smoothly $U$-turning paths of
Fig.3b is less obvious. In Fig.4, associated with the time-machine
geometry, the light-cone is {\it smoothly}
turning upside down along the world line, what resembles the
``geometric" Fig.3b, rather than ``physical" Fig.3c.
All this means that the story
of geometrical first-quantized formulation of theories with
CP-violation and, in particular, the problem of
particle-antiparticle conversion in MTM is somewhat obscure and
deserves further investigation.

\section{Conclusion}

No question, the statements in the previous sections and even their mutual
compatibility are disputable or at
least require a lot of comments and justification.
However, attempts to make above naive arguments more rigorous would take
us back to controversial discussion of time-machine physics, which we
suggested to avoid in the Introduction.
Instead, as we suggested, one can try to make equally naive estimates
of the values of above effects, assuming that -- for one or another reason --
they can avoid the existing or the future counter-arguments and still show up
in physical experiments.
Of principal importance for reliable estimates is deeper understanding
of the issues, mentioned in s.\ref{s2}.

\section*{Note added}

 This paper concerns a subject which lies
at the intersection of two controversial subjects: time-machines in
general relativity and low-energy quantum gravity. Recent paper
\cite{AV} raises the same kind of questions, and we decided to put
this old paper to the ArXiv in order to contribute to the
discussion. References have not been updated since 2005 and we
apologize for non-indicating many new contributions to particular
subjects mentioned in the text.

\section*{Acknowledgements}

We are grateful to T.Mironova for help in making figures.
This work was supported in part by the EU under the RTN contract
MRTN-CT-2004-512194.
The A.M.s acknowledge the support of two NATO travel grants and
the hospitality of the Department of Physics of the University of Crete, where
this work was done.
Our work is partly supported by the Federal Program of the
Russian Ministry of Industry, Science and Technology No
40.052.1.1.1112, by Russian Federal Agency of Atomic Enery, by the grants RFBR
04-02-16538a (Mironov), RFBR 04-02-16880 (Morozov), by the Grant of
Support for the Scientific Schools 8004.2006.2, NWO project
047.011.2004.026, INTAS grant 05-1000008-7865
and ANR-05-BLAN-0029-01 project.

redpajama_set_name: RedPajamaArXiv


text:
ACP - Delete forum category

{{Session::get('message')}}

Are you sure you wish to delete the forum category "{{$category->name}}"?

This will delete all forums, topics and replies the category contains.

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<input type="submit" value="Delete" /> or {{HTML::link('admin/forums_manage', 'Cancel')}}

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redpajama_set_name: RedPajamaGithub


conair home pollenex solid teak roll up folding shower spa may function as intelligent way to decorate your own floor . however, it still has got the role. You will find many approaches in which you are able to try to do to be able to embellish your floor with out have to bring the extra decorator. Check this out. Only piling the towels are sometimes a wonderful notion. But obviously it does not necessarily mean that you can stack them . It is fantastic to offer a towel rack using glass onto the do or close to the sink and sink area. This really is simple-yet assisting one to deal with your floor look.
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Under Armour's first wristband tracker may not be revolutionary, but it offers decent insight and feedback on your workouts and progress.
Mjuk kant, fasar in i en metalldetalj.
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You know what's more accurate than one fitness device?? Two of them! Biostrap's approach to fitness tracking is two-fold, with their wrist-worn band and their shoe-clip, working in unison to track your activities and gauge correctly the amount of energy expended. The two devices track your entire body's movements, while the Biostrap is programmed to record and track any sort of repetitive exercise. BUY NOW!
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Coyote Valley Elementary would like to recognize Janet Campbell as the number one classified employee for the 2011-12 school year. Mrs. Campbell serves as a special education para-professional aide supporting students in the Coyote Valley resource program. Resource teacher, Mr. Mannisto, has been described by parents as a "magician" in helping students. If Mr. Mannisto were a magician, then Mrs. Campbell would certainly be considered a magician's assistant.
Mrs. Campbell performs her "magic" through her uniform and calm approach with children. She is a dedicated employee that can be relied upon to show up daily and provide consistent instructional support to students that generally benefit from routine, predictability and patience.
Mrs. Campbell works with students ranging from 1st to 6th grade and has the ability to quickly shift gears to work with different aged children as well as different grade level standards that range from adding two one-digit numbers to determining the variable in a mathematically expression involving fractions.
Mr. Mannisto shares that Janet has a keen sense of where and when to assist students with special needs without hovering or enabling. She has strong academic skills, has a straight-forward approach and her consistent support, positive feedback, kind and compassionate nature greatly enhance the education of the students she serves.
Congratulations to Mrs. Campbell for this well deserved honor. We appreciate all you do.


