Skip to main content
Science & AcademiaAstronomy Science261 lines

cosmology

Deep scientific knowledge of physical cosmology: the origin, structure, evolution, and ultimate fate of the universe. Use when the user asks about the Big Bang, cosmic microwave background, dark matter, dark energy, the expansion of the universe, cosmological parameters, inflation, the LCDM model, or the fate of the cosmos. Triggers: "Big Bang", "CMB", "dark matter", "dark energy", "Hubble constant", "cosmological constant", "inflation theory", "LCDM", "expansion of the universe", "cosmic microwave background", "cosmological parameters", "fate of the universe".

Quick Summary28 lines
The science of the universe's origin, large-scale structure, evolution, and ultimate fate. This skill covers the standard cosmological model (LCDM), its observational foundations, open tensions, and alternative proposals.

## Key Points

- **1965**: Penzias and Wilson detect excess 3.5 K microwave noise with Bell Labs horn antenna; Dicke, Peebles, Roll, Wilkinson interpret it as relic radiation. Nobel Prize 1978.
- **COBE** (1989-1993): FIRAS confirms perfect blackbody at T = 2.7255 +/- 0.0006 K; DMR detects anisotropies at delta-T/T ~ 10^-5 level. Nobel Prize 2006 (Mather, Smoot).
- **WMAP** (2001-2010): Full-sky maps at 5 frequencies (23-94 GHz); determined cosmological parameters to percent-level precision; confirmed flat geometry, age 13.77 Gyr.
- **Planck** (2009-2013): ESA mission; 9 frequency bands (30-857 GHz); angular resolution to 5 arcmin; definitive measurement of power spectrum to l ~ 2500; polarization maps.
- **First acoustic peak** (l ~ 220, angular scale ~ 1 degree): confirms flat spatial geometry (Omega_total ~ 1)
- **Second peak** (l ~ 540): constrains baryon density Omega_b h^2
- **Third peak** (l ~ 800): constrains matter density Omega_m h^2
- **Damping tail** (l > 1000): Silk damping from photon diffusion
- **Sachs-Wolfe plateau** (l < 30): large-scale gravitational redshifts, nearly scale-invariant
- **E-modes**: gradient-type pattern from Thomson scattering at last scattering surface; well measured by Planck
- **B-modes**: curl-type pattern; two sources — gravitational lensing of E-modes (detected by SPTpol, POLARBEAR, ACT, Planck) and primordial gravitational waves from inflation (not yet detected)
- Tensor-to-scalar ratio r < 0.032 (BICEP/Keck 2024 upper limit); future targets: CMB-S4, LiteBIRD aim for r ~ 0.001

## Quick Example

```
v = H_0 * d
```

```
1 + z = a_0 / a_emit = lambda_obs / lambda_emit
```
skilldb get astronomy-science-skills/cosmologyFull skill: 261 lines
Paste into your CLAUDE.md or agent config

Cosmology

The science of the universe's origin, large-scale structure, evolution, and ultimate fate. This skill covers the standard cosmological model (LCDM), its observational foundations, open tensions, and alternative proposals.


Big Bang Timeline

The universe evolved through distinct epochs after the initial singularity (t = 0):

EpochTime After BangTemperatureKey Physics
Planck epoch0 to ~5.4 x 10^-44 s>10^32 KQuantum gravity regime; all four forces unified; current physics breaks down
Grand unification~10^-43 to ~10^-36 s~10^29 KGravity separates; GUT symmetry holds for strong + electroweak
Inflation~10^-36 to ~10^-32 sExponential expansion by factor ~10^26; seeds quantum fluctuations that become large-scale structure
Electroweak epoch~10^-36 to ~10^-12 s~10^28 to ~10^15 KStrong force separates; electroweak symmetry intact
Quark epoch~10^-12 to ~10^-6 s~10^15 to ~10^12 KElectroweak symmetry breaks (Higgs mechanism); quarks and gluons in plasma
Hadron epoch~10^-6 to ~1 s~10^12 to ~10^10 KQuarks confine into protons and neutrons; matter-antimatter annihilation leaves baryon asymmetry (~1 in 10^9)
Lepton epoch~1 to ~10 s~10^10 to ~10^9 KNeutrinos decouple (cosmic neutrino background, ~1.95 K today); electron-positron annihilation
Big Bang nucleosynthesis (BBN)~10 s to ~20 min~10^9 to ~10^8 KLight nuclei form: ~75% H, ~25% He-4 by mass, trace D, He-3, Li-7; predicted abundances match observations — key pillar of Big Bang model
Photon epoch / radiation domination~20 min to ~47,000 yrRadiation energy density dominates; photons, electrons, baryons tightly coupled
Matter-radiation equality~47,000 yr (z ~ 3400)~10^4 KMatter energy density overtakes radiation; structure growth accelerates
Recombination~370,000 yr (z ~ 1100)~3000 KElectrons combine with nuclei to form neutral atoms; photons decouple — this is the CMB surface of last scattering
Dark ages~370,000 yr to ~100-200 MyrNo luminous sources; neutral hydrogen pervades; density perturbations grow
Cosmic dawn / reionization~100 Myr to ~1 Gyr (z ~ 20 to z ~ 6)First stars and galaxies ionize intergalactic hydrogen; Gunn-Peterson trough in quasar spectra marks end of reionization
Structure formation~1 Gyr onwardGalaxies, clusters, cosmic web assemble hierarchically
Dark energy domination~9.8 Gyr (z ~ 0.4) to presentExpansion begins accelerating
Present13.787 +/- 0.020 Gyr2.7255 K (CMB)Observable universe radius ~46.5 Gly (comoving)

