text:
Mayor welcomes freshmen Scots to promote David Douglas bond
Following the unique tradition there, incoming David Douglas High School freshmen are greeted by upper-class student mentors, teachers, and administrators. But see why, this year, Mayor Tom Potter was part of the welcoming committee …
Mayor Tom Potter and district superintendent Barbara Rommel join some of the Scot "Link Team", as they welcome, and gave the "wave", to the largest class in DDHS history.
At David Douglas High School, the "new kids in school" are cheered, not jeered, by a school-wide welcoming committee on Freshman Orientation Day.
But this year was different. Mayor Tom Potter was there also, joining in the welcome of the new students to the state's largest high school 'Äì a campus housing more students than many Oregon towns have population.
Sharing a light moment outside the school are DDHS Principal Randy Hutchinson, Mayor Tom Potter, and Superintendent Barbara K. Rommel.
We asked the Mayor why he came to outer East Portland early on this particular morning.
"I'm the Mayor of this school district, too," Potter told us, flashing a broad smile. "I'm here to draw the attention of East Portland people to the fact they have a great school district in David Douglas. And, I'm asking the people here to vote for ballot measure 26-85, so we can really create the best future for our children."
Mayor meets Link Crew
Mayor Tom Potter meets DDHS "Link Crew" members Thuan Huinh, Emily Yip, Samantha Cha, and Oile Dao.
On his way into the school, Mayor Potter met representatives of the school's "Link Crew" He learned team's mission is to ease the transition of grade-schoolers 9th grade.
"It is like a Big Brother/Sister program," explained the school's Principal, Randy Hutchinson. "Each Link Crew member takes eight to ten freshmen under their wing, especially the first week. The young kids can ask any Link Crew member for help and know they'll get it."
Hutchinson said Link Crew members aren't necessarily the team captains and club presidents. "They are middle-of-the-road, ordinary students who have a drive to, and desire to, help others."
"Let's go in and meet the freshmen," Potter said.
David Douglas' challenges
On our way in, we spoke Barbara K. Rommel, Superintendent of David Douglas School District.
"Our biggest challenge," Rommel told us, "is our enrollment growth. We're anticipating 3% more students than last year — the largest enrollment in the history of David Douglas school system. In all, we've had a 25% increase since 1999. This is really stretching our classroom space. While other schools are closing, we're working to create the space we need to keep class sizes manageable."
Rommel said the Mayor's visit demonstrates his commitment to education at all of the schools in the City of Portland. "And, with David Douglas being the largest high school in the state, it is really great to see our city's Mayor here, welcoming the freshmen."
Mayor Tom Potter addresses 800+ freshmen – the largest single class in David Douglas High history – at their orientation.
The mayor's introduction at the assembly was met with wild cheering. "Good morning everybody! What a good-looking group of people you are. You are so fortunate. You are attending, not only the largest high school in Oregon, but one of the very best. All of your teachers, staff members, and Link Crew members are here to help you succeed. Have a great year."
Asked why he was coming out in support of David Douglas building program bond, the mayor responded, "Investing in students today pays all of Oregon back tomorrow."
Building project underway
The school's Principal, Randy Hutchinson, commented on our way out, "It's is nice to see that he [Potter] has hung his hat on being an 'education mayor', and he's paying attention to East County."
The challenge for the school, Hutchinson told us, is "sheer numbers. Enrollment keeps increasing. It looks like our enrolment is about 2,900, and another 200 students at our alternative school."
The growling of earth-moving equipment was punctuated with the blaring of back-up claxons as he pointed to an area east of the main building. "While other schools are closing and consolidating, this construction project will add twenty classrooms. We need them."
© 2006 David F. Ashton ~ East PDX News


text:
La Sarcelle d'été (Spatula querquedula) est une espèce d'oiseaux aquatiques appartenant à la famille des Anatidae.

En Camargue, elle est connue sous le nom de cacharel, terme que le Nîmois Jean Bousquet adopta en 1962 pour nommer sa marque de prêt-à-porter Cacharel.

Description
Elle mesure 40 à  de long pour 58 à  d'envergure et un poids de 300 à .
Le mâle revêt son plumage nuptial au printemps : de larges sourcils blancs et des scapulaires gris-bleu. En été, il adopte le même plumage que sa femelle mais garde des couvertures alaires bleu clair. Comme la Sarcelle d'hiver, cette espèce se lève facilement de l'eau avec des battements d'ailes rapides, un peu comme les échassiers.

Répartition
Elle niche dans une grande partie de l'Europe et l'Asie occidentale, mais est strictement migratrice, avec toute la population passant en Afrique australe et en Australasie en hiver, où elle peut former de grands rassemblements.

Habitat
Les préférences écologiques de la sarcelle d'été sont assez proches de celles de la sarcelle d'hiver, même si la première tend à éviter les eaux saumâtres.

Alimentation
Son alimentation est constituée principalement de substances animales et végétales (petits poissons, petits amphibiens, crustacés, mollusques, insectes, vers, bourgeons, feuilles, racines, grains).

Reproduction
La femelle niche au sol au milieu de la végétation. Elle pond de 8 à 11 œufs qu'elle couve pendant 21 à 23 jours. Les petits, nidifuges, sont élevés par la femelle et volent au bout de 5 à 6 semaines.

Menaces
L'Union internationale pour la conservation de la nature classe la sarcelle d'été comme préoccupation mineure. En Wallonie, l'espèce est jugée en danger critique.

Galerie

Notes et références

Bibliographie
 Bologna G., Les Oiseaux du Monde, Guide Vert, Solar, 1993, 511 p.
 Chantelat J.C, Les Oiseaux de France, Guide Vert, Solar, 2012, 77 p.

Liens externes

Anatidae
Faune de la Camargue
Oiseau d'Eurasie
Oiseau d'Afrique

redpajama_set_name: RedPajamaWikipedia


Its weight is 230 pound and can bear the limit of 237-pound weight for workout and measures 27 w-58 h-83 d when fully spread.
It comes in dimensions of 41 x 26.5 and weighs around 63 lbs.
Easy customization of workout routine Elliptical trainers machines allow you to use it with different resistance levels, speed and stride length to get amazing workout experience throughout your session without getting bored and it also makes sure that your all kinds of body muscles get.
To help you work out at right intensity it allows you to adjust the resistance digitally up to 25 levels to give you best workout experience at every fitness level.Click image for latest price This elliptical machine comes with good quality backlit LCD display with lots of tracking function to give exact information about your workout and track your goals.Besides workout on elliptical try to change your diet patterns also from junk to healthy food for faster and better results with your elliptical workout.If you want an elliptical machine thats compact and powerful as you dont win 7 ie 11 download have enough space in your house to fit a large machine then we got you covered with Cubii Mini Elliptical.its powerful but portable and mini elliptical machine made to solve the problem.Handlebars with multiple grips and curved structure help to focus on different muscles sets on the body for better body fitness and muscles.It is a high quality midrange elliptical machine with a lot of good features which makes it worth the price.Things to keep in mind before buying best elliptical Machine Make sure to go through all the points given to get an insight about what you should know about the elliptical machines for your personal use before you head out to buy a top elliptical.You can also put an infuser water bottle in the holder to keep your thirst at the bay.It comes with display console which shows all the vital body information like calories burned along with distance traveled, speed etc.After workout, always wipe down your 1260Ef unit.It also comes with Bluetooth connection to sync all your workout data to your smart devices.Quiet Operation For some people, little noise is fine as they use headphones while workout but for some, it is not and they like very quite working machines, so it depends on personal choice what you want and what you can pay for.Your heart rate will also increase and the rate of calories burnt per hour will also increase with a higher incline.If you want to buy an advanced version of this machine with some more features and advancements like Bluetooth connectivity etc then you can check out.
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Repair or replace any damaged or worn parts, tighten all loose hardware.
Portability Portable elliptical machines are easy to move for a workout.Look for loose hardware, loose pedals, loose handrails, loose cranks and frayed wires.So its the time to decide, which one to zero in on your choice taking in consideration your needs and budget and zeal to stay fit forever.if you are serious about your workout and staying healthy throughout your life then i dont think that you.When you workout on elliptical with incline your legs remain straight when the legs move on forward and backward pedal only their is a slight degree of change in your hip extensions along with knee angle and ankle plantar flexion.Using it is quiet and smooth without any problem as it works on the belt is driven flywheel and its maximum supported user weight is about 220 lbs.Nautilus E616, pros cons, dual lcd display compact and space-efficient equipment comes with media shelf to keep book or tablet metal ring under pedal pops off sometimes sometimes usb connectivity may give problem some times it squeaks and produces noise click image for latest price and.With adjustable resistance, you can start low and later on you can work with high-intensity by increasing the resistance on your elliptical machine easily as per your body requirement and fitness goals to reach them without any pain in your body and legs.


text:
Personal Loan Tadepalligudem, 21 January 2020 from shamrao Vithal Co-op Bank
Wedding Loan from shamrao Vithal Co-op Bank in Tadepalligudem
Tadepalligudem, also known as TPG, is located in West Godavari in the state of Andhra Pradesh. It has a municipality and the headquarters of Tadepalligudem is situated in the Elluru division. The demographics of the city is fascinating with the sex-ratio at 1022 females per 1000 males. The population constitutes of 51,378 males and 52,528 females and the total population adds up to 103,906. One of the striking features of this city is the high literacy rate, 83.10% much higher than the national literacy rate of 73%. It is not surprising that the city has a large number of schools and colleges. The towns and cities surrounding Tadepalligudem include Bhimadalu, Dabacherla, Madhavaram etc. The historical significance of Tadepalligudem in World War 2 cannot be overstated. It was a military base for the East India Company and the Britishers constructed an airport in the city for sending military off to the War. However, the airport has not been modified for commercial use, once it is renovated suited for commercial purposes, the trade and commerce in the city can also improve. Tadepalligudem is famous for its jaggery market and rice cultivation. While Maharashtra has the tag of the largest producer of jaggery, Tadipalligudam is considered as the chief producer of jaggery. Tadepalligudem has the largest rice mill in the entire district. Along with rice mills, food, fat and fertilizer industries are also moderately successful in this region. Transportation is a big industry in this town, with more than 6000 transport vehicles, the transport industry of Tadepalligudem is comparable to the coastal capital of Andhra Pradesh, Vijayawada.
Low interest rate Wedding Loan in Tadepalligudem, 21 January 2020 from shamrao Vithal Co-op Bank
The SVC Bank was initially registered as a Co-operative Credit Society on 27 December 1906. In 1907, cumulative deposit scheme, fixed deposit scheme and saving bank deposit were introduced by the bank. The bank in opened first Co-operative store in 1910. In 1915, the first Co-operative housing society was built in Bombay. In 1927, the Fidelity Guarantee Fund was launched simultaneously with Distress Relief Fund in 1931 and Staff Gratuity Fund in 1954. In 1964, Safe Deposit Vaults were introduced by the bank. In Fiscal 2016, the deposits of the bank crossed 13000 crores. In 2002, the corporate office was opened by the bank at SVC Tower in Vakola. In 2003, Genius I Core banking solution was implemented in all the branches of SVC bank. In 2006, the SVC bank successfully sold the software. In 2007, AD-I license was offered to the Shamrao Vithal Co-operative bank. The SVC bank was also allowed to sell the core banking software services to small co-operative banks. By 2010, the bank sold software services to around 25 other banks. The 193rd branch of the SVC bank was opened at Khmagaon. The Bank is present in 10 States of India. Maharashtra, Karnataka, Tamil Nadu, Telangana, Delhi, Rajasthan, Haryana, Goa, Gujarat and Madhya Pradesh

redpajama_set_name: RedPajamaCommonCrawl


As a sensor mounted on a high pressure hose, which triggers the strobe lamp to check the start of the injection. By means of this sensor, it is easy to convert a typical petrol engine strobe lamp into a diesel engine one.
As a sensor (sensors) mounted on a high pressure hose to check the high pressure waveform and to compare the measurements (without loosening the hoses) by means of an oscilloscope. This method allows a quick diagnosis of the injection system.
As a sensor for measuring the diesel engine speed.
As replacement sensor, for example, for strobe lamps and similar diagnostic tools.
In contrast to conventional sensors, which are designed to serve a single diameter of high pressure hoses, the SP-312 sensor supports all diameters of hoses ranging from 3 to 12 mm. The sensor has a robust construction, which makes it resistant to damage.