text:
Tweaking Diatoms For Nanofabrication Duties
by Kate Melville
Diatoms, tiny phytoplankton that encase themselves in intricately patterned shells, could represent the next big breakthrough in computer chip fabrication, say scientists from the University of Wisconsin-Madison.
Diatoms build their hard cell walls by laying down submicron-sized lines of silica, a compound related to the key material of the semiconductor industry - silicon. "If we can genetically control that process, we would have a whole new way of performing the nanofabrication used to make computer chips," says Michael Sussman, a University of Wisconsin-Madison biochemistry professor.
Reporting their findings in the Proceedings of the National Academy of Sciences, a team led by Sussman and diatom expert Virginia Armbrust of the University of Washington have identified a set of 75 genes specifically involved in silica bioprocessing in the diatom Thalassiosira pseudonana. Armbrust, an oceanography professor who studies the ecological role of diatoms, headed up the effort to sequence the genome of T. pseudonana in 2004.
The new data will enable Sussman to start manipulating the genes responsible for silica production and potentially harness them to produce lines on computer chips. This could vastly increase chip speed as diatoms are capable of producing lines much smaller than current technology allows.
"The semiconductor industry has been able to double the density of transistors on computer chips every few years. They've been doing that using photolithographic techniques for the past 30 years," explained Sussman. "But they are actually hitting a wall now because they're getting down to the resolution of visible light."
To determine which genes are involved in creating the distinctive patterns in diatoms, the research team used a DNA chip developed by Sussman, UW-Madison electrical engineer Franco Cerrina and UW-Madison geneticist Fred Blattner. The chip allows scientists to see which genes are involved in a given cellular process. In this case, the chip identified genes that responded when diatoms were grown in low levels of silicic acid, the raw material they use to make silica.
Of the 30 genes that increased their expression the most during silicic acid starvation, 25 are completely new, displaying no similarities to known genes. "Now we know which of the organism's 13,000 genes are most likely to be involved in silica bioprocessing. Now we can zero in on those top 30 genes and start genetically manipulating them and see what happens," said Sussman.
IBM Demos Self-Assembling Chip Turbocharger
Nanomaterial Error-Correction Process Mimics Nature
Radical Transistor Design Blasts Single Electrons Through Circuits
Nano-Imprinting Promises Even Smaller Electronics
DNA Creates Self-Assembling Nano-Transistor
Source: University of Wisconsin-Madison


These licenses are only for customers who have previously purchased DiffEngineX within the last three years and wish to upgrade to the latest version.
You are only entitled to one current upgrade license for every previous license you have purchased.
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at $50 USD per single user license (PayPal).
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text:
Q: Analyzing the behavior of a threaded program Is there an application that will do what Threadscope or the parallel tools of Visual Studio does for multithreaded program analysis in Linux?

