課程資訊
課程名稱
粒子天文物理學
Particle Astrophysics 
開課學期
112-1 
授課對象
理學院  天文物理研究所  
授課教師
裴思達 
課號
AsPhys8011 
課程識別碼
244ED1040 
班次
 
學分
3.0 
全/半年
半年 
必/選修
選修 
上課時間
星期四7,8,9(14:20~17:20) 
上課地點
天數812 
備註
本課程以英語授課。
總人數上限:30人
外系人數限制:5人 
 
課程簡介影片
 
核心能力關聯
本課程尚未建立核心能力關連
課程大綱
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課程概述

Particle Astrophysics is a relatively new topic combining Elementary Particle Physics, Cosmology and Astrophysics. 

課程目標
To cover the latest progress in the areas of Universe expansion, CMB, Inflation, Dark Energy and Dark Matter and more. 
課程要求
- Basic knowledge of relativity.
- Some knowledge of Particle Physics and Classical Field Theory would be preferred but not required. 
預期每週課後學習時數
 
Office Hours
備註: Flexible. 
指定閱讀
- Cosmology by Daniel Baumann
- Chapters 1-4 from Cosmology, by Steven Weinberg.
- Parts of Chapters 6 and 7 from Cosmology, by Steven Weinberg: needed to discuss the interpretation of CMB measurements.
- Some of the Appendices would also be useful: Appendix B is required. 
參考書目
- Cosmology by Daniel Baumann
- Cosmology Weinberg 
評量方式
(僅供參考)
   
針對學生困難提供學生調整方式
 
上課形式
以錄影輔助, 提供學生彈性出席課程方式
作業繳交方式
延長作業繳交期限
考試形式
書面(口頭)報告取代考試
其他
由師生雙方議定
課程進度
週次
日期
單元主題
Week 3
  The Metric of the Universe
- A homogeneous and isotropic Universe: The Robertson-Walker metric.
- Co-moving coordinates.
- Covariant Derivative and Geodesic Equation: massive particles and light
- Spatial Geodesics.
- Cold Matter, Hot Matter, Vacuum energy 
Week 4
  Fill Universe with fields
- Non Relativistic Matter, Dark Matter, Dark Energy, Radiation 
Week 5
  Expansion of the Universe 1: small z
The cosmological redshift: The Hubble Constant, Discovery of expansion
Some observations: Tully-Fisher relation, Type Ia supernovae and more. 
Week 6
  Expansion of the Universe 2: z>0.1
- Luminosity Distance
- Dynamics of Expansion
- Einstein field equations.
- Friedmann Equation. 
Week 7
  Expansion of the Universe 3
- Critical density, Flatness problem.
- Accelerated expansion.
- Age of the Universe 
Week 1-2
  Introduction to Cosmology
- Conventions: Einstein, Minkowski, Momentum 4-vector, Natural units.
- Equivalence Principle: the need for Manifolds.
- Scalars, Vectors, Tensors. The Metric Tensor.
- Equations of Einstein. The Cosmological Constant. Dark Energy.
- Covariant, Contravariant. Christoffel symbols. Why do we need tensors?
- The meaning of the stress energy tensor. 
Week 8-9
  The Early Universe (1 and 2) 
Week 10-11
  Inflation as the origin of cosmological fluctuations 
Week 12-13
  Other topics:
- Anisotropies in the Microwave sky
- Gravitational Lensing