Cosmic Microwave Background (CMB)

Discovery and Missions

  • 1965: Penzias and Wilson detect excess 3.5 K microwave noise with Bell Labs horn antenna; Dicke, Peebles, Roll, Wilkinson interpret it as relic radiation. Nobel Prize 1978.
  • COBE (1989-1993): FIRAS confirms perfect blackbody at T = 2.7255 +/- 0.0006 K; DMR detects anisotropies at delta-T/T ~ 10^-5 level. Nobel Prize 2006 (Mather, Smoot).
  • WMAP (2001-2010): Full-sky maps at 5 frequencies (23-94 GHz); determined cosmological parameters to percent-level precision; confirmed flat geometry, age 13.77 Gyr.
  • Planck (2009-2013): ESA mission; 9 frequency bands (30-857 GHz); angular resolution to 5 arcmin; definitive measurement of power spectrum to l ~ 2500; polarization maps.

Power Spectrum

The angular power spectrum C_l as a function of multipole moment l encodes:

  • First acoustic peak (l ~ 220, angular scale ~ 1 degree): confirms flat spatial geometry (Omega_total ~ 1)
  • Second peak (l ~ 540): constrains baryon density Omega_b h^2
  • Third peak (l ~ 800): constrains matter density Omega_m h^2
  • Damping tail (l > 1000): Silk damping from photon diffusion
  • Sachs-Wolfe plateau (l < 30): large-scale gravitational redshifts, nearly scale-invariant

Polarization

  • E-modes: gradient-type pattern from Thomson scattering at last scattering surface; well measured by Planck
  • B-modes: curl-type pattern; two sources — gravitational lensing of E-modes (detected by SPTpol, POLARBEAR, ACT, Planck) and primordial gravitational waves from inflation (not yet detected)
  • Tensor-to-scalar ratio r < 0.032 (BICEP/Keck 2024 upper limit); future targets: CMB-S4, LiteBIRD aim for r ~ 0.001

Expansion of the Universe

Hubble's Law

v = H_0 * d
  • v: recession velocity of a galaxy
  • H_0: Hubble constant (present-day expansion rate)
  • d: proper distance

Hubble Constant Tension

This is one of the most significant open problems in cosmology:

MethodValue (km/s/Mpc)Basis
Planck CMB (2018)67.36 +/- 0.54Early universe, assuming LCDM
SH0ES Cepheid-calibrated SNe Ia (2022)73.04 +/- 1.04Local distance ladder
CCHP TRGB (2024)~69.8 +/- 1.7Tip of red giant branch calibration
TDCOSMO strong lensing time delays~74 +/- 1.7Gravitational lensing
DESI BAO + CMB (2024)~67.97 +/- 0.38Baryon acoustic oscillations

The ~5 sigma discrepancy between early-universe (CMB) and late-universe (distance ladder) values may indicate new physics beyond LCDM or unresolved systematic errors.

Redshift

Cosmological redshift z: wavelength stretching from expansion.

1 + z = a_0 / a_emit = lambda_obs / lambda_emit

For z << 1: v ~ c * z (Hubble flow). For higher z, use full Friedmann cosmology.