A: There are many tools. Intel VTune Amplifier (formerly VTune Performance Analyzer), Oracle Solaris Studio for RedHat Linux includes visual Thread Analyzer. And a number of tools were mentioned in this Stackoverflow thread or this thread.
Many of the available profiling tools can be accessed via Eclipse Linux Tools project.

redpajama_set_name: RedPajamaStackExchange


Discussion in 'Google TV News' started by dandroid, Mar 22, 2017.
All Android TV devices come with a remote control, but those things do have a way of getting lost in the couch cushions. Luckily, your phone can connect to the TV box and act as a remote. Not as luckily, that can sometimes be buggy. Maybe it'll be a little less so going forward now that the remote service is being updated via the Play Store.


text:
class SharedMimeInfo < Formula
  desc "Database of common MIME types"
  homepage "https://wiki.freedesktop.org/www/Software/shared-mime-info"
  url "https://gitlab.freedesktop.org/xdg/shared-mime-info/uploads/b27eb88e4155d8fccb8bb3cd12025d5b/shared-mime-info-1.15.tar.xz"
  sha256 "f482b027437c99e53b81037a9843fccd549243fd52145d016e9c7174a4f5db90"

  bottle do
    cellar :any
    sha256 "137dfd734f5e7fe9b9ee80d1efa135f95a3ade95ceab83b2f79cd7ca1fd4d313" => :catalina
    sha256 "1be57687d8aef14d6bc95be0a02a5dfdbce4bf859ea057c93e3ff8545c700fcd" => :mojave
    sha256 "87ec03b8d25d6c3c455c98dbc8d9ac3569df6abaae0c07ad9444a1cfa462cd06" => :high_sierra
  end

  head do
    url "https://gitlab.freedesktop.org/xdg/shared-mime-info.git"
    depends_on "autoconf" => :build
    depends_on "automake" => :build
    depends_on "intltool" => :build
  end

  depends_on "intltool" => :build
  depends_on "itstool" => :build
  depends_on "pkg-config" => :build
  depends_on "gettext"
  depends_on "glib"

  def install
    # Disable the post-install update-mimedb due to crash
    args = %W[
      --disable-dependency-tracking
      --prefix=#{prefix}
      --disable-update-mimedb
    ]
    if build.head?
      system "./autogen.sh", *args
    else
      system "./configure", *args
    end
    system "make", "install"
    pkgshare.install share/"mime/packages"
    rmdir share/"mime"
  end

  def post_install
    global_mime = HOMEBREW_PREFIX/"share/mime"
    cellar_mime = share/"mime"

    if !cellar_mime.exist? || !cellar_mime.symlink?
      rm_rf cellar_mime
      ln_sf global_mime, cellar_mime
    end

    (global_mime/"packages").mkpath
    cp (pkgshare/"packages").children, global_mime/"packages"

    system bin/"update-mime-database", global_mime
  end

  test do
    cp_r share/"mime", testpath
    system bin/"update-mime-database", testpath/"mime"
  end
end


text:
Bio Details
Amit D. Munshi, MBA
Amit D. Munshi is Director, President and Chief Executive Officer of San Diego based Arena Pharma since May 2016. Previously, Amit served as President and Chief Executive Officer of Epirus Biopharmaceuticals, Inc. and Percivia LLC, a biotechnology company (sold to JNJ). Prior to Epirus and Percivia, he was a co-founder and served as Chief Business Officer of Kythera Biopharmaceuticals, Inc., from 2005 to 2010, (sold $2.1B to AGN) and held multiple leadership positions at Amgen Inc. from 1997 to 2005, including General Manager, Nephrology Europe. Amit holds a B.S. in Economics and a B.A. in History from the University of California, Riverside, and an M.B.A. from the Peter F. Drucker School of Management at Claremont Graduate University. He has more than 30 years of global biopharmaceutical industry experience in executive management, business development, product development and portfolio management. Amit currently serves on the boards of Pulmatrix, Inc. (Nasdaq: PULM) and Enterprise Therapeutics Ltd, and also serves as an advisor and lecturer at the Peter F. Drucker School of Management at the Claremont Graduate School.
Member of the Audit Committee


