Precise relic WIMP abundance and its impact on searches for dark matter annihilation
Published 2012 View Full Article
- Home
- Publications
- Publication Search
- Publication Details
Title
Precise relic WIMP abundance and its impact on searches for dark matter annihilation
Authors
Keywords
-
Journal
PHYSICAL REVIEW D
Volume 86, Issue 2, Pages -
Publisher
American Physical Society (APS)
Online
2012-07-06
DOI
10.1103/physrevd.86.023506
References
Ask authors/readers for more resources
Related references
Note: Only part of the references are listed.- Results from 730 kg days of the CRESST-II Dark Matter search
- (2012) G. Angloher et al. EUROPEAN PHYSICAL JOURNAL C
- WMAP7 and future CMB constraints on annihilating dark matter: implications for GeV-scale WIMPs
- (2011) G. Hütsi et al. ASTRONOMY & ASTROPHYSICS
- DARK MATTER AND SYNCHROTRON EMISSION FROM GALACTIC CENTER RADIO FILAMENTS
- (2011) Tim Linden et al. ASTROPHYSICAL JOURNAL
- SEVEN-YEARWILKINSON MICROWAVE ANISOTROPY PROBE(WMAP) OBSERVATIONS: COSMOLOGICAL INTERPRETATION
- (2011) E. Komatsu et al. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
- New results from DAMA/LIBRA
- (2011) R. Bernabei et al. EUROPEAN PHYSICAL JOURNAL C
- Cosmic-ray antiproton constraints on light singlino-like dark matter candidates
- (2011) David G. Cerdeño et al. NUCLEAR PHYSICS B
- Gamma rays from the Galactic center and the WMAP haze
- (2011) Dan Hooper et al. PHYSICAL REVIEW D
- Search for dark matter from the Galactic halo with the IceCube Neutrino Telescope
- (2011) R. Abbasi et al. PHYSICAL REVIEW D
- Origin of the gamma rays from the Galactic Center
- (2011) Dan Hooper et al. PHYSICAL REVIEW D
- Updated CMB constraints on dark matter annihilation cross sections
- (2011) Silvia Galli et al. PHYSICAL REVIEW D
- Constraining Dark Matter Models from a Combined Analysis of Milky Way Satellites with the Fermi Large Area Telescope
- (2011) M. Ackermann et al. PHYSICAL REVIEW LETTERS
- Exclusion of Canonical Weakly Interacting Massive Particles by Joint Analysis of Milky Way Dwarf Galaxies with Data from the Fermi Gamma-Ray Space Telescope
- (2011) Alex Geringer-Sameth et al. PHYSICAL REVIEW LETTERS
- Search for an Annual Modulation in ap-Type Point Contact Germanium Dark Matter Detector
- (2011) C. E. Aalseth et al. PHYSICAL REVIEW LETTERS
- Results from a Search for Light-Mass Dark Matter with ap-Type Point Contact Germanium Detector
- (2011) C. E. Aalseth et al. PHYSICAL REVIEW LETTERS
- Dark matter annihilation in the Galactic Center as seen by the Fermi Gamma Ray Space Telescope
- (2011) Dan Hooper et al. PHYSICS LETTERS B
- Scale for the Phase Diagram of Quantum Chromodynamics
- (2011) S. Gupta et al. SCIENCE
- Constraints on cosmological dark matter annihilation from the Fermi-LAT isotropic diffuse gamma-ray measurement
- (2010) A.A Abdo et al. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
- Conservative constraints on dark matter from the Fermi-LAT isotropic diffuse gamma-ray background spectrum
- (2010) Kevork N Abazajian et al. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
- Constraints on dark matter annihilation in clusters of galaxies with the Fermi large area telescope
- (2010) M Ackermann et al. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
- Review of Particle Physics
- (2010) K Nakamura et al. JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS
- Gamma rays and neutrinos from dark matter annihilation in galaxy clusters
- (2010) Qiang Yuan et al. PHYSICAL REVIEW D
- Confronting the direct search of low mass dark matter from CoGeNT data with antiproton PAMELA data
- (2010) Wai-Yee Keung et al. PHYSICAL REVIEW D
- From PAMELA to CDMS and back
- (2010) Qing-Hong Cao et al. PHYSICS LETTERS B
- Constraints on Dark Matter annihilations from reionization and heating of the intergalactic gas
- (2009) Marco Cirelli et al. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
Discover Peeref hubs
Discuss science. Find collaborators. Network.
Join a conversationCreate your own webinar
Interested in hosting your own webinar? Check the schedule and propose your idea to the Peeref Content Team.
Create Now