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text:
Q: SQL Server error: "Cannot insert explicit value for identity column" even when I SET IDENTITY_INSERT ON I REALLY review several times, that's the reason I am asking; looking for guidance...
I have one table, as the script below. Then, I set IDENTITY_INSERT ON. Then I try to do an insert select, (I NEED the very same ids)
I keep getting this error:

Msg 544, Level 16, State 1, Line 2
  Cannot insert explicit value for identity column in table 'Table1' when IDENTITY_INSERT is set to OFF.

Does anybody knows why? Any set up at DB level can overrule the IDENTITY_INSERT ON?
I appreciate any advice. Thanks in advance and kind regards.
Script to table:
SET ANSI_NULLS ON
GO

SET QUOTED_IDENTIFIER ON
GO

CREATE TABLE [dbo].Table1
(
    [TableId] [int] IDENTITY(1,1) NOT NULL,
    [Name] [nvarchar](256) NOT NULL,
    [RowVersion] [timestamp] NOT NULL,
    [AddedDate] [datetime2](7) NOT NULL,
    [stuff2] [int] NOT NULL,
    [ModifiedDate] [datetime2](7) NOT NULL,
    [LastModifiedBy] [int] NOT NULL,

    CONSTRAINT [Table1_PK]
        PRIMARY KEY CLUSTERED ([TableId] ASC)
) ON [PRIMARY]
GO

The insert statement:
SET IDENTITY_INSERT [dbo].Table1 ON;

INSERT INTO [dbo].Table1 ([TableId], [Name], [AddedDate], [stuff2], [ModifiedDate], [LastModifiedBy])
    SELECT
        [RoleID], [Name], [AddedDate], [stuff2], [ModifiedDate], [LastModifiedBy]
    FROM
        [dbo].Table2

A: I had the same error even though I had run the SET IDENTITY_INSERT mytable ON command on my table. I realized it was because I was closing lines in the query script.
If you are closing each line with ;, the SET IDENTITY_INSERT mytable ON command will not hold for the following lines.
i.e.
a query like
SET IDENTITY_INSERT mytable ON;
INSERT INTO mytable (VoucherID, name) VALUES (1, 'Cole');

Gives the error
Cannot insert explicit value for identity column in table 'mytable' when IDENTITY_INSERT is set to OFF.
But a query like this will work:
SET IDENTITY_INSERT mytable ON
INSERT INTO mytable (VoucherID, name) VALUES (1, 'Cole')
SET IDENTITY_INSERT mytable OFF;

It seems like the SET IDENTITY_INSERT command only holds for a transaction, and the ; will signify the end of a transaction.

A: Thank you so much @Sami, you help me to realize the right path.
It turns out, you can just use, IDENTITY_INSERT to one table at time (for obvious reasons is not a thing I do often).
When I did for several tables at time, I saw the error, but as the name of the tables were similar, I thought it was throwing an error because I ran the Identity_insert before on the same table, but it was because it was taken by the other table.
I didn't realized until I review the Error messages one by one. :P  :D
https://dba.stackexchange.com/questions/12650/why-is-identity-insert-on-only-allowed-on-one-table-at-a-time

A: I had the same error, then i found out that i was inserting an explicit value while my PK is set to Is Identity = true, while my relation was 1:1..0, meaning my child table uses the PK of the Parent table. [DatabaseGenerated(DatabaseGeneratedOption.Identity)] will only work if the Is Identity = true and there is no conflict in your table.

redpajama_set_name: RedPajamaStackExchange


text:
Q: How would I remove all the zeros before the 1 in this python list result = [0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 1, 1, 1, 1, 1, 1, 1, 0, 1, 1, 0, 0]

I want this list to be turned into
result = [1, 1, 1, 1, 1, 1, 1, 0, 1, 1, 0, 0]

I have tried using a while loop to keep removing zeros until it finds a 1 but I cant seem to get that to work.
for x in result:
    while (x == 0):
        result.remove(0)

A: If there always is a 1, you could just find it and delete everything before it:
del result[:result.index(1)]

Or if it could be all zeros:
if any(result):
    del result[:result.index(1)]

or
try:
    del result[:result.index(1)]
except ValueError:
    pass

or
result.append(1)
del result[:result.index(1)]
result.pop()

A: One way using itertools.dropwhile:
from itertools import dropwhile

list(dropwhile(lambda x: x == 0, result))

Output:
[1, 1, 1, 1, 1, 1, 1, 0, 1, 1, 0, 0]

A: Problem in your code is you are changing the list while iterating. Instead you can use while loop.
while result and result[0] == 0:
    result.pop(0)
print(result)

Output:
[1, 1, 1, 1, 1, 1, 1, 0, 1, 1, 0, 0]

A: Or else try the following :
result = [0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 1, 1, 1, 1, 1, 1, 1, 0, 1, 1, 0, 0]
a=''
for i in result:
    a=a+str(i)
print(list(a.lstrip('0')))

A: result = [0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 1, 1, 1, 1, 1, 1, 1, 0, 1, 1, 0, 0]

# prints index of 1st (leftmost) '1' encountered in the list
# print(result.index(1))

# print from that index to the wholw remaining list
print(result[result.index(1):])


At a time when the electoral system is coming under renewed scrutiny, this article examines the origins and creation of the present system in 1884-5, and its subsequent survival. This is the first such analysis to draw upon Public Record Office and party archives. Whilst showing that the political classes have been quite prepared to consider the merits of alternatives, particularly S.T.V., for Ireland or in colonial settings, they have usually been seen as less appropriate for Westminster. In exploring why that should be the case this article seeks to provide a new explanation for the longevity of the electoral arrangements of 1885.


text:
Les Roques de Sapera és una muntanya de 804 metres que es troba al municipi de Pontons, a la comarca de l'Alt Penedès.

Referències

Muntanyes de Pontons


Grilling steak this summer? Try one of these Argentine malbecs, all priced at $25 or less.
Mendoza is a giant in many ways.
In the most obvious way, it is the largest and most important wine region in one of the largest countries on earth — a prodigious, wine-producing nation that consistently hovers around the No. 5 spot worldwide.
Metaphorically, the Mendoza region of Argentina is a giant for what it has done with, and for, malbec, its adopted and most-prized grape variety. Mendoza lies in western Argentina, at the foot of the Andes mountain range, about 650 miles west of the capital city of Buenos Aires.
The Andes give Mendoza its altitude, with some of its best vineyards rising to roughly 3,000 feet in elevation, and others soaring past 5,000 feet, providing a sunny, dry climate with cool nights. The province of Mendoza is divided into regions, one of which, Lujan de Cuyo, was named Argentina's first protected wine appellation in 1993. Another is the legendary Uco Valley (or Valle de Uco, as it often appears on labels), which includes the Tupungato, Tunuyan and San Carlos districts.
Argentina has been home to winemaking operations since the late 1500s, due in part to both friendly and hostile visitors from across the Atlantic Ocean in Spain. But it wasn't until the mid-1800s that malbec arrived in Argentina from France. This is when the sleeping giant's eyelids began to flutter, though it would be another century and a half before the giant was fully awake. They move slowly, giants.
In Cahors, the wine region in southwestern France where malbec was born, it's often a big wine full of heft and tannins—a good partner for the rich, local cuisine, such as cassoulet, duck confit, game meats, foie gras and black truffles. Argentine malbec is generally fruitier and less tannic than it is in Cahors, with hints of plum, blackberries, chocolate, earth and spice, plus a supple, velvety mouthfeel. Still, though, it's a great complement to big foods: steaks, burgers and just about any seared meat plucked from a flame-kissed grate. Argentines eat their locally grown, grass-fed beef like it's the only food there is, after all.
Malbecs from Argentina are no longer the across-the-board bargains that they once were (due, presumably, in part to an influx of foreign interest in the region), but there are still plenty of affordable bottles out there. While other grapes, including cabernet sauvignon and bonarda, are sometimes blended with malbec, many Mendoza malbecs are 100 percent varietals. Even in the case of blends, to be labeled a malbec in Argentina, the bottle must contain at least 85 percent of the grape.
Argentine malbecs, especially from within Mendoza, are relatively easy to find in shops and restaurants. Below are brief notes from a recent tasting. The bottles are listed in ascending order, according to price.


