Dark Matter & Dark Energy

When astronomers mapped the rotation of spiral galaxies in the 1970s, they found something deeply unsettling: stars far from the galactic centre were orbiting far too fast. By Newton's law of gravity, orbital speed should fall off with distance — just as the outer planets of our Solar System orbit more slowly than the inner ones. Instead, rotation curves stayed nearly flat. The only explanation consistent with gravity was that galaxies are embedded in vast, invisible halos of mass that don't emit, absorb, or reflect any light. This unseen substance is called dark matter, and it accounts for roughly 27% of the total energy content of the universe. The story deepens when we look at the large-scale universe. In 1998, two independent teams measuring the brightness of distant Type Ia supernovae — which serve as 'standard candles' because their peak luminosities are well-calibrated — discovered that distant supernovae were dimmer than expected. The universe is not just expanding; its expansion is accelerating. Something is pushing space apart against the pull of gravity. Physicists call this agent dark energy, and it comprises approximately 68% of the total energy content of the universe. Ordinary matter — every atom, every star, every planet — makes up only about 5%. Together, dark matter and dark energy constitute the 'dark sector' of cosmology. Despite overwhelming indirect evidence, neither has been directly detected in a laboratory. They represent the two largest components of the universe and yet remain among the deepest unsolved problems in physics. Understanding them requires connecting quantum field theory, general relativity, and observational astronomy in ways that push the boundaries of current knowledge.

Key takeaways
  • Galaxy Rotation Curves
  • Gravitational Lensing
  • Cosmic Microwave Background (CMB) Acoustic Peaks
  • Type Ia Supernovae and Dark Energy
  • The ΛCDM Model

Galaxy Rotation Curves

For a star of mass m orbiting at radius r from a galactic centre containing enclosed mass M(r), gravitational centripetal balance gives v = √(GM(r)/r). If all mass were concentrated in the luminous disc, M(r) would be nearly constant beyond the visible edge, predicting v ∝ 1/√r (a Keplerian decline). Observations by Vera Rubin and Kent Ford showed v ≈ constant out to very large radii, implying M(r) ∝ r — mass keeps growing even where there is no visible matter. The simplest fit requires a spherical dark matter halo extending far beyond the stellar disc.

Gravitational Lensing

General relativity predicts that mass curves spacetime, bending light paths. The Bullet Cluster (1E 0657-558) is two galaxy clusters that passed through each other. The hot gas (detected in X-rays) slowed due to electromagnetic drag and piled up in the centre. But gravitational lensing maps show most mass concentrated around the two clusters of galaxies, not the gas. Since the galaxies themselves are mostly dark matter halos, the lensing mass 'passed through' the collision without interacting — exactly what collisionless, weakly-interacting dark matter predicts. This is one of the most direct lines of evidence.

Cosmic Microwave Background (CMB) Acoustic Peaks

The early universe was a hot plasma in which photons and baryons formed sound waves. When the universe cooled enough for atoms to form (recombination, ~380,000 years after the Big Bang), these waves froze. The CMB temperature map shows a characteristic angular power spectrum with peaks at specific multipoles. The relative heights of these peaks are exquisitely sensitive to the ratio of dark matter density to baryon density. Planck satellite data yield Ω_dm h² ≈ 0.120, giving dark matter density about 5× the baryon density. No modification of gravity has successfully reproduced all three observational pillars simultaneously without dark matter.

Type Ia Supernovae and Dark Energy

A Type Ia supernova results from a white dwarf accreting mass until it reaches the Chandrasekhar limit (~1.4 M☉) and undergoes thermonuclear runaway. The peak absolute magnitude is approximately M_B ≈ −19.3, making them excellent standard candles. The distance modulus μ = m − M gives the luminosity distance d_L. By plotting d_L against redshift z and comparing to theoretical Friedmann cosmology predictions, astronomers found supernovae at z ≈ 0.5 were ~0.25 magnitudes fainter than expected for a decelerating or coasting universe — they are farther away than expected, meaning the expansion accelerated. The simplest fit introduces a cosmological constant Λ, equivalent to a constant energy density of empty space, called dark energy.

The ΛCDM Model

ΛCDM (Lambda Cold Dark Matter) is the standard cosmological model. Λ is the cosmological constant representing dark energy with equation of state w = p/(ρc²) = −1 (negative pressure). CDM denotes cold dark matter — particles that were non-relativistic when they decoupled from other matter, enabling them to clump gravitationally and seed the large-scale structure we observe (galaxy clusters and cosmic web filaments). Candidates for CDM particles include WIMPs (Weakly Interacting Massive Particles) and axions, but none has been confirmed experimentally. The equation of state of dark energy is constrained by current data to w = −1.03 ± 0.03, tantalizingly close to Λ but not yet ruling out dynamical alternatives like quintessence fields.

The Key Equation

vrot(r)=G Menc(r)rv_{rot}(r) = \sqrt{\frac{G\,M_{enc}(r)}{r}}
  • v_{rot} — Circular orbital speed (m s⁻¹): Tangential speed of a star or gas cloud on a circular orbit.
  • G — Gravitational constant (m³ kg⁻¹ s⁻²): Universal constant, G = 6.674 × 10⁻¹¹ m³ kg⁻¹ s⁻².
  • M_{enc}(r) — Enclosed mass (kg): Total mass contained within radius r, including dark matter halo.
  • r — Orbital radius (m): Distance from the galactic centre to the orbiting object.

Worked Example

Problem. A galaxy's rotation curve is observed to be flat at v_rot = 220 km s⁻¹ out to a radius of r = 50 kpc (1 kpc = 3.086 × 10¹⁹ m). Estimate the enclosed dark matter mass within this radius, and compare it to the Milky Way's total stellar mass of approximately 5 × 10¹⁰ solar masses (M☉ = 1.989 × 10³⁰ kg).

Menc=v2rG≈5.6×1011 M⊙M_{enc} = \frac{v^2 r}{G} \approx 5.6 \times 10^{11}\,M_{\odot}

Answer. Approximately 5.6 × 10¹¹ solar masses — about 11 times the visible stellar mass.

Figure
Diagram
Galaxy Rotation Curve: Observed vs ExpectedRadius from galactic centre (kpc)Orbital speed (km/s)0102030400100200300400Observed (flat)Expected (Keplerian)Luminous discDark matter halo
Origins · 1 minVera Rubin and how this was discovered
VR
Vera Rubin
1928–2016 · American

Vera Rubin, working with astronomer Kent Ford at the Carnegie Institution, produced the first systematic, high-precision measurements of galaxy rotation curves in the 1970s. By carefully measuring Doppler shifts of emission lines across dozens of spiral galaxies, she demonstrated conclusively that orbital velocities did not decline at large radii as Newtonian gravity applied to visible mass predicted. Her work provided the most compelling early evidence for dark matter and transformed it from a theoretical curiosity into a central paradigm of astrophysics. Rubin was famously denied access to Palomar Observatory when she began her career in the 1950s because it did not admit women. She later quipped that she had to change the sign on the bathroom door herself.

  • Hubble Expansion and Redshift — The accelerating expansion evidence for dark energy comes directly from redshift–distance measurements of supernovae within the Hubble flow.
  • White Dwarfs and the Chandrasekhar Limit — Type Ia supernovae used as standard candles to detect dark energy arise when white dwarfs reach the Chandrasekhar mass limit.
  • Cosmic Microwave Background — CMB acoustic peak analysis provides the most precise measurements of dark matter and dark energy densities in the universe.
  • General Relativity and Spacetime — Both gravitational lensing evidence for dark matter and the cosmological constant interpretation of dark energy are rooted in Einstein's field equations.