Standard model of cosmology
[Elementary Particle](https://texonom.com/elementary-particle-1281a6571c1e4eba9fd77a52ad8e2eb5) 


## ΛCDM Model
표준 우주 모형은 총 6개의 자유 변수를 사용
- [Cosmological Constant](https://texonom.com/cosmological-constant-dcd8fb5b1655474f8e4f8b607b289e10) 
- [Cold Dark Matter](https://texonom.com/cold-dark-matter-a92f7104896e44cc9cbcfc63153fb761) 
- [Hubble Constant](https://texonom.com/hubble-constant-f5e3f368d9dc4961858e3a70a67a9eef) [Big Bang](https://texonom.com/big-bang-7386a11d0b67432fbe1c31f9edeb492f)
- [Cosmic Inflation](https://texonom.com/cosmic-inflation-5ca0f64fa19643d5b4a2ddc350bee17a) [Scalar Spectral Index](https://texonom.com/scalar-spectral-index-181741b7117843939525a07514ef8451) 
- [Cosmological Constant](https://texonom.com/cosmological-constant-dcd8fb5b1655474f8e4f8b607b289e10) 
우주는 꾸준히 증가하는 암흑에너지에 의해 가속 팽창을 겪은 끝에 [ Big Freeze](https://texonom.com/big-freeze-82e5a8dac2494fd5b31b88375936bc14)  의 형태로 결말을 맞을 것으로 추정
### Standard model of cosmology Notion
|Title|
|:-:|
|[Big Bang](https://texonom.com/big-bang-7386a11d0b67432fbe1c31f9edeb492f)|
|[Cosmological principle](https://texonom.com/cosmological-principle-23c01007dee946a881843248f93d24bf)|
|[wCDM](https://texonom.com/wcdm-c1d741fac2c84e60bc8aa3ee26210709)|
|[baryon asymmetry](https://texonom.com/baryon-asymmetry-cbc3f893af304188bb5cfc4b6548611f)|
![](https://www.notion.so/image/https%3A%2F%2Fs3-us-west-2.amazonaws.com%2Fsecure.notion-static.com%2F5fd59d6c-5444-4aee-92c9-9643fbc8f6b2%2FUntitled.png?table=block&id=7ea56b18-2bba-4159-99de-7360434c7a89&cache=v2)



> [Lambda-CDM model](https://en.wikipedia.org/wiki/Lambda-CDM_model)