You do not need specialist training at all! Simply complete our Schools Programme Training before you start tutoring - this should only take 5 minutes. It will give you a great overview on what the programme aims to do, whilst giving you some key details on how it operates.
You can also view our Schools Tutor Resource Library to help you deliver fantastic tutorials. We have a brilliant collection of regularly updated articles for numerous subjects, these are packed full of useful information and tips for planning out your tutorials.
We will also be releasing short tips and training guides to subject specific tutors to enable them to improve the effectiveness of their tutorials!
Finally, you may be provided with details of particular topics pupils need help with, and given resources provided by us and the schools, to help you deliver focused, high-impact lessons.


text:
Satan's Pilgrims - The Way In To Way Out? 7" EP (Satan's Pilgrims)
Marking the 10th anniversary of the Psychsploitation album, this 7" single "The Way In to Way Out?" features 3 original songs recorded in 2019 with Satan's Pilgrims and Psychsploitation engineer Eric Hedford. Artwork and layout for the single also brings back on board Aaron Mahony who did layout for Psychsploitation! Comes with a download card.
Tracks: The Way In To Way Out? - Solar Flare - Journey To Eden
Satan's Pilgrims - At Home With Satan's Pilgrims CD
Click the button below to add the Satan's Pilgrims - The Way In To Way Out? 7" EP to your wish list.
Satan's Pilgrims - Frankenstomp CD $15.75
Satan's Pilgrims - At Home With Satan's Pilgrims CD $14.75
Satan's Pilgrims - Siniestro CD $14.75
Satan's Pilgrims - Psychsploitation CD $14.75
Satan's Pilgrims - Splashdown / Dr. Mortis 7" $10.75


text:
Immigration Defense
Asylum, 8 U.S.C. §§ 1158(a), 1101(a)(42)
The "Real ID Act of 2005" was signed into law (Pub. Law No. 109-13) on May 11, 2005, as Division B of the Emergency Supplemental Appropriations Act for Defense, the Global War on Terror, and Tsunami Relief, 2005, and became effective on the date of enactment.
(Sec. 101) Amends Immigration and Nationality Act (INA) provisions concerning asylum to: (1) authorize the Secretary of Homeland Security, in addition to the Attorney General, to grant asylum (retroactive to March 1, 2003); (2) require asylum applicants to prove that race, religion, nationality, membership in a particular social group, or political opinion was or will be (if removed) the central reason for their persecution; and (3) provide that an applicant's testimony may be sufficient to sustain this burden of proof only if the trier of fact determines that it is credible, persuasive, and fact-specific. Requires corroborating evidence where requested by the trier of fact unless the applicant does not have the evidence and cannot reasonably obtain it without departing the United States. States that the inability to obtain corroborating evidence does not excuse the applicant from meeting his or her burden of proof.
Lists factors relevant to credibility determinations in asylum cases, including (but not limited to) the: (1) demeanor, candor, or responsiveness of the applicant or witness; (2) inherent plausibility of the applicant's or witness' account; (3) consistency between the applicant's or witness' written and oral statements; (4) internal consistency of each such statement; (5) consistency of such statements with other evidence of record (including the Department of State's reports on country conditions); and (6) any inaccuracies or falsehoods in such statements regardless of whether they go to the heart of the applicant's claim. States that there is no presumption of credibility.
Makes this Act's provisions regarding proof requirements and credibility determinations in asylum proceedings applicable to other requests from relief for removal.
Limits judicial review of determinations regarding the availability of corroborating evidence.
Removes the numerical limit on the number of aliens granted asylum who may become lawful permanent residents in any fiscal year (currently set at 10,000).
Asylum is strictly a discretionary form of relief. To qualify for asylum, an alien must demonstrate a well grounded fear of persecution upon return to the country of such person's nationality on account of race, religion, nationality, membership in a particular social group, or political opinion. An application for asylum is deemed also to constitute an application for withholding of deportation (discussed below). An alien who has been convicted of an aggravated felony may not apply for or be granted asylum. 8 U.S.C. § 1158(d). Moreover, an asylum application must be denied if the alien having been convicted by a final judgment of a particularly serious crime in the United States, constitutes a danger to the community. 8 C.F.R. § 208.14.
To be successful on an asylum claim, the alien must prove: (1) that he or she has a well-founded fear of persecution or has suffered past persecution; (2) that such persecution is because of race, religion, nationality, membership in a particular social group or political opinion; and (3) that asylum should be granted in the exercise of discretion.
Criminal Activity And Immigration Status
Deportation Defense
Withholding of Removal
Temporary Protected Status, 8 U.S.C. § 1254a
212(h) & Adjustment Of Status To LPR
Inadmissibility
Deportability
Cancellation of Removal
Convention Against Torture
Family Based Petitions
Immigration & Crimes
U Visas
Asylum, 8 U.S.C. §§ 1158(a), 1101(a)(42) | Wisconsin Immigration Lawyer


Located at the northern part of the Hutchinson Island in Florida, the U.S. Navy SEAL Museum is nestled at the original place where the Frogmen underwent their training back in the early 1940s. The Navy SEAL Museum is dedicated to the elite group of the Naval Special Warfare, the only one in the whole world.
The U.S. Navy Frogmen, the original name given to the Navy SEALs, were born and came to existence at Fort Pierce, Florida, where the National Navy SEAL Museum now stands. The U.S. Navy Underwater Demolition Teams and the U.S. Naval Combat Demolition Units were composed primarily of brave volunteers for the Second World War.
It was in November 1985 when the Navy SEAL Museum was formally dedicated to the elite group of the U.S. Special Operations Forces. Thereafter, an endless number of artifacts have continuously been sent to Fort Pierce.
The Navy SEAL Museum provides a good venue for people to learn more about the history of the Naval Special Warfare. Inside the Navy SEAL Museum, one will be able to discover the beginnings of the Underwater Demolition Team, learn about their exploits in the Second World War, and understand more about the Navy SEALs by way of the artifacts and the many photographs displayed in the museum.
Outside, one will feel nostalgic seeing various modes of transportations that have been used by the Navy SEALs. A helicopter, two-man submarines, and patrol boats are artfully displayed outside the museum. The vehicle's story can be read on a statue that stands on each of them.
Inside, one will be greeted by a volunteer, who could be a retired SEAL, a retired Frogman, or a spouse of a Frogman or a SEAL. The volunteer will serve as your guide in your tour of the museum and will explain every memorabilia on display.
Like the usual museum, the Navy SEAL Museum also has a shop for us navy seals visitors where they can purchase their choice of SEAL souvenirs such as a pin, a cap, or a book. Tactical gear like backpacks, gloves, bags, and holsters can likewise be bought at the Navy SEAL Museum store.
U.S. Navy SEAL shirts, polos, cammies, and other tactical apparel (ideally for souvenir purposes) are available at the museum shop. Items are moderately priced, and the museum also accepts donations for it maintenance. Also, for a $100 donation, one can make his name part of the great Navy SEAL history with his own memorial brick being used nowhere else but within the grounds of the museum.
About the Author: This Article is written by James Kara Murat from USNavySealStore.com, the contributor of Navy Seal Store. More information on the subject is at A Tour of the Navy SEAL Museum, and related resources can be found at navy seal workout.


The Pacific Alliant – comprising Mexico, Colombia, Peru and Chile – has agreed to set up an infrastructure investment fund.
Intended to improve connectivity in the region, the fund will receive investments both from private entities and from institutions from within the bloc and globally. These include the Inter-American Development Bank (IDB) and the Development Bank of Latin America (CAF), according to Chile's finance minister Rodrigo Valdés.
Martín Vizcarra, president pro tempore of the alliance, said that the primary objective now is to decide what structure the fund will have. It remains to be established how investors will be matched to projects, the type of corporate governance the fund will have, and each Pacific Alliance country's share in it.
Authorities have estimated that the initiative could mobilise more than US$100 billion.


Opening the doors to the unique guestrooms will immediately launch you into a world of "manga." The rooms have been designed based on a playful theme typical of Japan, and they are sure to give you a chuckle.
All rooms are equipped with shower booths. Although compact, the booths are large enough to provide stress-free showers.
Under-bed storage space is available with sufficient capacity to easily store large suitcases and travel bags to ensure that you can make the best use of the space available in your room.


text:
Women's March LA Canceled Due To COVID, National Unrest
By City News Service Jan 12, 2021
LOS ANGELES (CNS) - The annual Women's March LA was canceled today, with organizers citing the continuing COVID-19 pandemic and national unrest following the recent storming of the U.S. Capitol.
The march, which annually attracts thousands of women, along with elected officials and celebrities, had been scheduled for Jan. 23.
In a statement, the Women's March Foundation said it would be "irresponsible'' to organize a march "in the face of these issues and it is imperative to keep our communities safe.''
"Although we would have loved to take to the streets to celebrate our very own (Vice President-elect) Kamala Harris, it simply is not possible,'' Emiliana Guereca, president of Women's March LA, said in a statement. "We hope to march for International Women's Day.''
In the meantime, the organization has announced plans for a virtual viewing party for the inauguration of Joe Biden and Harris on Jan. 20. Registration for that event is at
https://www.mobilize.us/womensmarchaction/event/367457/


You may have noticed the "Featured Image" box when editing a post or page. It allows you to upload or select an associated image for the article. It generally appears as a thumbnail when viewing a list of posts, perhaps in a category index or search results.
Thumbnail support must be enabled within your theme. You could add it to a plug-in so it's available to all themes but that may not be appropriate in every case. Therefore, you'll need to open or create a 'functions.php' file within your theme folder (wp-content/themes/theme-name/).
Default thumbnail sizes can be set in WordPress's Settings > Media screen. However, you can also set a default height and width in functions.php, e.g.
This will produce thumbnails with 100px width and a 75px height (a pleasing 4:3 ratio). However, what happens when a user uploads an image with different aspect ratio — say 100 x 150? In this case, the whole image is proportionally reduced to fit the space and the resulting thumbnail is 50 x 75.
The "Featured Image" box should now appear on your WordPress post/page edit screen. If it's not there, check it's enabled in "Screen Options" or review your functions.php code.
The second is an associative array containing the src, class, alt and title.
That's about as complex as it gets. Have fun adding thumbnail support to all your WordPress themes.


text:
window.chart = require('chart.js');

var randomScalingFactor = function () {
    return Math.round(Math.random() * 1000)
};

var lineChartData = {
    labels: ["January", "February", "March", "April", "May", "June", "July"],
    datasets: [
        {
            label: "My First dataset",
            fillColor: "rgba(220,220,220,0.2)",
            strokeColor: "rgba(220,220,220,1)",
            pointColor: "rgba(220,220,220,1)",
            pointStrokeColor: "#fff",
            pointHighlightFill: "#fff",
            pointHighlightStroke: "rgba(220,220,220,1)",
            data: [randomScalingFactor(), randomScalingFactor(), randomScalingFactor(), randomScalingFactor(), randomScalingFactor(), randomScalingFactor(), randomScalingFactor()]
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            strokeColor: "rgba(48, 164, 255, 1)",
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            pointStrokeColor: "#fff",
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            pointHighlightStroke: "rgba(48, 164, 255, 1)",
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        highlight: "#fac878",
        label: "Orange"
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        highlight: "#fac878",
        label: "Orange"
    },
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        color: "#1ebfae",
        highlight: "#3cdfce",
        label: "Teal"
    },
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        value: 120,
        color: "#f9243f",
        highlight: "#f6495f",
        label: "Red"
    }

];

window.onload = function () {
    var chart1 = document.getElementById("line-chart");
    if (chart1) {
        chart1 = chart1.getContext("2d");
        var mychart = new Chart(chart1, {
            type: 'line',
            data: lineChartData
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     window.myDoughnut = new Chart(chart3).Doughnut(doughnutData, {
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     window.myPie = new Chart(chart4).Pie(pieData, {
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redpajama_set_name: RedPajamaGithub


text:
"Gott würfelt nicht!" ist ein Ausspruch, der auf Äußerungen des Physikers Albert Einstein zurückgeht und dessen Haltung in der Bohr-Einstein-Debatte verdichtet.

Einstein schrieb in einem auf den 4. Dezember 1926 datierten Brief an Max Born (evtl. auch in einem Brief an Niels Bohr):

Interpretation
Die Metaphorik des Satzes lässt einen weiten Interpretationsspielraum zu, den Einstein nicht durch nähere Erläuterungen eingeschränkt hat.

