The Dark Matter Landscape
Rocky Kolb
Radiation: Chemical Elements: 0.005% (other than H & He) 0.025% Neutrinos: ne 0.17% nµ nt Stars: 0.8%
H & He: gas 4%
? Dark Matter: 25%
? Dark Energy: 70% Precision (but not accurate) cosmology
Epicycle Mars
Deferent Eccentric A precision (but not accurate) cosmological ´ model that agreed with observations for Earth Equant 1300 years!
We have to discover how dark matter, dark energy, inflation, the baryon asymmetry, t =0, is grounded in physical law. 95% of mass-energy in the universe is dark! 25% Dark Matter 70% Dark Energy
Dark matter usually assumed to be • Non-baryonic (not quark nuggets, 30 M⊙ Black Holes, planets, little stars, etc.) • Cold (slowly moving) • Dissipationless Is • Not self-interacting this • Associated with all galaxies and other structures true? • A particle • Stable • No strong or electromagnetic interactions
Two philosophies: Simplicio Salviati
I don’t care about the nature of dark I care about the nature of dark matter matter, as long as it is dark, cold, & because it must exist for a reason other dissipationless (CDM) I can calculate than to be a part of Simplicio’s code. (simulate) its role in the evolution of Feynman: “Nature weaves its tapestry structure and understand necessary from the longest threads.” What is the astrophysics. dark matter thread? Physics crucial for cosmology
"Until cosmology and particle physics can be brought together in the same context there is not much hope for real progress in cosmology."
Bohr’s 1939 reply to question after a Berkeley colloquium (Philip Morrison, private communication) Astronomy crucial for physics
"How helpful to us is astronomy's pedantic accuracy, which I used to secretly ridicule!"
Einstein’s statement to Arnold Sommerfeld on December 9, 1915 (regarding measurements of the advance of the perihelion of Mercury) Dark Matter particle mass range
Mass Range for Particle Dark Matter m 10-22 eV: de Broglie wavelength smaller than dark-matter dominated objects m 1019 GeV: mass less than Planck mass m few eV: if fermion (exclusion principle)
If thermal freeze-out m me : annihilation to SM particles m 100 TeV: annihilation cross section too small for larger masses
Is Dark Matter a Particle Or a Wave? m 1 eV: occupation number in de Broglie-wavelength volume 1 ® WAVE m 1 eV: occupation number in de Broglie-wavelength volume 1 ® PARTICLE Dark Matter particle mass range
19 Plancktons: m ~ mPlanck = 10 GeV
10 13 WIMPzillas: m ~ minflaton = 10 – 10 GeV
Supermassive: m > 100 TeV
WIMP range: mproton < m < 1 TeV
Light dark matter: melectron < m < mproton
Ultralight dark matter: m < 1 eV
Fuzzy dark matter: m ~ 10-22 eV Particle dark-matter debate: need > two nights for debate
• (sub-) eV mass neutrinos (WIMPs exist!) (hot) • sterile neutrinos, gravitinos (warm) thermal relics, or decay of or oscillation from • lightest supersymmetric particle (cold) thermal relics • lightest Kaluza-Klein particle (cold) • Bose-Einstein condensates from phase • axions, axion miniclusters transitions • solitons (Q-balls, B-balls, …) nonthermal relics • supermassive WIMPZILLAs from inflation
Mass Interaction Strength 10-22 eV (10-56 g) Bose-Einstein only gravitational: WIMPzillas -8 +25 10 Mʘ (10 g) axion miniclusters strongly interacting: B balls Most popular paradigm: cold thermal relic* • DM abundance set by creation/annihilation with standard-model particles • Equilibrium abundance of DM determined by M / T (no asymmetry) • DM species final abundance determined by “freeze-out” of equilibrium, or “freeze-in” to final abundance Freeze-out
nncg Freeze-in Equilibrium
• Freeze-out/in: interplay between mTc particle physics (DM—SM interactions) and expansion rate (gravity)
* An object of particular veneration. Dark Matter talks to Standard Model through a PORTAL
DM (c) SM
gc g PORTAL
DM (c) SM
Usually assume PORTAL is some mediator more massive than dark matter
Evolution of DM abundance set by Boltzmann equation:
22 nHn+=3v--s A ( nnEQ )
NR annihilation cross m2 � v = s v = 22 c Tm � section × Møller flux A ggc 4 c á …thermal average…ñ M Final freeze-out abundance: