CMB and 21-cm Signals for Dark Matter with a Long-Lived Excited State
arXiv:0805.3531 · doi:10.1103/PhysRevD.78.063530
Abstract
Motivated by the eXciting Dark Matter (XDM) model of Finkbeiner & Weiner, hypothesized to explain the 511 keV signal in the center of the Milky Way, we consider the CMB and 21-cm signatures of models of dark matter with collisional long-lived excited states. We compute the relic excitation fraction from the early universe for a variety of assumptions about the collisional de-excitation cross-section and thermal decoupling. The relic excitation fraction can be as high as 1% for natural regions of parameter space, but could be orders of magnitude smaller. Since the lifetime of the excited state is naturally greater than 10^13s, we discuss the signatures of such relic excitation on cosmic microwave background (CMB) and high-z 21-cm observations. Such models have potentially richer astrophysical signals than the traditional WIMP annihilations and decays, and may have observable consequences for future generations of experiments.
11 pages, 11 figures, slightly revised, Phys. Rev. D in press
References in corpus (12)
- Three Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization Analysis
- Exciting Dark Matter and the INTEGRAL/SPI 511 keV signal
- Impact of dark matter decays and annihilations on reionization
- The Effects of Dark Matter Decay and Annihilation on the High-Redshift 21 cm Background
- The sky distribution of positronium annihilation continuum emission measured with SPI/INTEGRAL
- The galactic 511 keV line from electroweak scale WIMPs
- The impact of dark matter decays and annihilations on the formation of the first structures
- Constraining DM through 21 cm observations
- Spin Exchange Rates in Electron-Hydrogen Collisions
- Intergalactic medium heating by dark matter
- The Spin-Resolved Atomic Velocity Distribution and 21-cm Line Profile of Dark-Age Gas
- The Accelerated Recombination, and the ACBAR and WMAP data
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- Searching for Dark Matter in the CMB: A Compact Parameterization of Energy Injection from New Physics
- Energy Injection And Absorption In The Cosmic Dark Ages
- Direct Detection of Multi-component Secluded WIMPs
- Dark matter-neutrino interactions through the lens of their cosmological implications
- Constraints on dark matter annihilation from CMB observations before Planck
- An X-Ray Line from eXciting Dark Matter
- Constraining dark matter late-time energy injection: decays and p-wave annihilations
- Consistent Scenarios for Cosmic-Ray Excesses from Sommerfeld-Enhanced Dark Matter Annihilation
- PAMELA, DAMA, INTEGRAL and Signatures of Metastable Excited WIMPs
- Self-interacting inelastic dark matter: A viable solution to the small scale structure problems
- Lifetime Constraints for Late Dark Matter Decay
- A Dark Matter Model with Non-Abelian Gauge Symmetry
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- Nonabelian dark matter models for 3.5 keV X-rays
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- A Model For Late Dark Matter Decay
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- Perturbed Recombination from Dark Matter Annihilation
- Cosmic Microwave Background Constraints on Dark Matter Models of the Galactic Center 511 keV Signal
- MiXDM: Cosmic Ray Signals from Multiple States of Dark Matter
- The Hydrogen Mixing Portal, Its Origins, and Its Cosmological Effects