Dark Matter Notes

Astronomy and Humility

  • Astronomy reveals our diminished importance in the universe.
  • Earth is a small planet orbiting a typical star in the suburbs of a vast galaxy.
  • Observable matter is only a fraction of what exists.

Vera Rubin and Galaxy Rotation

  • Vera Rubin studied spiral galaxy rotation in the 1960s-70s.
  • She aimed to understand galaxy rotation to learn about their structure and mass.
  • Johannes Kepler discovered planets farther from the Sun orbit slower.
  • Isaac Newton quantified this with gravity calculations, allowing mass determination.
  • The same principles should apply to galaxies.
  • Measuring gas cloud orbits at galaxy edges allows calculation of total galaxy mass using Doppler shift.

Unexpected Rotation Curves

  • Rubin expected gas clouds farther from the galactic center to move slower.
  • She observed the opposite: gas clouds moved faster at greater distances.
  • At best, velocities flattened out instead of declining as predicted.
  • This indicated constant gravity throughout the galaxy disk.
  • Visible matter decreases with distance from the center, so there was not enough visible mass to cause constant gravity.
  • The explanation is dark matter contributes to gravity.
  • Galaxies are embedded in dark matter halos.
  • Rubin determined there is five to six times more dark matter than visible matter.

Fritz Zwicky and Galaxy Clusters

  • In the 1930s, Fritz Zwicky found galaxies in clusters moving too fast to remain bound by visible matter.
  • He suggested more gravity than that provided by visible matter was present.
  • Zwicky's observations had large uncertainties and overestimated dark matter.
  • Rubin's more accurate work is now credited with the discovery.
  • The term "dark matter," coined by Zwicky, is still used.

Confirmation and Skepticism

  • Observations of elliptical galaxies and galaxy clusters confirmed Rubin’s findings.
  • Initially, the concept of dark matter faced skepticism.
  • Everything emits light but dark matter does not.

What is Dark Matter?

  • Astronomers systematically considered all potential candidates for dark matter.
  • Candidates included cold gas, dust, dead stars, rogue planets, and exotic subatomic particles.
  • Various detection methods were employed, but all yielded negative results.
  • Normal matter was eliminated as a possibility.

Axions

  • Axions are hypothetical subatomic particles that could make up dark matter.
  • Axions possess mass and exert gravitational force.
  • Axions do not emit much light.
  • Axions interact weakly with normal matter.
  • Clouds of axions could envelop galaxies and clusters without being detected.

Gravitational Lensing

  • Einstein proposed that space is a "fabric."
  • Gravity is the warping of space caused by mass and energy.
  • Light bends when passing through warped space.
  • The amount of bending depends on the mass causing the warping.
  • Lenses also bend light.
  • Gravitational lensing occurs when a massive object bends light from a more distant object.
  • A galaxy cluster can act as a lens, distorting the images of galaxies behind it.
  • Einstein's equations allow mass measurement of galaxy clusters via gravitational lensing.

The Bullet Cluster

  • The Bullet Cluster is a collision of two galaxy clusters located 3,500,000,0003,500,000,000 light years away.
  • Galaxies pass through each other during cluster collisions.
  • Gas clouds in clusters collide and heat up, emitting X-rays.
  • Chandra X-ray Observatory maps hot gas distribution.
  • Optical images reveal background galaxies distorted by Bullet Cluster gravity.

Dark Matter Distribution

  • Dark matter clouds pass through each other like galaxies during a cluster collision.
  • Gravitational lensing maps the mass distribution, revealing dark matter surrounding the subclusters.
  • Dark matter is separate from the hot gas.

Implications and the Nature of Dark Matter

  • Observations of the Bullet Cluster support the existence of dark matter.
  • Simpler explanations suggest ordinary matter cannot fully explain the structure and movements we see in the universe.
  • The exact composition of dark matter remains unknown.
  • Axions are one possibility, but other particles are also considered.

The Profound Effect of Dark Matter

  • Dark matter has significantly influenced the universe's evolution.
  • Smaller objects formed first, then merged into larger structures.
  • The formation of large structures would have been difficult without dark matter due to high energy output from early stars and galaxies.
  • Dark matter facilitates the formation of the structures we observe.

Our Place in the Universe

  • Ordinary matter in the universe is a small minority.
  • Dark matter surrounds and penetrates everything, binding galaxies together.
  • Approximately 85% of matter in the universe is dark matter.