Космология

Introduction to Cosmology
Sarkar, S (speaker) (The Rudolf Peierls Centre for Theoretical Physics)
Лекция 1: Seeing the edge of the universe: from speculation to science   
Лекция 2: Constructing the Universe: relativistic world models   
Лекция 3: The history of the Universe: decoupling of the relic radiation and synthesis of the light elements   
Лекция 4: The content of the Universe: baryons, dark matter and dark energy   
Лекция 5: Making sense of the Universe: fundamental physics and cosmology     

Introduction to Cosmology (Введение в космологию)
Verde, L (ICE, IEEC/CSIC, Bellaterra)
Лекция 1
Лекция 2
Лекция 3
Лекция 4
Лекция 5

Kari Enqvist
    Cosmological Inflation
    Космологическая инфляция

Valery Rubakov
    Cosmology
    Космология

• Expanding Universe. Dark matter: evidence. WIMPs ( Weakly Interacting Massive Particle). Warm dark matter: gravitinos?  (+)
  Расширяющаяся Вселенная. Темная материя: свидетельства существования. WIMPы (слабо взаимодействующие массивные частицы). Теплая темная материя: гравитино?
• Baryon asymmetry of the Universe. Dark energy (+)
  Барионная асимметрия Вселенной. Темная энергия.
• Лекция 3 (+)

Licia Verde (ICREA & ICC, Barcelona)
    Introduction to Cosmology
    Введение в космологию

The standard cosmological model. The successes of cosmology over the past 10 years. Cosmic Microwave Background. Large-scale structure. Inflation and outlook for the future.
Стандартная космологическая модель. Успехи космологии за последние 10 лет. Реликтовое микроволнового излучение. Крупномасштабная структура. Инфляция и перспективы на будущее

• Лекция 1 (+)
• Лекция 2 (+)

Pierre Binetruy (APC)
    Cosmology and gravitaton
    Космология и гравитация

• A not so brief history of cosmology
  Не очень короткая история космологии
• The days where cosmology became a quantitative science: Cosmic Microwave Background. The violent Universe.
  Дни, когда космология стала количественной наукой: реликтовое микроволновое излучение.
• Dark matter. Dark energy
  Темная материя. Темная энергия.

Hitoshi Murayama (IPMU Tokyo & LBL Berkeley)
    Cosmology, astro-particle physics and dark matter  
    Космология, физика космических лучей и темная материя

• Cosmology, astro-particle physics and dark matter 1
• Cosmology, astro-particle physics and dark matter 2
• Cosmology, astro-particle physics and dark matter 3

Dmitry Gorbunov (Russian Academy of Sciences)

Cosmology

Juan Garcia-Bellido (IFT Madrid)

Cosmology 

 

Jonathan Feng (UC Irvine)

Cosmology
Essential Cosmology: Contents and History of the Universe
WIMP Dark Matter: Candidates and Methods of Detection
Inflation, Gravitinos, and Hidden Sectors

 

Valery Rubakov (INR Moscow)

Cosmology
Lecture 1
Expanding Universe
Dark matter: evidence
WIMPs
Lecture 2
Axions
    Theory
    Cosmology
    Search
Warm dark matter
    Sterile neutrino
    Gravitino
Dark matter summary
Baryon asymmetry of the Universe
    Generalities.
    Electroweak baryon numberr non-conservation
Lecture 3
Electroweak baryogenesis. What can make it work?
Before the hot epoch
    Cosmological perturbations
        Regimes of evolution
        Acoustic oscillations: evidence for pre-hot epoch
    Inflation and alternatives
    BICEP-2 saga
Conclusions
Appendices
    Calculation of WIMP mass density
    Estimating axion mass density
    Wave equation in expanding Universe
    Dark energy
    CMB anisotropies, BAO and recent Universe
    Anthropic principle/Environmentalism

Kerstin Elena Kunze (University of Salamanca (ES))

Cosmology
The homogeneous universe. The expansion stages of the universe.
The inhomogeneous universe. The cosmic microwave background. Large scale structure.
Dark matter. Dark energy

Andrea De Simone (SISSA)

 Cosmology (Космология)
Lecture 1:
    • The Universe around us. Dynamics. Energy Budget.
    • The Standard Model of Cosmology:
    • the 3 pillars (Expansion, Nucleosynthesis, CMB).
Lecture 2:
    • Dark Energy.
    • Dark Matter as a thermal relic. Searches for WIMPs.
Lecture 3:
    • Shortcomings of Big Bang cosmology. Inflation. Baryogenesis

Takeo Moroi (Tokyo University)

Cosmology (Космология)
0. Introduction
1. Big-Bang Cosmology: Basic Issues
2. Big-Bang Nucleosynthesis
3. Inflation
4. Dark Matter

Jonathan Feng (UC Irvine)

Cosmology
Essential Cosmology: Contents and History of the Universe
WIMP Dark Matter: Candidates and Methods of Detection
Inflation, Gravitinos, and Hidden Sectors

Igor Tkachev

Cosmology