Sixteen years ago, the Guggenheim Museum shocked the Manhattan art world with an enormous exhibition titled The Art of the Motorcycle.Critics scoffed, but it pulled in big crowds. Not even King Tut had an edge on the bespoke machines. This interest in vintage iron doesn't seem surprising today, particularly with the growing popularity of local events like Caffeine & Carburetors in New Canaan, where hundreds of automotive enthusiasts gather to indulge their inner gear head. But before there were spectators, there were collectors. Across our towns, there are countless obsessives who comb the county for that magneto spring that will bring the old flivver to life again.
And ride he does. Earlier this year, Kanter, Pat Simmons—founder of the Doobie Brothers band—and Pat's wife, Cris, did a cross-country Cannonball jaunt on some glorious old bikes. Kanter's 1936 Harley-Davidson VLH was the newbie machine. Surgery and rehab were constant during the trip, but the riders finished it grinning.
After he hung up his racing leathers, Kanter found more time to work at his parents' business, Penny Press in Norwalk, a publisher of crossword-puzzle magazines. He also attended the University of New Haven, where he earned a master's degree. For his 1989 thesis, he started a bike-gear classified listing called Old Bike Journal. That led to his present operation, TAM Communications. In his office is a rack of ancient Harley engines, which, cleaned and painted, look like Babylonian artifacts. A 1915 Harley he calls Selma is parked here, along with a vintage Italian make and a distinguished oddball called the Airone, which occupies one corner.
Fairfield County, he knows, is a hotbed of collectors. "I have several friends into vintage machines," he says. "There's a group of us who meet every Sunday at Blind Charlie's Café in Scotts Corners [in Pound Ridge, New York]. Twenty or thirty bikes show up." Some machines are the latest and fastest. And then there are guys like Kanter who show up with a Ducati 250, a slower machine but still a jewel to anyone who recognizes the beauty of its wonderfully finned engine. Kanter prefers a more sedate pace on runs into the hills with the Blind Charlie's gang. More ambitious are the MotoGiro events, two-day competitions on old bikes running at legal speeds along New England's back roads. "I started racing again, after thirty years," Kanter admits.
His snarling race bike of choice? A 1937 Indian, purchased at an auction. After restoring it, Kanter took it to vintage races in New Hampshire. "I had mechanical problems all three times," he says with a wide smile. Nobody knows if loving the old machines is to love wisely, but if you love classic motorcycles, you love well.


Decided to take a jaunt out in the 911 and saw a lovely GT2 with upgrade to 997.2/GT2RS rear. Looked a treat. Anyone know it?
Ridders was test driving it.
I'm surprised anyone changed to the RS rear. The GT2 rear bumper looked great to me.


