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dark matter
an undetected form of mass that does not interact with light, but whose existence we infer from its gravitational influence on observed motions of stars and gas clouds
dark energy
an unknown form of energy that seems to cause a repulsive force accelerating the Universe’s expansion
current best model of BB and cosmology is called
lambda CDM
Lambda CDM meaning
Cold - moving at nonrelativistic speeds
Dark - does not emit electromagnetic radiation (light)
Matter - we see it through its gravitational pull, like normal masses
Lambda - cosmological constant associated with dark energy
overall geometry of universe is
flat (critical density possessed by total mass + energy)
composition of universe percentages
5% baryons, 27% dark matter, 68% dark energy
baryons
“normal” matter e.g. protons and neutrons
vera rubin’s findings
rotation curves of spiral galaxies are flat; outermost components move as quickly as those close to the center, indicating large amounts of dark matter
how to measure galaxy rotation
doppler shift of atomic hydrogen’s 21cm line
elliptical galaxy
ellipsoidal or spherical shape with no well organized disk, composed of older stars with little new star formation; believed to form from merger of smaller galaxies
orbital speeds in elliptical galaxies
while randomized, they still depend on the mass within their orbit, and these galaxies also have dark matter
we can tell how fast stars are orbiting through
broadening of spectral lines

dark matter halo
dark matter appears to be contained in a sphere around a galaxy
dark matter is collisionless, meaning it
doesn’t lose energy through friction or gas shocks
galaxy clusters
massive and bound by gravity, contain galaxies + gas + dark matter
% composition of galaxy clusters
85% dark matter, 13% hot gas, 2% stars
fritz zwicky found that
orbits of galaxies around a gravitational center disagreed with their apparent baryonic mass content
galaxy cluster motion
can be measured from doppler shifts, and the mass we find from these motions is about 40 times larger than the mass in stars
hot gas in galaxy clusters
10x star mass in hot, x-ray emitting gas in an equilibrium where gas pressure balances gravity
temperature is the KE of particles, which is determined by
their gravitational potential (and therefore the mass of the cluster)
gravitational lensing
cluster’s gravity bends light from a single galaxy so that it reaches Earth from multiple directions; direct measure of mass

einstein ring
gravitational lensing with the exact alignment of the source, lens, and observer
bullet cluster
two colliding galaxy clusters, separating the x-ray emitting hot gas from the bulk of stars and galaxies
options for existence of dark matter
either it really exists and we are observing its effects, or something is wrong with our understanding of gravity causing a mistaken inference
properties of dark matter that theory must fit
interacts strongly via gravity and maybe weak force, does not emit or interact with detectable light, cold (non-relativistic), stable (on the timescales of the universe)
ordinary dark matter
made of protons, neutrons, and electrons, but too dark to detect with current instruments
extraordinary dark matter
new types of particles (weakly interacting massive particles, axions or axion-like, sterile neutrino) and primordial black holes
ordinary matter possibility
unlikely, but would be if ejected into the outer reaches of a galaxy and are dim e.g. planets, dwarfs, black holes - a massive compact halo object
most dark matter is unlikely to be ordinary matter because
large, dark, compact objects seem to be rare and % of the observed elements do not match this theory
big bang nucleosynthesis predicts
observed abundance of elements
based on density of matter we can predict
how much deuterium should be left over from when protons and neutrons formed it in the early universe
if we were 100% density of ordinary matter, abundance of deuterium would be
very low, mostly fusing into helium
deuterium we have measured indicates
we have around 5% density of ordinary matter, so dark matter is unlikely to be made of baryons
wimps could come from
big bang; if produced back then at theorized mass range, they would naturally exist in the abundance to explain dark matter, but we haven’t detected them yet
axions
hypothetical elementary particles, become more popular due to non-detection of WIMPs, theory that explains strong force violation
weakly interacting massive particle (wimp)
e.g. a neutrino; dark by nature, no electrical charge or radiation, only interact via gravity and weak force - neutrinos move too fast but similar, heavier particles could exist
sterile neutrino
hypothetical particle that interacts only via gravity, theorized to explain neutrino masses in the standard model
primordial black holes
hypothetical black holes that formed soon after BB; collisionless, stable (as long as they are large enough to avoid evaporation on universe’s timescale), and nonrelativistic
how to detect dark matter
indirect detection, direct detection, observe effects through large scale structure surveys
indirect detection
measuring the expected annihilation or decay products expected from dark matter candidates
direct detection
trying to detect the constituent components of dark matter themselves
dark matter detectors are located
underground to minimize background signals
axion dark matter experiment
axions should weakly convert to photons in presence of a large magnetic field, producing a very small signal from the interaction between possible axions in the milky way dark matter halo and the magnetic field in the cavity
protogalactic clouds in early times contracted because of
dark matter’s gravity
universe grows lumpier with time because
gravity of dark matter pulls mass into denser regions

large scale structure of universe is made up of
superclusters and voids

dark matter is cold because
hot dark matter would smear out large scale structure