Eine mögliche Interpretation Einsteins Aussage besteht darin, dass er die wahrscheinlichkeitstheoretische (stochastische) Erklärung der Quantenmechanik ablehnte. Diese Interpretation ist allerdings umstritten.

So schreibt Ballentine, dass Einsteins Argumente bezüglich der Interpretation der Quantenmechanik von anderen Physikern oft völlig falsch verstanden worden seien. Nach Ballentine habe Einstein die statistische Interpretation von Max Born nicht abgelehnt, sondern im Gegenteil für die einzig zufriedenstellende gehalten – entgegen der Interpretation von Niels Bohr, der sie für ein Phänomen einzelner Teilchen hielt. Und Einstein sei auch kein Unterstützer der Theorien versteckter Variablen gewesen und seine Argumentation erforderte auch keinen zugrunde liegenden Determinismus.

Gregor Schiemann folgert, dass Einstein mit "dem Geheimnis des Alten" eine allen Erscheinungen zu Grunde liegende einheitliche Struktur der Natur meint. In Einsteins am ehesten als spinozistisch zu bezeichnenden Gottesauffassung "stehe Gott einerseits für das Ganze der Natur und andererseits für ein in der Natur wirksames aktives Prinzip".

Mario Wingert beschreibt das "Dilemma" so, dass Bohr "die Auflösung des Welle-Teilchen-Paradoxon als unmöglich – und unnötig" erachtete, während Einstein davon ausging, dass "es Strukturen der Realität geben muss, die zu erkennen Aufgabe der Physik sei".

Letztlich ging es um die Frage, ob der Determinismus der klassischen Physik, z. B. der Newtonschen Mechanik oder der klassischen Elektrodynamik, in der Quantenmechanik noch Gültigkeit hat oder nicht, was inzwischen im letztgenannten Sinn entschieden ist. Einstein versuchte deshalb bis zu seinem Tode 1955 vergeblich, die Quantenmechanik durch sog. verborgene Variablen deterministisch zu machen. Die These, dass Gott nicht würfelt, also die Physik keinen Zufall kennt, war Einsteins Antwort auf die Frage, was ihm an der damals aufkommenden Quantenphysik nicht behage, denn dort werden Zustände eines physikalischen Systems mittels Wahrscheinlichkeiten beschrieben, z. B. mit Aufenthaltswahrscheinlichkeiten; siehe u. a. den Artikel Zustand (Quantenmechanik).

Über die Quantenmechanik schrieb er in einem Brief an Cornelius Lanczos am 21. März 1942:

Aber schon in den Gesprächen mit Niels Bohr während der späten 1920er Jahre bekam er Widerspruch.

Ulrich Walter schreibt:

Experimentelle Widerlegung
Obwohl Einstein einen außergewöhnlichen Ruf als Wissenschaftler hatte und die scharfsinnigen physikalischen Feststellungen, die seiner Arbeit zur Interpretation der Quantenmechanik (EPR-Effekt, 1935) zugrunde lagen, sich – im Gegensatz zu den seiner Arbeit zugrunde liegenden philosophischen Prämissen  – ausnahmslos als korrekt und grundlegend für die gegenwärtige physikalische Begriffswelt erwiesen haben (z. B. für den Begriff der Quantenverschränkung), sind seine Folgerungen aufgrund der in der Arbeit genannten philosophischen Voraussetzungen (die auf "Gott würfelt nicht" hinauslaufen) inzwischen durch sorgfältige Experimente, basierend auf der Bellschen Ungleichung, explizit falsifiziert worden, was ein wissenschaftstheoretisches Grundlagenergebnis darstellt.

Die Bellsche Ungleichung, die in Sachen Quantenmechanik eine experimentelle Entscheidung für oder wider Einstein ermöglichte, wurde erst lange nach Einsteins Tod bekannt, und es dauerte weitere Jahrzehnte, ehe die Entscheidung experimentell durchgeführt werden konnte. Sie fiel gegen Einstein aus.

Heute gelten Einsteins grundlegende Einwände gegen die Quantenmechanik daher als widerlegt und werden in der Physik nicht mehr vertreten. Trotzdem ist Einsteins Autorität auch in dieser Angelegenheit bei den Physikern ungebrochen, weil er als Erster "den Finger in eine offene Wunde gelegt hat" und seine Einwände, obwohl sie sich wegen nicht zutreffender philosophischer Prämissen als falsch erwiesen haben, trotzdem die Entwicklung einer Fülle konkreter und zukunftsweisender Physik bedingten.

Zu den oben genannten experimentellen Ergebnissen siehe z. B. Alain Aspect. Ein Resümee unter vielen:

Trivia
EinStein würfelt nicht war das Begleitspiel der Wanderausstellung zum Einstein-Jahr Gott würfelt nicht: Wissenschaft im Spiel – Spiel in der Wissenschaft, die im Juli 2005 in Göttingen startete.

Literatur
 Paul Davies: Die Unsterblichkeit der Zeit. Die moderne Physik zwischen Rationalität und Gott. Scherz, Bern u. a. 1995.
 Dieter Hattrup: Einstein gegen den würfelnden Gott. Kindle Edition, 2011.
 Werner Heisenberg:  Der Teil und das Ganze. Gespräche im Umkreis der Atomphysik. Piper, München 1969.
 Richard Morris: Gott würfelt nicht. Universum, Materie und kreative Intelligenz. Europa, Hamburg 2001, ISBN 3-203-80099-3.

Anmerkungen

Geflügeltes Wort
Albert Einstein


text:
Q: Knitting from rmd to html I'm trying to knit this rmd file for my class and I have to do it on the class server. Problem is I access to that server with a ssh connection (since I didn't want to install a virtual machine) and therefore can't use the RStudio really handy knit button
I've tried using knitr() and rmarkdown::render() and nothing seems to work.
So far i've tried :
require(knitr)
require(rmarkdown)
knit(file.rmd, file.md)
makdownToHTML(file.md, file.html)

this allows me to knit the file, but won't add the theme, author name, date and toc that are necessary for this project
I've also tried :
rmarkdown::render(file.rmd)

Which gives me:
pandoc version 1.12.3 or higher is required and was not found.

I've checked and for some reason the rmarkdown::pandoc_version() is null on the server (even though it's supposed to be installed with RStudio that the rest of the class uses on the virtual machine)
Right now I am looking for way to bypass the pandoc or load the files in my home to be able to knit this rmd file once and for all...
Any idea on the matter??


text:
\section{Introduction}

Flavour-changing neutral current (FCNC) processes provide an
extraordinarily useful tool to investigate new physics beyond the
Standard Model (SM). In supersymmetry (SUSY), as in other models beyond
the SM, an alternative to the direct search for new particles is to look
for their radiative effects.  In the SM, FCNCs are absent at tree level,
but they arise at one-loop order, being strongly suppressed as a consequence
of the GIM mechanism~\cite{GIM}.  The Minimal
Supersymmetric Standard Model (MSSM)~\cite{HaberKane} provides a natural
framework where FCNCs are enhanced.  In the scenario with minimal
flavour violation (MFV) of the MSSM, squarks are assumed to be aligned
with the corresponding quarks, and flavour violation originates from the
Cabibbo--Kobayashi--Maskawa (CKM) matrix as the only source, proceeding
via loop contributions, in analogy to the SM.  Therefore, its size is
expected to be very small.  In more general scenarios which include
misalignment between the quark and squark sectors, sizeable
contributions to FCNC processes are expected to occur.  This is the case
of the MSSM with non-minimal flavour violation (NMFV).

The quantum contributions from supersymmetric particles in $B$-meson
physics have been studied in a series of processes, including
$B^0$--$\bar B^0$ mixing~\cite{toharia,newchanko}, leptonic $B$-meson
decays~\cite{kolda,oldchanko,alemanes,newisidori} and $B\to
X_s\gamma$~\cite{bstanbeta,bsgamma,leadingbsg,gambinobsg,hurth}, and
have been found to be large.  In order not to be in conflict with
present experimental data, these in turn imply restrictions both on the
SUSY parameters and on the parameters measuring the size of flavour
mixing in the squark sector~\cite{newisidori,hurth,9604387,ciuchini}.
The rare decay $B\to X_s \gamma$ is at present one of the most important
since its observation~\cite{boundsbsg} sets stringent constraints on the
parameter space of various extensions of the
SM~\cite{gambinobsg,9604387,hurth}.
Furthermore, the recent data from $B\to X_s\mu^+\mu^-$ indicate that the
sign of the $\bsg$ amplitude is the same as in the SM \cite{Gambino:2004mv}.

Moreover, it is well known that FCNC processes related to Higgs-boson
physics are also very sensitive to supersymmetric quantum
effects~\cite{Maria,nos,dedes,Demir,radFCNC,santi,kolda,oldchanko,alemanes,newisidori}.
In particular, large rates of neutral Higgs decays into two quarks of
different flavours have been predicted~\cite{Maria,nos,santi}.\footnote{%
        In the following, $\BR(\Hbs)$ denotes the sum of the Higgs
        branching ratios into $b\bar s$ and $\bar bs$.  The Higgs boson
        $H$ stands for that of the SM, $H\sub{SM}$, or one of
        those of the MSSM, $h^0$, $H^0$, or $A^0$.}
In the SM, one finds $\BR(H\sub{SM}\to bs) \approx 4\times 10^{-8}$ for
$m_{H\sub{SM}}= 114$ GeV.  For the neutral MSSM Higgs bosons the
ratios could be of $\Ord(10^{-4}$--$10^{-3})$.  Constraints from $\bsg$
data reduce these rates, though~\cite{santi,nos}.

In this paper we provide a phenomenological analysis of the general
constraints on flavour-changing neutral Higgs decays $H\to b\bar s,
s\bar b$, set by bounds from $\bsg$ on the flavour-mixing parameters in
the squark mass matrices of the MSSM with NMFV.  We include the SM and
the full genuine SUSY contributions by taking into account their
interference and, in particular, the influence of several
flavour-changing parameters contributing simultaneously.  Since the full
diagrammatic approach is used, our computation is valid for all values
of the characteristic parameter measuring the squark-mixing strength,
beyond the mass-insertion approximation, and for all values of
$\tan\beta$.  Previous analyses of bounds on SUSY flavour-mixing
parameters from $\bsg$~\cite{hurth} have shown the importance of the
interference effects between the different types of flavour
violation~\cite{9604387}.  In the present work we derive predictions for
$\BR(\Hbs)$ compatible with present experimental $\bsg$ bounds
and recent data from $B\to X_s\mu^+\mu^-$, assuming
first one and then several types of flavour mixing contributing at a
time for comparison.

The paper is organized as follows.  In Section \ref{sect:FC_MSSM} the
squark mass matrices in the MSSM with NMFV are described in detail and
the notation is introduced.  The numerical analysis of the branching
ratios $\BR(\Hbs)$
compatible with the observed decay rates for $B\to X_s\gamma$ and
$B\to X_s\mu^+\mu^-$ is included in
Section \ref{sect:Higgsdecays}.  In that section, we consider only one
specific flavour-mixing parameter different from zero and discuss the
interference effects of the SM and the new physics contributions.  The
interplay between $\Hbs$ and $\bsg$ is presented in Section
\ref{sect:interplay}.  The constraints on flavour-changing neutral heavy
Higgs-boson decays due to different types of flavour violation are
derived there.  Conclusions are given in Section 5.  The relevant
Feynman rules are listed in Appendix \ref{sect:frules}.

