Cosmology Study Guide
Study Guide
📖 Core Concepts
Physical Cosmology – Treats the universe as a whole, merging mathematics with observations (e.g., CMB, supernovae).
Big Bang Model – Universe began in a hot, dense state → expansion & cooling; supported by Hubble redshift, CMB, primordial abundances.
Cosmic Inflation – Ultra‑rapid exponential expansion fractions of a second after the Big Bang; explains uniform temperature and flat geometry.
ΛCDM Model – Standard framework: cosmological constant (Λ, dark energy) + cold dark matter (CDM); fits CMB, galaxy clustering, supernovae.
Dark Matter vs. Dark Energy – Dark matter (≈ 26.6 % of total) clusters gravitationally; dark energy (≈ 68.5 %) drives accelerated expansion.
Cosmic Microwave Background (CMB) – Relic radiation (2.73 K) with tiny temperature anisotropies; a snapshot of the universe 380 kyr after the Big Bang.
Age of the Universe – $13.799 \pm 0.021$ Gyr (Planck 2014).
Spatial Geometry – Closed (finite, can recollapse) vs. Open (infinite, expands forever).
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📌 Must Remember
Hubble Law (1929): $v = H0 d$ (galaxy recession speed ∝ distance).
CMB Composition (Planck 2014): 4.9 % baryonic matter, 26.6 % dark matter, 68.5 % dark energy.
Key Observational Milestones
1923‑24: Cepheid variables → Andromeda distance → extra‑galactic nebulae.
1964: CMB discovery → strong Big Bang evidence.
Late 1990s: Type Ia supernovae → accelerating expansion.
Inflation solves: horizon problem, flatness problem, monopole problem.
Einstein’s Λ: Introduced 1917; later re‑interpreted as dark energy causing acceleration if Λ > 0.
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🔄 Key Processes
From Newtonian Mechanics to Relativistic Cosmology
Newton → universal gravitation → Kepler’s laws.
Einstein (1917) → General Relativity (GR) → dynamic spacetime models.
Establishing Cosmic Expansion
Friedmann (1922) derives expanding solutions from GR.
Hubble measures redshifts → linear distance‑redshift relation → expansion confirmed.
Inflationary Epoch
Quantum fluctuations → exponential expansion (scale factor $a(t) \propto e^{Ht}$).
Stretching smooths density variations → uniform CMB temperature.
ΛCDM Parameter Determination
CMB anisotropy spectra (Planck) → fit six base parameters (Ωb, Ωc, ΩΛ, ns, τ, H0).
Complement with supernovae (distance modulus) & BAO (baryon acoustic oscillations) for consistency.
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🔍 Key Comparisons
Closed vs. Open Universe
Closed: Positive curvature, finite volume, possible recollapse.
Open: Zero/negative curvature, infinite volume, expands forever.
Λ (Cosmological Constant) vs. Dark Energy (General)
Λ: Constant energy density, equation of state $w = -1$.
Dark Energy: May vary with time (e.g., quintessence), $w \lesssim -1/3$.
Big Bang vs. Steady‑State (historical)
Big Bang: Finite age, evolving density, CMB relic.
Steady‑State: Continuous matter creation, no CMB (now disfavored).
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⚠️ Common Misunderstandings
“Inflation = Big Bang” – Inflation is a brief pre‑expansion phase; the Big Bang describes the subsequent hot, dense evolution.
“Dark matter is dark energy” – Dark matter clusters gravitationally; dark energy drives acceleration and does not clump.
“ΛCDM predicts a static universe” – ΛCDM includes expansion; Λ merely adds an accelerating term.
Age vs. Hubble Time – Age $≈$ 13.8 Gyr ≠ $1/H0$ (≈ 14.4 Gyr) because of deceleration/acceleration history.
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🧠 Mental Models / Intuition
Balloon Analogy – Surface of an inflating balloon represents the expanding universe; galaxies are dots on the surface, moving apart as the balloon stretches, not moving through space.
Frozen Sound Waves – CMB temperature peaks correspond to sound waves frozen at recombination; their spacing sets the angular scale of anisotropies.
Energy Budget Pie – Visualize the universe as a pie: tiny slice (≈ 5 %) ordinary matter, larger slice (≈ 27 %) invisible matter, biggest slice (≈ 68 %) mysterious energy causing acceleration.
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🚩 Exceptions & Edge Cases
Spatial Curvature Near Zero – Observations are consistent with flat geometry (Ωk ≈ 0) but tiny positive/negative curvature remains within error bars.
Dynamic Dark Energy – Current data fit Λ (constant), but future measurements could reveal a time‑varying $w$.
Modified Gravity Theories – Some propose alternatives to dark energy (e.g., f(R) gravity); not part of ΛCDM but worth recognizing as “edge‑case” explanations.
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📍 When to Use Which
Redshift–Distance (Hubble Law) – Use for nearby galaxies (z ≲ 0.1) where linear approximation holds.
Type Ia Supernovae – Best for measuring accelerated expansion (z ≈ 0.5–1.5) and constraining Λ.
CMB Power Spectrum – Primary tool for global parameters (Ωb, Ωc, ΩΛ, ns).
Gravitational Lensing – Ideal for mapping dark matter distribution in clusters and the cosmic web.
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👀 Patterns to Recognize
Exponential Growth → Flatness – Any process described by $a(t) \propto e^{Ht}$ quickly drives curvature toward zero.
Temperature Anisotropy Peaks → Acoustic Oscillations – Peaks at multipole ℓ ≈ 200 correspond to sound horizon scale.
Supernova Light‑Curve Stretch → Standard Candle – Uniform peak luminosity after correcting for stretch; deviations hint at new physics.
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🗂️ Exam Traps
Confusing Age with Expansion Rate – A common distractor swaps $13.8$ Gyr with $1/H0$; remember the age includes deceleration/acceleration phases.
Mixing Percentages – Some choices reverse dark matter and dark energy fractions; recall: 5 % baryons, 27 % dark matter, 68 % dark energy.
Inflation vs. Big Bang Timing – Options may state “inflation occurred after recombination”; correct answer: inflation preceded recombination by 10⁻³⁶ s.
Closed vs. Open Geometry vs. Fate – Closed ≠ necessarily recollapse if Λ dominates; an accelerated Λ can keep a closed universe expanding forever.
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