Dark Matter

Observational Evidence

  1. Galaxy rotation curves (Rubin & Ford, 1970s): flat rotation curves at large radii imply M(r) proportional to r, far exceeding visible mass
  2. Gravitational lensing: strong lensing arcs in clusters; weak lensing shear maps reveal mass distributions exceeding baryonic content
  3. CMB power spectrum: relative heights of acoustic peaks constrain Omega_DM h^2 ~ 0.120
  4. Bullet Cluster (1E 0657-56): X-ray gas (baryonic) offset from lensing mass (dark matter) after cluster collision — direct evidence dark matter is collisionless and distinct from baryons
  5. Structure formation: simulations require cold dark matter to reproduce observed galaxy clustering; baryons alone cannot form structure fast enough
  6. BBN: baryon density from light element abundances is only ~5% of critical density; total matter is ~31%

Candidates

  • WIMPs (Weakly Interacting Massive Particles): mass ~10 GeV to ~10 TeV; motivated by WIMP miracle (thermal relic abundance naturally gives correct Omega_DM); increasingly constrained by null results
  • Axions: mass ~10^-6 to 10^-3 eV; originally proposed to solve strong CP problem; searched via microwave cavity experiments (ADMX)
  • Sterile neutrinos: mass ~keV range; warm dark matter candidate; X-ray line searches (3.5 keV anomaly debated)
  • Primordial black holes: constrained across most mass ranges but windows remain (~10^-12 to 10^-11 solar masses; asteroid mass)

Detection Experiments

  • Direct detection: LUX-ZEPLIN (LZ), XENONnT — liquid xenon time projection chambers; world-leading spin-independent WIMP-nucleon cross-section limits (~10^-48 cm^2 at 30 GeV); PandaX-4T (China)
  • DAMA/LIBRA: claims annual modulation signal consistent with dark matter wind; not reproduced by any other experiment; controversial
  • Indirect detection: Fermi-LAT gamma-ray searches; IceCube neutrinos from Sun/galactic center; AMS-02 positron excess (astrophysical explanations compete)
  • Collider searches: LHC searches for missing transverse energy events; no confirmed dark matter production

Dark Energy

Discovery

In 1998, two teams independently found that Type Ia supernovae at z ~ 0.5 were ~25% fainter than expected in a decelerating universe, implying accelerating expansion:

  • Supernova Cosmology Project (Perlmutter et al.)
  • High-z Supernova Search Team (Riess, Schmidt et al.)
  • Nobel Prize in Physics 2011

Cosmological Constant (Lambda)

Einstein's cosmological constant: Lambda term in field equations acts as constant vacuum energy density.

rho_Lambda = Lambda * c^2 / (8 * pi * G) ~ 5.96 x 10^-27 kg/m^3
  • Constitutes ~68% of total energy density today
  • Cosmological constant problem: quantum field theory predicts vacuum energy ~10^120 times larger than observed
  • Coincidence problem: why are Omega_m and Omega_Lambda of similar magnitude now?

Equation of State

Dark energy equation of state parameter:

w = P / (rho * c^2)
  • Cosmological constant: w = -1 exactly (constant in time)
  • Quintessence models: w varies with time; -1 < w < -1/3
  • Phantom energy: w < -1 (leads to Big Rip)

DESI Results (2024-2025)

The Dark Energy Spectroscopic Instrument released BAO measurements across redshift bins 0.1 < z < 4.2 using >5.7 million galaxies and quasars:

  • Hints that w may evolve with time (w_0 w_a parameterization: w(a) = w_0 + w_a(1-a))
  • w_0 ~ -0.55, w_a ~ -1.6 (combined with CMB + SNe) — >2 sigma deviation from cosmological constant
  • If confirmed, would rule out simple Lambda; suggests dynamical dark energy or modified gravity
  • More data releases expected to clarify

Cosmological Parameters (Planck 2018 + BAO)

ParameterSymbolValue
Hubble constantH_067.36 +/- 0.54 km/s/Mpc
Total matter densityOmega_m0.3153 +/- 0.0073
Baryon densityOmega_b0.0493 +/- 0.0006
Dark energy densityOmega_Lambda0.6847 +/- 0.0073
Dark matter densityOmega_c h^20.1200 +/- 0.0012
Amplitude of fluctuationssigma_80.8111 +/- 0.0060
Scalar spectral indexn_s0.9649 +/- 0.0042
Optical depth to reionizationtau0.0544 +/- 0.0073
Age of the universet_013.787 +/- 0.020 Gyr