\section{Non-minimal Flavour Mixing in the MSSM}
\label{sect:FC_MSSM}

In the MSSM there are two sources of flavour violation.  The first one
arises from different rotations of the $d$- and $u$-quark fields
from the interaction to the physical bases, and its strength is driven
by the off-diagonal CKM-matrix elements, as in the SM.
The second one consists of a
possible misalignment between the rotations that
diagonalize the quark and squark sectors (NMFV).
The part of the soft-SUSY-breaking Lagrangian responsible for
this non-minimal squark family mixing is given by
\begin{align}
\label{eq:lagrangian}
\mathcal{L}^{\text{squark}}_{\text{soft}} &=
-\tilde Q_i^\dagger (M_{\tilde Q}^2)_{ij} \tilde Q_j
-\tilde U_i^\dagger (M_{\tilde U}^2)_{ij} \tilde U_j
-\tilde D_i^\dagger (M_{\tilde D}^2)_{ij} \tilde D_j \nonumber \\
&\quad + y^u_i A^u_{ij} \tilde Q_i H_u \tilde U_j
+ y^d_i A^d_{ij} \tilde Q_i H_d \tilde D_j\,,
\end{align}
where $\tilde Q$ is the SU(2) scalar doublet, $\tilde U$, $\tilde D$ are
the up- and down-squark SU(2) singlets, respectively, $y^{u,d}$ are the
Yukawa couplings and $i,j$ are generation indices.  The flavour-changing
effects come from the non-diagonal entries in the bilinear terms
$M_{\tilde Q}^2$, $M_{\tilde U}^2$, and $M_{\tilde D}^2$, and from the
trilinear terms $A_u$ and $A_d$.

We assume that the non-CKM squark mixing is significant only for
transitions between the
squarks of the second and third generations.  They are expected to be
the largest in Grand Unified Models and are also experimentally the
least constrained.  The most stringent bounds are set by $\bsg$.  In
contrast, there exist strong experimental bounds involving the first
squark generation, based on data from $K^0$--$\bar K^0$ and $D^0$--$\bar
D^0$ mixing~\cite{9604387,ciuchini}.

Our parameterization of the flavour-non-diagonal squark mass
matrices for the up- and down-type squarks, for the MSSM with real
parameters, reads as follows,
\begin{equation}
\label{eq:usquarkmass}
M^2_{\tilde u} = \left(\begin{array}{ccc|ccc}
\ML{u}^2 & 0 & 0 & m_u X_u & 0 & 0 \\
0 & \ML{c}^2 & \Delta_\LL^u & 0 & m_c X_c & \Delta_\LR^u \\
0 & \Delta_\LL^u & \ML{t}^2 & 0 & \Delta_\RL^u & m_t X_t \\[.3ex]
\hline
m_u X_u & 0 & 0 & \MR{u}^2 & 0 & 0 \\
0 & m_c X_c & \Delta_\RL^u & 0 & \MR{c}^2 & \Delta_\RR^u \\
0 & \Delta_\LR^u & m_t X_t & 0 & \Delta_\RR^u & \MR{t}^2
\end{array}\right)\,,
\end{equation}
\begin{equation}
\label{eq:dsquarkmass}
M^2_{\tilde d} = \left(\begin{array}{ccc|ccc}
\ML{d}^2 & 0 & 0 & m_d X_d & 0 & 0 \\
0 & \ML{s}^2 & \Delta_\LL^d & 0 & m_s X_s & \Delta_\LR^d \\
0 & \Delta_\LL^d & \ML{b}^2 & 0 & \Delta_\RL^d & m_b X_b \\[.3ex]
\hline
m_d X_d & 0 & 0 & \MR{d}^2 & 0 & 0 \\
0 & m_s X_s & \Delta_\RL^d & 0 & \MR{s}^2 & \Delta_\RR^d \\
0 & \Delta_\LR^d & m_b X_b & 0 & \Delta_\RR^d & \MR{b}^2
\end{array}\right)\,,
\end{equation}
where
\begin{equation}
\begin{aligned}
\label{eq:squarkparam}
\ML{q}^2 &=
  M_{\tilde Q,q}^2 + m_q^2 + \cos2\beta (T_3^q - Q_q s_W^2) m_Z^2\,, \\
\MR{\{u,c,t\}}^2 &=
  M_{\tilde U,\{u,c,t\}}^2 + m_{u,c,t}^2 + \cos2\beta Q_t s_W^2 m_Z^2\,, \\
\MR{\{d,s,b\}}^2 &=
  M_{\tilde D,\{d,s,b\}}^2 + m_{d,s,b}^2 + \cos2\beta Q_b s_W^2 m_Z^2\,, \\
X_{u,c,t} &= A_{u,c,t} - \mu\cot\beta\,, \\
X_{d,s,b} &= A_{d,s,b} - \mu\tan\beta\,,
\end{aligned}
\end{equation}
with $m_q$, $T_3^q$, $Q_q$ the mass, isospin, and electric charge of the
quark $q$, $m_Z$ the $Z$-boson mass, $s_W \equiv \sin\theta_W$,
$\theta_W$ the electroweak mixing angle, and $\mu$ the Higgsino mass
parameter.

We define the dimensionless flavour-changing parameters
$(\delta^{u,d}_{ab})_{23}$ $(ab = \LL,\LR,\RL,\RR)$ from the
flavour-off-diagonal elements of the squark mass matrices
(\ref{eq:usquarkmass}) and (\ref{eq:dsquarkmass}) in the following way,
\begin{equation}
\begin{aligned}
\label{eq:FCparam}
\Delta_\LL^u &\equiv \deu\LL \ML{c} \ML{t}\,,\quad &
\Delta_\LL^d &\equiv \ded\LL \ML{s} \ML{b}\,, \\
\Delta_\LR^u &\equiv \deu\LR \ML{c} \MR{t}\,,\quad &
\Delta_\LR^d &\equiv \ded\LR \ML{s} \MR{b}\,, \\
\Delta_\RL^u &\equiv \deu\RL \MR{c} \ML{t}\,,\quad &
\Delta_\RL^d &\equiv \ded\RL \MR{s} \ML{b}\,, \\
\Delta_\RR^u &\equiv \deu\RR \MR{c} \MR{t}\,,\quad &
\Delta_\RR^d &\equiv \ded\RR \MR{s} \MR{b}\,.
\end{aligned}
\end{equation}
In our phenomenological study, they are free parameters determining the
size of NMFV induced by SUSY and are analogous to those defined in the
mass-insertion approximation~\cite{9604387}.

In order to diagonalize the two $6\times 6$ squark-mass matrices given
above, the $6\times 6$ matrices $R^{\tilde u}$ for the up-type squarks and
$R^{\tilde d}$ for the down-type squarks are needed,
\begin{equation}
\tilde u_\sigma = R^{\tilde u}_{\sigma,j} \begin{pmatrix}
  \tilde u_L \\
  \tilde c_L \\
  \tilde t_L \\
  \tilde u_R \\
  \tilde c_R \\
  \tilde t_R
\end{pmatrix}_j\,, \quad
\tilde d_\sigma = R^{\tilde d}_{\sigma,j} \begin{pmatrix}
  \tilde d_L \\
  \tilde s_L \\
  \tilde b_L \\
  \tilde d_R \\
  \tilde s_R \\
  \tilde b_R
\end{pmatrix}_j\,.
\end{equation}

The diagonalization yields the squark mass eigenvalues and eigenstates
depending on the flavour-mixing parameters $\de{ab}$, i.e.\ $R^{\tilde
q} M_{\tilde q}^2 R^{\tilde q\dagger} = \diag(M^2_{\tilde
q_1},\dots,M^2_{\tilde q_6})$.  The dependence of the squark masses on
$\de\LL$ has already been studied in~\cite{Maria}.  Typically, out of
the four eigenvalues involving the second and third generations, two are
weakly dependent on the amount of flavour mixing and for the other two,
one grows and the other decreases with $\de\LL$.  In general,
flavour mixing through the flavour non-diagonal entries in the squark
mass matrices generates large splittings between the squark mass
eigenvalues.

\section{Flavour-changing decay processes}
\label{sect:Higgsdecays}

We focus here on the loop-induced flavour-changing decays of the MSSM
heavy neutral Higgs bosons $H = H^0, A^0$ into second- and
third-generation quarks, $H\to b\bar s, s\bar b$
(an independent analysis for the lightest Higgs boson $h^0$
will be reported elsewhere~\cite{future}).
We include the
contributions from SM particles and their superpartners (squarks,
gluinos, charginos, and neutralinos), as well as those from the MSSM
Higgs sector, and also their interference effects.  We use the full
diagrammatic approach for arbitrary values of $\tan\beta$  and of the
flavour-mixing parameters $\deud{ab}$.
Note that $\bsg$ constrains
$\ded{ab}$ only.  For simplicity, we take the same values for the
flavour-mixing parameters in the up- and down-squark sectors:
$\de{ab}\equiv\deu{ab} = \ded{ab}$.  Actually, the LL blocks of the up-
and down-squark mass matrices are related by the SU(2)$_L$ gauge
symmetry \cite{9604387}, therefore a large difference between $\deu\LL$
and $\ded\LL$ is not allowed.  For the same reason,
$\MQ{u}\approx\MQ{d}$, $\MQ{c}\approx\MQ{s}$, and $\MQ{t}\approx\MQ{b}$.

We have taken the expression for the branching ratio $\BR(B\to X_s\gamma)$ to NLO
from \cite{Kagan}. In the MSSM with NMFV, the relevant operators of the effective
Hamiltonian are
\begin{equation}
\begin{aligned}
O_2 &= \bar s_L\gamma_\mu c_L\gamma^\mu b_L ,\\
O_7 &= \frac{e}{16\pi^2}m_b \bar s_L \sigma_{\mu\nu}F^{\mu\nu} b_R,\quad
&\tilde O_7 &= \frac{e}{16\pi^2}m_b \bar s_R \sigma_{\mu\nu}F^{\mu\nu} b_L,\\
O_8 &= \frac{g_s}{16\pi^2}m_b \bar s_L\sigma_{\mu\nu}G^{\mu\nu}_a t_a b_R,\quad
&\tilde O_8 &= \frac{g_s}{16\pi^2}m_b \bar s_R\sigma_{\mu\nu}G^{\mu\nu}_a t_a b_L.\\
\end{aligned}
\end{equation}
We have calculated the corresponding Wilson coefficients $C_{2,7,8}$ and
$\tilde C_{7,8}$ to one loop. The tilded operators do not contribute in the SM or
in the MSSM with MFV, in the limit of massless strange quark.
The data from $B\to X_s\mu^+\mu^-$ require that the sign of the coefficient
$C_7(m_b)$ is the same as in the SM.

