A theory of dark matter

Journal Article · Thu Jan 01 00:00:00 EST 2009 · Physical Review. D, Particles Fields

DOI:https://doi.org/10.1103/PHYSREVD.79.015014· OSTI ID:21254742

Arkani-Hamed, Nima ^[1]; Finkbeiner, Douglas P ^[2]; Slatyer, Tracy R ^[3]; Weiner, Neal ^[4]

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1. School of Natural Sciences, Institute for Advanced Study, Princeton, New Jersey 08540 (United States)
2. Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts 02138 (United States)
3. Physics Department, Harvard University, Cambridge, Massachusetts 02138 (United States)
4. Center for Cosmology and Particle Physics, Department of Physics, New York University, New York, New York 10003 (United States)

We propose a comprehensive theory of dark matter that explains the recent proliferation of unexpected observations in high-energy astrophysics. Cosmic ray spectra from ATIC and PAMELA require a WIMP (weakly interacting massive particle). with mass M{sub {chi}}{approx}500-800 GeV that annihilates into leptons at a level well above that expected from a thermal relic. Signals from WMAP and EGRET reinforce this interpretation. Limits on p and {pi}{sup 0}-{gamma}'s constrain the hadronic channels allowed for dark matter. Taken together, we argue these facts imply the presence of a new force in the dark sector, with a Compton wavelength m{sub {phi}}{sup -1} > or approx. 1 GeV{sup -1}. The long range allows a Sommerfeld enhancement to boost the annihilation cross section as required, without altering the weak-scale annihilation cross section during dark matter freeze-out in the early universe. If the dark matter annihilates into the new force carrier {phi}, its low mass can make hadronic modes kinematically inaccessible, forcing decays dominantly into leptons. If the force carrier is a non-Abelian gauge boson, the dark matter is part of a multiplet of states, and splittings between these states are naturally generated with size {alpha}m{sub {phi}}{approx} MeV, leading to the eXciting dark matter (XDM) scenario previously proposed to explain the positron annihilation in the galactic center observed by the INTEGRAL satellite; the light boson invoked by XDM to mediate a large inelastic scattering cross section is identified with the {phi} here. Somewhat smaller splittings would also be expected, providing a natural source for the parameters of the inelastic dark matter (iDM) explanation for the DAMA annual modulation signal. Since the Sommerfeld enhancement is most significant at low velocities, early dark matter halos at redshift {approx}10 potentially produce observable effects on the ionization history of the universe. Because of the enhanced cross section, detection of substructure is more probable than with a conventional WIMP. Moreover, the low velocity dispersion of dwarf galaxies and Milky Way subhalos can increase the substructure annihilation signal by an additional order of magnitude or more.

• OSTI ID: 21254742
• Journal Information: Physical Review. D, Particles Fields, Vol. 79, Issue 1; Other Information: DOI: 10.1103/PhysRevD.79.015014; (c) 2009 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); ISSN 0556-2821
• Country of Publication: United States
• Language: English

Related Subjects

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
ANNIHILATION
ASTROPHYSICS
BOSONS
COMPTON WAVELENGTH
COSMIC RADIATION
CROSS SECTIONS
GEV RANGE 100-1000
INELASTIC SCATTERING
IONIZATION
LEPTONS
MEV RANGE
MILKY WAY
MODULATION
NONLUMINOUS MATTER
PARTICLE DECAY
PIONS NEUTRAL
POSITRONS
RED SHIFT
UNIVERSE
WEAK INTERACTIONS