Cosmic Inflation

Problems Solved

  • Horizon problem: regions on opposite sides of the CMB sky (separated by >2 degrees) were never in causal contact in standard Big Bang — inflation stretches a causally connected patch to encompass the entire observable universe
  • Flatness problem: without inflation, Omega must be fine-tuned to 1 part in 10^60 at the Planck time; inflation drives Omega toward 1 dynamically
  • Monopole problem: GUT phase transitions produce magnetic monopoles; inflation dilutes them to undetectable density

Theory

  • Alan Guth (1981): proposed old inflation (first-order phase transition); bubble nucleation problem
  • New inflation (Linde; Albrecht & Steinhardt, 1982): slow-roll down a potential — solves graceful exit
  • Chaotic inflation (Linde, 1983): inflation from generic initial conditions with large-field potentials
  • Inflaton field phi rolls slowly: slow-roll parameters epsilon and eta << 1
  • Quantum fluctuations in phi become density perturbations (scalar) with nearly scale-invariant power spectrum (n_s ~ 0.96)
  • Tensor perturbations (gravitational waves): amplitude parameterized by tensor-to-scalar ratio r

Eternal Inflation and Multiverse

  • In many models, inflation never ends globally — quantum fluctuations keep some regions inflating forever
  • Produces a "multiverse" of causally disconnected pocket universes with potentially different physical constants
  • Controversial: not directly testable; raises measure problem

LCDM: Successes and Tensions

Successes

  • Predicts CMB power spectrum with extraordinary precision (6 parameters fit thousands of data points)
  • Correctly predicts BBN light element abundances
  • Reproduces observed large-scale structure (BAO, galaxy clustering, weak lensing)
  • Consistent with observed accelerating expansion

Tensions

  • H_0 tension: 4-6 sigma discrepancy between CMB-inferred and local measurements; most significant challenge to LCDM
  • S_8 tension: weak lensing surveys (KiDS, DES, HSC) measure S_8 = sigma_8 * sqrt(Omega_m/0.3) ~ 0.76, while Planck predicts ~0.83; 2-3 sigma discrepancy; possible evidence for less clumping than expected
  • DESI dark energy hints: possible time-varying w challenges cosmological constant assumption
  • Lithium problem: BBN predicts 3x more Li-7 than observed in old stars
  • Sigma-8 / lensing anomaly: Planck internal lensing amplitude A_L prefers >1 at ~2-3 sigma

Fate of the Universe

ScenarioConditionOutcome
Big Freeze / Heat Deathw = -1 (Lambda); current best fitExpansion accelerates forever; galaxies beyond Local Group become unreachable; stars burn out (~10^14 yr); black holes evaporate via Hawking radiation (~10^100 yr); maximum entropy state
Big Ripw < -1 (phantom energy)Dark energy density increases; eventually tears apart galaxy clusters, galaxies, solar systems, planets, atoms; finite time to singularity
Big CrunchOmega > 1, no dark energyExpansion reverses; universe collapses to singularity; ruled out by observations of acceleration
Big BounceCyclic modelsUniverse oscillates between expansion and contraction; no true beginning or end

Current data favors the Big Freeze / heat death scenario.


Alternative Cosmologies

  • MOND (Modified Newtonian Dynamics; Milgrom, 1983): modifies gravity at low accelerations (a < a_0 ~ 1.2 x 10^-10 m/s^2) instead of invoking dark matter; explains galaxy rotation curves but struggles with cluster-scale observations and CMB without supplementary dark matter; relativistic extension TeVeS largely ruled out by gravitational wave speed measurement (GW170817)
  • Cyclic models (Steinhardt & Turok): brane collisions in extra dimensions produce repeated Big Bang events; avoids initial singularity; no inflation needed; generates nearly scale-invariant perturbations via ekpyrotic contraction
  • f(R) gravity: generalization of Einstein's equations; can produce late-time acceleration without dark energy; constrained by solar system tests and gravitational wave observations
  • Emergent gravity (Verlinde): gravity as entropic force; dark matter as emergent phenomenon from entanglement entropy; not yet a complete theory

Anti-Patterns

  • Stating the Big Bang was an explosion in space: It was an expansion of space itself; there is no center or edge; every point was the Big Bang
  • Claiming dark matter has been directly detected: No confirmed direct detection as of 2025; all evidence is gravitational/indirect; DAMA claims are not independently reproduced
  • Treating the Hubble constant as precisely known: The H_0 tension is real and unresolved; always note the measurement method and value range (~67-73 km/s/Mpc)
  • Conflating dark matter and dark energy: Fundamentally different phenomena — dark matter gravitates and clumps; dark energy is smooth and causes accelerating expansion
  • Presenting inflation as confirmed fact: Inflation is the leading paradigm but remains unproven; primordial B-modes (smoking gun) have not been detected; alternatives exist
  • Saying the universe is 13.8 billion light-years in radius: The observable universe has a comoving radius of ~46.5 billion light-years due to expansion; the age in years does not equal the radius in light-years
  • Treating LCDM tensions as proof of new physics: They may reflect systematic errors in measurements; state them as tensions, not confirmed anomalies
  • Confusing recombination with the end of the universe's opacity: Recombination made the universe transparent to photons but neutral hydrogen was opaque to UV until reionization
  • Presenting the multiverse as scientific consensus: It is a theoretical prediction of some inflation models, not an observationally confirmed framework
  • Ignoring error bars on cosmological parameters: Always cite uncertainties; cosmology is a precision science and the uncertainties matter

Install this skill directly: skilldb add astronomy-science-skills

Get CLI access →

Related Skills

exoplanet-science

Comprehensive knowledge of exoplanet detection, characterization, and habitability science. Use when the user asks about finding planets around other stars, habitable zones, biosignatures, transit methods, radial velocity, or specific exoplanet systems. Triggers: "how do we find exoplanets", "what is the transit method", "explain radial velocity", "what is the habitable zone", "tell me about TRAPPIST-1", "what is a hot Jupiter", "how does JWST study exoplanet atmospheres", "what is eta-Earth", "explain biosignatures", "Kepler mission results", "what is a super-Earth", "exoplanet atmospheric characterization".

Astronomy Science358L

galactic-astronomy

Deep scientific knowledge of galaxies: classification, structure, formation, evolution, dynamics, and active nuclei. Use when the user asks about the Milky Way, galaxy types, galaxy formation and evolution, active galactic nuclei, quasars, supermassive black holes, galaxy mergers, spiral structure, or dwarf galaxies. Triggers: "Milky Way", "galaxy classification", "Hubble sequence", "elliptical galaxy", "spiral galaxy", "galaxy formation", "galaxy evolution", "AGN", "quasar", "supermassive black hole", "galaxy merger", "Sgr A*", "galactic dynamics".

Astronomy Science269L

Gravitational Wave Astronomy

Deep knowledge of gravitational wave theory, detection methods, landmark observations, waveform physics, source types, pulsar timing arrays, future detectors, and multi-messenger astronomy for authoritative scientific discussion.

Astronomy Science160L

large-scale-structure

Deep scientific knowledge of the large-scale structure of the universe: the cosmic web, galaxy clusters and groups, superclusters, filaments, voids, baryon acoustic oscillations, structure formation theory, and observational surveys. Use when the user asks about the cosmic web, galaxy clusters, superclusters, voids, BAO, large-scale structure surveys, N-body simulations, or the distribution of matter in the universe. Triggers: "cosmic web", "galaxy cluster", "supercluster", "Laniakea", "Great Attractor", "baryon acoustic oscillations", "BAO", "galaxy survey", "SDSS", "DESI", "Euclid", "large-scale structure", "cosmic void", "filament", "N-body simulation".

Astronomy Science297L

observational-astronomy

Comprehensive knowledge of observational astronomy techniques, instruments, and methods. Use when the user asks about telescopes, spectroscopy, photometry, astrometry, imaging techniques, astronomical surveys, coordinate systems, or atmospheric effects on observations. Triggers: "how do telescopes work", "explain spectroscopy", "what is adaptive optics", "how do astronomers measure distance", "explain redshift", "what is the magnitude system", "how does Gaia work", "explain CCD imaging", "what is seeing in astronomy", "compare Hubble and JWST", "explain the electromagnetic spectrum in astronomy".

Astronomy Science323L

planetary-science

Comprehensive knowledge of solar system science including planets, moons, dwarf planets, ring systems, planetary formation, geological processes, and space missions. Use when the user asks about any solar system body, planetary atmospheres, missions to planets or moons, or how the solar system formed. Triggers: "tell me about Mars", "what is Europa's ocean", "how did the solar system form", "explain Titan's atmosphere", "what did Cassini discover", "compare gas giants and ice giants", "what are dwarf planets", "explain planetary differentiation", "Mars rover missions", "what is the Great Red Spot", "explain tidal heating", "ring systems of Saturn".

Astronomy Science325L