We used \textsl{FeynArts}, \textsl{FormCalc}, and \textsl{LoopTools} to
obtain our results.  To this end, we had to modify the MSSM model file of
\textsl{FeynArts} to include general flavour mixing,  and  we added
$6\times 6$ squark mass and mixing matrices to the \textsl{FormCalc}
evaluation \cite{hahn,thtalk}.  A list of the Feynman rules needed for our
computation is given in Appendix A.
The masses and total decay widths of the Higgs bosons were computed with
{\sl FeynHiggs}~\cite{Feynhiggs}.

For a concrete evaluation,
we choose the following six flavour-diagonal MSSM parameters
as input parameters: $m_A$,
$\tan \beta$, $\mu$, $M_{2}$, $M\sub{SUSY}$, $A$, where $m_A$ denotes the mass
of the CP-odd Higgs boson $A^0$.
For simplicity, we have taken a common value for the soft SUSY-breaking
squark mass parameters $M\sub{SUSY}\equiv \MU{\{u,t,c\}} =
\MD{\{d,b,s\}}$, and all the various trilinear parameters to be
universal, $A\equiv A_t = A_b = A_c = A_s$.  These parameters and the
$\delta$'s will be varied over a wide range, subject only to the
requirements that all the squark masses be heavier than 100 GeV,
$|\mu| > 90$ GeV and $M_2 > 46$ GeV~\cite{pdg2004}.

The following MSSM parameters have been chosen as a default set
(if not specified differently),
\begin{equation}
\label{eq:numparameters}
\begin{gathered}
M\sub{SUSY} = 800\text{ GeV}\,, \quad
M_2 = 300\text{ GeV}\,, \quad
M_1 = \frac 53 \frac{s_W^2}{c_W^2} M_2\,, \\
A   = 500\text{ GeV}\,, \quad
m_A = 400\text{ GeV}\,, \quad
\tan\beta = 35\,, \quad
\mu = -700\text{ GeV}\,.
\end{gathered}
\end{equation}
A detailed study of the values of the Higgs-boson decay widths in
a wider range of these parameters and for $\deu\LL \neq 0$
has been done in~\cite{nos}.

Let us remark that the $\mu$-parameter plays an important role in our
analysis.  The $H^0$ decay width is approximately symmetric under $\mu
\to -\mu$, depending on the $m_A$ values, and increases with $\mu$ up to
a certain value around $600$ GeV; then it reaches a maximum value, and
finally decreases~\cite{Maria,nos}.  Moreover, the $\mu$-parameter
enters in the gluino and chargino contributions to $\bsg$, producing
significant cancellations at large $\tan\beta$.

For illustration, we give in this section an overview over
the various contributions
to both $\Hzbs$ and $B \to X_s\gamma$, keeping only a single
flavour-off-diagonal element, $\de\LL$. For the Higgs decays, we agree with
the results of previous studies on the subject~\cite{Maria,nos,santi}.

\begin{figure}
\begin{center}
\begin{tabular}{cc}
\includegraphics[width=.45\hsize]{brlambdaHbs.eps} &
\includegraphics[width=.45\hsize]{brlambdabsg.eps} \\
\includegraphics[width=.45\hsize]{brlambdaHbsnoGUT.eps} &
\includegraphics[width=.45\hsize]{brlambdabsgnoGUT.eps} \\
\end{tabular}
\end{center}
\vspace*{-3ex}
\caption{\label{fig:contrib}$\BR(\Hzbs)$ [left] and
$\BR(B\to X_s\gamma)$ [right] as a function of $\de\LL$.  In the
upper row $\MGl$ is determined from $M_2$ through the GUT relation, in
the lower row $\MGl = 300$~GeV is chosen.  The other input parameters
are given in Eq.~(\ref{eq:numparameters}). The SM and the MSSM Higgs
sector contributions (sH) are included (horizontal lines in
$\BR(B\to X_s\gamma)$ [right], but invisible in $\BR(\Hzbs)$ [left]).}
\end{figure}

Fig.~\ref{fig:contrib} shows on the left $\BR(\Hzbs)$ and on the right
$\BR(B\to X_s\gamma)$ as a function of $\de\LL$.  In the upper row the GUT
relation $M_3 = \alpha_s/(\alpha s_W^2) M_2$ is assumed, yielding the
rather large gluino mass of $\MGl\approx 1$ TeV. In the lower row $\MGl
= 300$ GeV is chosen.

Our purpose is to show the size of the radiative corrections separately
for the different sectors and their interference effects.  The SUSY
electroweak (SUSY-EW) contribution includes charginos, neutralinos, and
the MSSM Higgs sector, the latter being negligible in $\Hzbs$ but
important in $\bsg$ (horizontal lines in $\BR(\bsg)$ because they do not
depend on $\de\LL$). The chargino and neutralino contributions are
plotted independently to show that in both cases the charginos dominate.
Gluino--squark loops constitute the SUSY-QCD contribution.

$\BR(\Hzbs)$ increases with $\de\LL$, as already
known~\cite{Maria,nos,santi}.
We can see that the SUSY-QCD contribution is dominant,
at least one order of magnitude larger than that of SUSY-EW.  Both
interfere with opposite signs, as discussed in~\cite{nos}.  The SM value
for the Higgs branching ratio is several orders of magnitude smaller
than the corresponding MSSM value, of $\Ord(10^{-8})$.

In $\bsg$, the SUSY-QCD contribution is also dominant in most of the
flavour parameter space, but becomes subdominant for large gluino masses
(see the upper row in Fig.~\ref{fig:contrib}).
This result, however, strongly depends on the choice of parameters
and changes if the GUT relation is relaxed.
The interference effects of the
various MSSM sectors in $\bsg$ must therefore be carefully considered.

\section{Compatibility between $\Hzbs$  and $\bsg$}
\label{sect:interplay}

Next we derive the maximum values of $\BR(H^0 \to b s)$ compatible with
$\BR(B\to X_s\gamma)\sub{exp} = (3.3\pm 0.4)\times 10^{-4}$
\cite{boundsbsg} within three standard deviations by varying the
flavour-changing parameters of the squark mass matrices.
The results for the $A^0$ boson are very similar and we do not show them
separately.

\subsection{One flavour-mixing parameter}

As a first step, we select one possible type of flavour violation in the
squark sector, assuming that all the others vanish.  The interference
between different types of flavour mixing is thus ignored.  Previous
analyses on bounds coming from $\bsg$, by using the mass-insertion
approximation and by neglecting any kind of interference effects, led to
bounds on the single off-diagonal element for the down sector of
$|\ded{\LL,\RR}| < \Ord(1)$, $|\ded{\LR,\RL}| < \Ord(10^{-2})$
(see~\cite{9604387,hurth} and references therein).  The MSSM inputs are
those in Eq.~(\ref{eq:numparameters}) with GUT relations.

\begin{figure}
\begin{center}
\includegraphics{lambdabsg}
\end{center}
\vspace*{-3ex}
\caption{\label{fig:stddev}$\Delta\BR(B\to X_s\gamma)$ in standard
deviations (see text) as a function of $\de{\LL,\LR,\RL,\RR}$. The thinner
lines for $\de{\LL}$ and $\de{\LR}$ correspond to regions disfavoured by
$B\to X_s\mu^+\mu^-$.}
\end{figure}

In Fig.~\ref{fig:stddev} we show $\BR(B\to X_s\gamma)$ as a function of the
flavour parameters $\de{ab}$ with $ab = \LL,\LR,\RL,\RR$.  The results
are expressed in standard deviations (s.d.) through
\begin{equation}
\frac{\Delta\BR(B\to X_s\gamma)}{1\text{ s.d.}}=
  \frac{\BR(B\to X_s\gamma)-\BR(B\to X_s\gamma)\sub{exp}}{\Delta\BR\sub{exp}}\,.
\label{DeltaBR}
\end{equation}

We can see in Fig.~\ref{fig:stddev} that the flavour-off-diagonal
elements are independently constrained to be at most $\de{ab}\sim
10^{-3}$--$10^{-1}$.  As expected~\cite{9604387,hurth}, the bounds on
$\de\LR$ are the strongest, $\de\LR\sim 10^{-3}$--$10^{-2}$. The
data from $B\to X_s\mu^+\mu^-$ further constrain the parameters $\de{\LL}$
and $\de{\LR}$, the others remaining untouched.

\begin{figure}
\begin{center}
\begin{tabular}{cc}
\includegraphics[width=.45\hsize]{lambdaHbs.LL.eps} &
\includegraphics[width=.45\hsize]{lambdaHbs.RR.eps} \\
\includegraphics[width=.45\hsize]{lambdaHbs.LR.eps} &
\includegraphics[width=.45\hsize]{lambdaHbs.RL.eps}
\end{tabular}
\end{center}
\vspace*{-3ex}
\caption{\label{fig:Hbs}$\BR(\Hzbs)$ as a function of
$\de{\LL,\RR,\LR,\RL}$.  The allowed intervals of these
parameters determined from $\bsg$ (see Fig.~\ref{fig:stddev}) are
indicated by coloured areas. The red areas (b) are disfavoured by
$B\to X_s\mu^+\mu^-$.}
\end{figure}

The allowed intervals for the corresponding flavour-mixing parameters
thus obtained are indicated in
Fig.~\ref{fig:Hbs}, in which we present the results for $\BR(\Hzbs)$ as
a function of $\de{ab}$.  The predictions compatible with the $\bsg$
constraints can be read off directly from there.

For our reference point (\ref{eq:numparameters}) we find that the
largest allowed value of $\BR(\Hzbs)$, of $\Ord(10^{-3})$ or $\Ord(10^{-5})$,
is induced by $\de\RR$ or $\de\LL$, respectively.
These are the flavour-changing parameters least
stringently constrained by the $\bsg$ data.  $\BR(\Hzbs)$ can reach
$\Ord(10^{-6})$ if induced by $\de\LR$ or by $\de\RL$, the most stringently
constrained flavour-changing parameter.
We remark that, because of the restrictions imposed by $\bsg$, $\BR(\Hzbs)$
depends very little on $\de\LR$ and $\de\RL$.