text:
FEATURED PETITION
Signature Goal
2 out of 1,000
Deadline has been reached.
Signatures are no longer accepted. This petition is now closed.
Pamela Hennes 1 petition
Petition Info
Type: Members
Item: Pamela Hennes
Goal: 1,000 signatures
Deadline: September 1, 2016 2:00 AM EDT
Category: Environment & Wildlife
#Cumberland Plateau #Crab Orchard #Apex #Cumberland County #Wind Farm #Government Subsidies
Cumberland Mountain Preservation Coalition is not about politics. The Coalition's main concern is the HEALTH of the people in Crab Orchard and surrounding area.
Petition Statistics
Created By: Pamela Hennes
2 signatures
Petition Home Page »
Browse Petitions »
Stop the Industrial Wind Farm in Crab Orchard, TN
Target: Apex Clean Energy, Inc.
Sponsored By: Cumberland Mountian Preservation Coalition
Petition Comment
In January 2016, Apex Clean Energy announced that it would spoil the beauty of the Cumberland Plateau; erecting 23 wind turbines more than 650' high. Research recently completed in the Cumberland County Register's Office indicates the origional 7,000 acres controlled by Apex Energy is more like 16,000 acres that includes land in 2 additional counties, making this area a possibility for one of the largest wind farms in the U.S.
TVA the source for electricity in TN has NO need for any power generated from the Crab Orchard Wind Farm. The Wind Industry i.e. Apex is the beneficiary of at least 5 major subsidies. 1. Federal Production Tax Credit. 2. Accelerated depreciation rules. 3. Federal Loan guarantees. 4. Renewable Energy Certificates. 5. State & local utility tax rebates. The construction of the wind farm in Crab Orchard is about $$$$ lots of it. Billions of dollars of wasteful federal taxpayer subsidies allow wind producers, in some markets, to give away wind power and still make a profit."
Fairfield Glade is a community next to Crab Orchard of over 1,800 homes, a Wyndam Time Share resort community incl. 14 golf courses; Crab Orchard/Crossville TN is known as the golf capital of Tennessee.
There is a large population of combat veterans from multiple wars that reside in the "Glade" that will be forced from their homes once the bombing...I mean blasting starts on the Plateau...30' down for each turbine erected. We have 2 schools where students will be affected by infra sound along with an aging community with existing hearing issues. Please help us stop APEX...sign our petition, visit our web site http://www.saveourcumberlandmountains.com and comment on our Facebook Page https://www.facebook.com/cumberlandmountainpreservation/?ref=aymt_homepage_panel Thank you for signing our petition.
Cumberland Mountain Preservation Coalition (CMPC) spoke to a packed house in Fairfield Glades Multi-Purpose building last Thursday afternoon. Much of the crowd was left standing and many people could not attend because the parking lot was full.
It was a barnburner of a meeting. There were posters showing the planned location of the Industrial Wind Farm on the Mountain ridge that separates Crab Orchard and Fairfield Glade residents.
The discussion focused on Apex Energy, an out of state company who has been planning this project for over two years. It is understood they plan to sell the energy to the highest bidder, not to Tennessee residents, which is what the Coalition were led to believe by a statement by their president.
Since many of Glade residents are from different areas of the country, they have seen projects like this before and lived in States that had WIND FARMS. They were able to educate folks on many of their concerns.
Many people commented that the county's they were from had ordinances or zoning regulations that required input from the residents, wildlife groups, and activist leaders so that they understand the full impact this would have on their community.
Many of the people who will live with these 650-foot Turbines felt betrayed that they were not given that opportunity by the County.
You could here a pin drop when a few of our residents from Illinois explained their experience living around these industrial turbines, the crowd listened intently to these ladies mimic the disturbing sounds that the turbines made while in operation.
George Chiaramonte, the CMPC Committee Chair began the meeting by introducing the mission statement of the recently formed coalition as an opposition group to the Crab Orchard project. It will research and gather information and report weekly to the residents of FFG and Cumberland County. Before the committee could even get under way the concerned residents started firing questions, Mr. Chiaramonte, for almost an hour answered questions and allowed comments from an electrified audience. It was obvious to everyone in attendance people were really upset.
Many comments were regarding the fact that Crab Orchard and Fairfield Glade residents were ignored and left out of the process for over two years.
Why weren't issues concerning our wildlife habitat, infrasound, shadow flicker, blinking lights at night and loss of property values being addressed by our local leaders?
Many questions are still going unanswered. Another key point made was why was APEX now acquiring leases for over 7,000 acres when their original project only called for 1,800 acres?
One person said: "This is a slap in the face by Cumberland County officials to all the residents in the area that will be affected. "
Has Apex found their "POT of Gold" right here in Cumberland County?
Address for Delivery of Petition Through USPS, FedEx or UPS P.O. Box 1974 · Crossville, TN 38558
Email Address for Electronic Delivery p.baetzel@gmail.com
City Crossville
State Tennessee
I fully support
by Samantha Jergen
When health is involved, I feel we must do everything possible to protect human life. Though I think wind turbines are an ok source for energy, if there is proof that people's health is at risk, then we must look at either moving it elsewhere or finding... moreWhen health is involved, I feel we must do everything possible to protect human life. Though I think wind turbines are an ok source for energy, if there is proof that people's health is at risk, then we must look at either moving it elsewhere or finding another solution.
I fully support this petition
by Nap-Sack ....