\subsection{Two flavour-mixing parameters}

In this second part of our analysis, we investigate whether the maximum
values reachable by the $H^0$ branching ratios remain stable when
several off-diagonal elements of the squark mass matrix contribute
simultaneously.  It is known that the participation of several types of
flavour-changing parameters weaken the bounds, imposed by $\bsg$, on the
off-diagonal elements of the squark-mass matrix by at least one order of
magnitude~\cite{hurth}.  We derive bounds on these flavour-mixing
parameters by switching on simultaneously two of those parameters, with
all the others vanishing.  Indeed, we performed the analysis for all
possible combinations of two of the four dimensionless parameters
(\ref{eq:FCparam}).

\begin{figure}
\begin{center}
\begin{tabular}{cc}
\includegraphics[height=.42\hsize]{Hbs-bsg.RL.LR.eps} &
\includegraphics[height=.42\hsize]{Hbs-bsg.RR.LR.eps} \\[1ex]
\includegraphics[height=.42\hsize]{Hbs-bsg.LL.LR.eps} &
\includegraphics[height=.42\hsize]{Hbs-bsg.RR.RL.eps} \\[1ex]
\includegraphics[height=.42\hsize]{Hbs-bsg.LL.RL.eps} &
\includegraphics[height=.42\hsize]{Hbs-bsg.LL.RR.eps}
\end{tabular}
\end{center}
\vspace*{-3ex}
\caption{\label{fig:planes}Contours of constant $\Gamma(\Hzbs)$ in
various planes of the flavour-mixing parameters $\de{ab}$.  The coloured
bands indicate regions experimentally allowed by $B\to X_s\gamma$. The red
bands show regions disfavoured by $B\to X_s\mu^+\mu^-$.}
\end{figure}

Fig.~\ref{fig:planes} displays the results for our parameter set
(\ref{eq:numparameters}).  Drawn are contours of constant
$\Gamma(\Hzbs)\equiv \Gamma(H^0\to b\bar s) + \Gamma(H^0\to s\bar b)$
for various combinations $\de{ab}$--$\de{cd}$ of flavour-mixing
parameters, which we shall refer to as ``$ab$--$cd$ planes'' for short
in the following.  The coloured bands represent regions experimentally
allowed by $B\to X_s\gamma$. The red bands are regions disfavoured by
$B\to X_s\mu^+\mu^-$.

Contributions in the $\LR$--$\RL$ and $\LR$--$\RR$ planes lead to
maximal values
\begin{align}
\Gamma(\Hzbs)\sub{max} &= 3\times 10^{-4}\text{ GeV}
&\text{for } \de\LR &= 0.04, & \de\RL &= 0.04\,, \\
\Gamma(\Hzbs)\sub{max} &= 0.15\text{ GeV}
&\text{for } \de\LR &= 0.035, & \de\RR &= \pm0.7\,.
\end{align}
This translates to branching ratios compatible with experimental data
of $\BR(\Hzbs)\sub{max}\sim 10^{-5}$ in the first, and
$\Ord(10^{-3})$ in the second case.  Here we have used the total
width of $\Gamma(H\to X)\approx 26$ GeV, $H = H^0, A^0$, for the point
(\ref{eq:numparameters}) in the MSSM with MFV.

The bounds on $\de\LR$, the best constrained for only one non-zero
flavour-off-diagonal element, are dramatically relaxed when
other flavour-changing parameters contribute simultaneously.  Values of
$\de\LR\sim 10^{-1}$ are allowed.  In particular, large although
fine-tuned values of $\de\LL$ and $\de\LR$ combined are not excluded by
$\bsg$, yielding e.g.
\begin{align}
\Gamma(\Hzbs)\sub{max} &= 0.25\text{ GeV}
&\text{for } \de\LR &= -0.22, & \de\LL &= -0.8\,, \\
\Gamma(\Hzbs)\sub{max} &= 0.35\text{ GeV}
&\text{for } \de\RL &= \pm0.04, & \de\RR &= -0.15\,.
\end{align}
The branching ratio is $\BR(\Hzbs)\sub{max}\sim 10^{-2}$ in both
cases.

Finally, we studied the combined effects of $\RL$--$\LL$ and
$\RR$--$\LL$.  We obtain
\begin{align}
\Gamma(\Hzbs)\sub{max} &= 2.5\times 10^{-3}\text{ GeV}
&\text{for } \de\RL &= 0.006, & \de\LL &= -0.128\,, \\
\Gamma(\Hzbs)\sub{max} &= 0.12\text{ GeV}
&\text{for } \de\RR &= 0.65, & \de\LL &= \pm0.14\,.
\end{align}
This means $\BR(\Hzbs)\sub{max}\sim 10^{-4}$ for the $\RL$--$\LL$
and $\BR(\Hzbs)\sub{max}\sim 10^{-2}$ for the $\RR$--$\LL$ case.

Therefore, we conclude that the predictions on $\BR(\Hzbs)$ induced by
$\de\RR$ or $\de\LL$ only, of $\Ord(10^{-3})$ or $\Ord(10^{-5})$, are greatly
exceeded by the combination of $\de\LL$ and $\de\LR$ or $\de\RR$ and $\de\RL$ or
$\de\LL$ and $\de\RR$, which are of $\Ord(10^{-2})$.  Values of
$\BR(\Hzbs)\sim \Ord(10^{-3})$ emerge when considering the $\LR$--$\RR$.
Thus, the destructive interference of the
combined set of flavour-mixing parameters leads to large allowed values
for the $\Hzbs$ branching ratio, which in general can be two orders of
magnitude larger than if induced by just one flavour-mixing parameter.

\section{Conclusions}

In this work we carried out a phenomenological analysis of the
predictions for flavour-changing neutral heavy Higgs decays $H\to b\bar
s,s\bar b$, taking into account the constraints from $\bsg$ on the
flavour-mixing parameters $\de{\LL,\LR,\RL,\RR}$ of the MSSM with NMFV.
We followed a fully diagrammatic approach at one loop, valid for
arbitrary values of $\tan\beta$ and the $\delta$'s, as long as they are
kinematically allowed.  The calculations were performed with
\textsl{FeynArts}, \textsl{FormCalc}, and \textsl{LoopTools}, which were
extended to include the MSSM with NMFV in a new model file and the
corresponding $6\times 6$ diagonalization, both of which are now
available in the public distributions of \textsl{FeynArts} and
\textsl{FormCalc}.  The contributions and interfering effects of the SM
and the various sectors of the MSSM were fully accounted for and the
interplay between the different types of non-minimal flavour mixing
explored, both individually and in combinations.

We found that $\BR(\Hbs)$, whose value is at most of $\Ord(10^{-6})$
when induced by $\de\RL$ or $\de\LR$, can be of $\Ord(10^{-5})$
or $\Ord(10^{-3})$ if induced by $\de\RR$ or $\de\LL$.  By imposing
the constraints from $\bsg$ over the flavour-changing parameters, the
$\Hbs$ branching ratio depends only weakly on $\de\RL$ and $\de\LR$.
The combined effect of two of the flavour-mixing parameters may raise
the predictions for $\BR(\Hbs)$ by one or two orders of magnitude,
typically $\Ord(10^{-3}$--$10^{-2})$.

Overall, the predictions for $H\to b\bar{s}$ are more optimistic when
the bounds from $\bsg$ are accounted for in the more realistic case of
several flavour-mixing parameters contributing simultaneously.

\section*{Acknowledgements}

We thank D.~St\"ockinger, S.~Heinemeyer, J.~Guasch and J.~Prades
for very helpful discussions.  The work of S.P.\ has been supported by the
European Union under contract No.~MEIF-CT-2003-500030.  J.I.I.\ acknowledges the
financial support by the E.U.\ (HPRN-CT-2000-149), the Spanish MCYT
(FPA2003-09298-C02-01) and Junta de Andaluc{\'\i}a (FQM-101).

\begin{appendix}

\section{NMFV Feynman Rules}
\label{sect:frules}

The following table lists Feynman rules needed for our computation in
the MSSM with NMFV.  These vertices were generated automatically from
the new \textsl{FeynArts} model file FVMSSM.mod, available from
www.feynarts.de.

The upper and lower entries of the FFS couplings are the prefactors of
the left- and right-handed chirality projectors.  The matrices
$T_{ab}^g$ are the SU(3) generators with gluon index $g$ and colour
indices $a$, $b$.  The matrices $U$, $V$ ($Z$) are the chargino
(neutralino) mixing matrices and CKM is the Cabibbo--Kobayashi--Maskawa
quark mixing matrix, with $i,j$ the fermion and $\rho,\sigma$ the squark
generation indices.  The angle $\alpha$ is the mixing angle in the
neutral Higgs sector.

\begin{small}
\noindent
\begin{longtable}{p{.97\linewidth}}
\Coupling{FFS}{Gluino -- Quark -- Squark}
$
{C}(\tilde g,\Bar{u_i},\tilde u_{\sigma}) = { }
\begin{CoupVec}
\sqrt 2\,\ii\,g_s\,R_{\sigma,3 + {i}}^{\tilde u*}\,T_{ab}^g\\
\\[-3ex]
-\sqrt 2\,\ii\,g_s\,R_{\sigma,{i}}^{\tilde u*}\,T_{ab}^g
\end{CoupVec}
$\\
\bigskip
$
{C}(\tilde g,\Bar{d_i},\tilde d_{\sigma}) = { }
\begin{CoupVec}
\sqrt 2\,\ii\,g_s\,R_{\sigma,3 + {i}}^{\tilde d*}\,T_{ab}^g\\
\\[-3ex]
-\sqrt 2\,\ii\,g_s\,R_{\sigma,{i}}^{\tilde d*}\,T_{ab}^g
\end{CoupVec}
$\\
\bigskip
$
{C}(\tilde g,u_i,\tilde u_{\sigma}^{\dagger}) = { }
\begin{CoupVec}
-\sqrt 2\,\ii\,g_s\,R_{\sigma,{i}}^{\tilde u}\,T_{ba}^g\\
\\[-3ex]
\sqrt 2\,\ii\,g_s\,R_{\sigma,3 + {i}}^{\tilde u}\,T_{ba}^g
\end{CoupVec}
$\\
\bigskip
$
{C}(\tilde g,d_i,\tilde d_{\sigma}^{\dagger}) = { }
\begin{CoupVec}
-\sqrt 2\,\ii\,g_s\,R_{\sigma,{i}}^{\tilde d}\,T_{ba}^g\\
\\[-3ex]
\sqrt 2\,\ii\,g_s\,R_{\sigma,3 + {i}}^{\tilde d}\,T_{ba}^g
\end{CoupVec}
$\\
\bigskip
\Coupling{FFS}{Chargino -- Quark -- Squark}
$
{C}(\tilde \chi_{{c}}^{-},\Bar{d_j},\tilde u_{\sigma}) = { }
\begin{CoupVec}
\sum\limits_{{i}=1}^{3}
\frac{\ii\,e\,m_{d_j}\,{\rm CKM}_{ij}^{*}\,R_{\sigma,{i}}^{\tilde u*}\,U_{c2}^{*}}{\sqrt 2\,c_\beta\,M_W\,s_W}\\
\\[-3ex]
-\sum\limits_{{i}=1}^{3}
\frac{\ii\,e\,{\rm CKM}_{ij}^{*}}{2\,M_W\,s_\beta\,s_W}\,\left( 2\,M_W\,R_{\sigma,{i}}^{\tilde u*}\,s_\beta\,V_{c1} - \sqrt 2\,m_{u_i}\,R_{\sigma,3 + {i}}^{\tilde u*}\,V_{c2} \right)
\end{CoupVec}
$\\
\bigskip
$
{C}(\tilde \chi_{{c}}^{+},\Bar{u_i},\tilde d_{\sigma}) = { }
\begin{CoupVec}
\sum\limits_{{j}=1}^{3}
\frac{\ii\,e\,m_{u_i}\,{\rm CKM}_{ij}\,R_{\sigma,{j}}^{\tilde d*}\,V_{c2}^{*}}{\sqrt 2\,M_W\,s_\beta\,s_W}\\
\\[-3ex]
-\sum\limits_{{j}=1}^{3}
\frac{\ii\,e\,{\rm CKM}_{ij}}{2\,c_\beta\,M_W\,s_W}\,\left( 2\,c_\beta\,M_W\,R_{\sigma,{j}}^{\tilde d*}\,U_{c1} - \sqrt 2\,m_{d_j}\,R_{\sigma,3 + {j}}^{\tilde d*}\,U_{c2} \right)
\end{CoupVec}
$\\
\bigskip
$
{C}(d_j,\tilde \chi_{{c}}^{+},\tilde u_{\sigma}^{\dagger}) = { }
\begin{CoupVec}
-\sum\limits_{{i}=1}^{3}
\frac{\ii\,e\,{\rm CKM}_{ij}}{2\,M_W\,s_\beta\,s_W}\,\left( 2\,M_W\,R_{\sigma,{i}}^{\tilde u}\,s_\beta\,V_{c1}^{*} - \sqrt 2\,m_{u_i}\,R_{\sigma,3 + {i}}^{\tilde u}\,V_{c2}^{*} \right) \\
\\[-3ex]
\sum\limits_{{i}=1}^{3}
\frac{\ii\,e\,m_{d_j}\,{\rm CKM}_{ij}\,R_{\sigma,{i}}^{\tilde u}\,U_{c2}}{\sqrt 2\,c_\beta\,M_W\,s_W}
\end{CoupVec}
$\\
\bigskip
$
{C}(u_i,\tilde \chi_{{c}}^{-},\tilde d_{\sigma}^{\dagger}) = { }
\begin{CoupVec}
-\sum\limits_{{j}=1}^{3}
\frac{\ii\,e\,{\rm CKM}_{ij}^{*}}{2\,c_\beta\,M_W\,s_W}\,\left( 2\,c_\beta\,M_W\,R_{\sigma,{j}}^{\tilde d}\,U_{c1}^{*} - \sqrt 2\,m_{d_j}\,R_{\sigma,3 + {j}}^{\tilde d}\,U_{c2}^{*} \right) \\
\\[-3ex]
\sum\limits_{{j}=1}^{3}
\frac{\ii\,e\, m_{u_i}\,{\rm CKM}_{ij}^{*}\,R_{\sigma,{j}}^{\tilde d}\,V_{c2}}{\sqrt 2\,M_W\,s_\beta\,s_W}
\end{CoupVec}
$\\
\bigskip
\Coupling{FFS}{Neutralino -- Quark -- Squark}
$
{C}(\tilde \chi_{{n}}^{0},\Bar{u_i},\tilde u_{\sigma}) = \newline
\begin{CoupVec}
\frac{\ii\,e}{3\,\sqrt 2\,c_W\,M_W\,s_\beta\,s_W}\,
\left( 4\,M_W\,R_{\sigma,3 + {i}}^{\tilde u*}\,s_\beta\,s_W\,Z_{n1}^{*} - 3\,c_W\,m_{u_i}\,R_{\sigma,{i}}^{\tilde u*}\,Z_{n4}^{*} \right) \\
\\[-3ex]
-\frac{\ii\,e}{3\,\sqrt 2\,c_W\,M_W\,s_\beta\,s_W}\,
\left( 3\,c_W\,m_{u_i}\,R_{\sigma,3 + {i}}^{\tilde u*}\,Z_{n4} + M_W\,R_{\sigma,{i}}^{\tilde u*}\,s_\beta\,\left( s_W\,Z_{n1} + 3\,c_W\,Z_{n2} \right)  \right)
\end{CoupVec}
$\\
\bigskip
$
\vrule width 0ex height 6ex depth 0ex
{C}(\tilde \chi_{{n}}^{0},\Bar{d_i},\tilde d_{\sigma}) = \newline
\begin{CoupVec}
-\frac{\ii\,e}{3\,\sqrt 2\,c_\beta\,c_W\,M_W\,s_W}\,
\left( 2\,c_\beta\,M_W\,R_{\sigma,3 + {i}}^{\tilde d*}\,s_W\,Z_{n1}^{*} + 3\,c_W\,m_{d_i}\,R_{\sigma,{i}}^{\tilde d*}\,Z_{n3}^{*} \right) \\
\\[-3ex]
-\frac{\ii\,e}{3\,\sqrt 2\,c_\beta\,c_W\,M_W\,s_W}\,
\left( 3\,c_W\,m_{d_i}\,R_{\sigma,3 + {i}}^{\tilde d*}\,Z_{n3} + c_\beta\,M_W\,R_{\sigma,{i}}^{\tilde d*}\,\left( s_W\,Z_{n1} - 3\,c_W\,Z_{n2} \right)  \right)
\end{CoupVec}
$\\
\bigskip
$
\vrule width 0ex height 6ex depth 0ex
{C}(u_i,\tilde \chi_{{n}}^{0},\tilde u_{\sigma}^{\dagger}) = \newline
\begin{CoupVec}
-\frac{\ii\,e}{3\,\sqrt 2\,c_W\,M_W\,s_\beta\,s_W}\,
\left( M_W\,R_{\sigma,{i}}^{\tilde u}\,s_\beta\,s_W\,Z_{n1}^{*} + 3\,c_W\,\left( M_W\,R_{\sigma,{i}}^{\tilde u}\,s_\beta\,Z_{n2}^{*} + m_{u_i}\,R_{\sigma,3 + {i}}^{\tilde u}\,Z_{n4}^{*} \right)  \right) \\
\\[-3ex]
\frac{\ii\,e}{3\,\sqrt 2\,c_W\,M_W\,s_\beta\,s_W}\,
\left( 4\,M_W\,R_{\sigma,3 + {i}}^{\tilde u}\,s_\beta\,s_W\,Z_{n1} - 3\,c_W\,m_{u_i}\,R_{\sigma,{i}}^{\tilde u}\,Z_{n4} \right)
\end{CoupVec}
$\\
\bigskip
$
\vrule width 0ex height 6ex depth 0ex
{C}(d_i,\tilde \chi_{{n}}^{0},\tilde d_{\sigma}^{\dagger}) = \newline
\begin{CoupVec}
-\frac{\ii\,e}{3\,\sqrt 2\,c_\beta\,c_W\,M_W\,s_W}\,
\left( c_\beta\,M_W\,R_{\sigma,{i}}^{\tilde d}\,s_W\,Z_{n1}^{*} - 3\,c_W\,\left( c_\beta\,M_W\,R_{\sigma,{i}}^{\tilde d}\,Z_{n2}^{*} - m_{d_i}\,R_{\sigma,3 + {i}}^{\tilde d}\,Z_{n3}^{*} \right)  \right) \\
\\[-3ex]
-\frac{\ii\,e}{3\,\sqrt 2\,c_\beta\,c_W\,M_W\,s_W}\,
\left( 2\,c_\beta\,M_W\,R_{\sigma,3 + {i}}^{\tilde d}\,s_W\,Z_{n1} + 3\,c_W\,m_{d_i}\,R_{\sigma,{i}}^{\tilde d}\,Z_{n3} \right)
\end{CoupVec}
$\\
\bigskip
\Coupling{SSS}{Higgs -- 2 Squarks}
$
{C}(H^{0},\tilde u_{\rho},\tilde u_{\sigma}^{\dagger}) =\newline
{-}\displaystyle\sum\limits_{{i},{j}=1}^{3}\frac{\ii\,e}{6\,c_W\,M_W\,s_\beta\,s_W}\,
\begin{PlusB}
R_{\rho,3 + {i}}^{\tilde u*}\,
\begin{PlusB}
4\,c_{\alpha+\beta}\,\delta_{ij}\,M_W\,M_Z\,R_{\sigma,3 + {j}}^{\tilde u}\,s_\beta\,s_W^{2} \\
- 3\,c_W\,R_{\sigma,{j}}^{\tilde u}\,( c_{\alpha}\,\delta_{ij}\,m_{u_i}\,\mu - m_{u_j}\,s_{\alpha}\,A^{u*}_{ji} ) \,\\
+6\,c_W\,\delta_{ij}\,m_{u_i}^{2}\,R_{\sigma,3 + {j}}^{\tilde u}\,s_{\alpha}
\end{PlusB}\,\\
-R_{\rho,{i}}^{\tilde u*}\,
\begin{PlusB} 3\,c_W\,R_{\sigma,3 + {j}}^{\tilde u}\,( c_{\alpha}\,\delta_{ij}\,m_{u_i}\,\mu^{*} - A^u_{ij}
\,m_{u_i}\,s_{\alpha})  \\
 - \delta_{ij}\,R_{\sigma,{j}}^{\tilde u}\,( 6\,c_W\,m_{u_i}^{2}\,s_{\alpha} + c_{\alpha+\beta}\,M_W\,M_Z\,s_\beta\,( 3 - 4\,s_W^{2} ) ) \end{PlusB}
\end{PlusB}
$\\
\bigskip
$
\vrule width 0ex height 6ex depth 0ex
{C}(H^{0},\tilde d_{\rho},\tilde d_{\sigma}^{\dagger}) = \newline
\displaystyle\sum\limits_{{i},{j}=1}^{3}
\frac{{\ii}\,e}{6\,c_\beta\,c_W\,M_W\,s_W}\,{ }
\begin{PlusB}
R_{\rho,3 + {i}}^{\tilde d*}\,
\begin{PlusB}
2\,c_{\alpha+\beta}\,c_\beta\,\delta_{ij}\,M_W\,M_Z\,R_{\sigma,3 + {j}}^{\tilde d}\,s_W^{2} \\
+ 3\,c_W\,R_{\sigma,{j}}^{\tilde d}\,( \delta_{ij}\,m_{d_i}\,\mu\,s_{\alpha} - c_{\alpha}\,m_{d_j}\, A^{d*}_{ji}) \,\\
-6\,c_{\alpha}\,c_W\,\delta_{ij}\,m_{d_i}^{2}\,R_{\sigma,3 + {j}}^{\tilde d}
\end{PlusB}\,\\
-R_{\rho,{i}}^{\tilde d*}\,
\begin{PlusB}
 3\,c_W\,R_{\sigma,3 + {j}}^{\tilde d}\,( A^d_{ij}\,c_{\alpha}\,m_{d_i} - \delta_{ij}\,m_{d_i}\,\mu^{*}\,s_{\alpha} )  \\
+ \delta_{ij}\,R_{\sigma,{j}}^{\tilde d}\,( 6\,c_{\alpha}\,c_W\,m_{d_i}^{2} - c_{\alpha+\beta}\,c_\beta\,M_W\,M_Z\,( 3 - 2\,s_W^{2}))
\end{PlusB} \end{PlusB}
$\\
\bigskip
\end{longtable}
\end{small}

\end{appendix}

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