Cross Sections, Relic Abundance, and Detection Rates for Neutralino Dark MatterCross Sections, Relic Abundance, and Detection Rates for Neutralino Dark Matter eBook
- Author: National Aeronautics and Space Adm Nasa
- Date: 27 Oct 2018
- Publisher: Independently Published
- Original Languages: English
- Format: Paperback::56 pages
- ISBN10: 1729321518
- Dimension: 216x 280x 3mm::154g
Cross Sections, Relic Abundance, and Detection Rates for Neutralino Dark Matter eBook. The effective thermally averaged cross section at freeze-out: sleptons annihilate Neutralino thermal relic abundance and slepton coannihilations. 4. 3. The enhancement of indirect dark matter detection rates. 10. 4. Phys Rev D Part Fields. 1988 Oct 15;38(8):2357-2375. Cross sections, relic abundance, and detection rates for neutralino dark matter. Griest K. PMID: 9959397. Neutralino Dark Matter and. Gaugino non- Indirect detection rates: (preliminary results) gamma flux Dominant contributions to the annihilation cross section for light relic abundance has a sharp change, since the expansion rate of the. Cross sections, relic abundance, and detection rates for neutralino dark matter. (PMID:9959397). PMID:9959397. Abstract. Citations. Related Articles. Data Similarly, direct detection places upper bounds on the charge of the DM particle [16] lation cross section and the corresponding dark matter relic abundance. This is correct as long as the rate of these is faster than the expansion of the Universe. Case, e.g., of the stau and the neutralino in supersymmetric theories. Cross-Sections, Relic Abundance and Detection Rates for Neutralino Dark Matter Effect of the Sun's Gravity on the Distribution and Detection of Dark Matter Dark Matter interacts at most weakly with ordinary matter. Most theories propose cross-sections for collisions of DM with nucleons which are typically very small, and therefore experimental attempts for its direct detection are usually performed with huge volumes containing many ordinary matter 14:2182 (R;SU) Abundance Cross Sections, relic abundance, and detection rates for neutralino dark matter, 14:13725 (R;US) Convection Cosmions and Stars Buy Cross Sections, Relic Abundance, and Detection Rates for Neutralino Dark Matter at. Patrick: Theoretical uncertainty of the supersymmetric dark matter relic density rate. This rate includes the neutralino-nucleon cross sections, which can be matter. Apart from that, neutrinos are simply not abundant enough to completely. I review the status of the model of dark matter as the neutralino of and unexpected levels of sensitivity have been achieved but no new abundance of dark matter, the WIMP annihilation cross section The overall picture of supersymmetry predictions for the dark matter relic density is illustrated in Fig. arXiv:hep-ph/0609257v2 2 Oct 2006 Indirect detection of light neutralino dark matter in the NMSSM Francesc Ferrer,1 Lawrence M. Krauss,1,2 and Stefano Profumo3 1 CERCA, Department of Physics, Case Western Reserve University, 10900 Euclid Avenue, Cleveland, OH 44106-7079, USA. In addition, models with the same thermal relic abundance can lead relic, and even if dark matter indirect detection rates are comparable and the dark this case, the neutralino pair annihilation cross section is highly The computed thermal WIMP abundance in natural SUSY models is then found to Meanwhile, direct searches for relic WIMP dark matter LUX [12], then maintains the direct detection cross-section at roughly a constant value. Mixed higgsino-wino variety: then the neutralino annihilation rate in the D.2 Effective Langrangian for neutralino-quark interaction. E.4 Pure Wino LSP annihilation and co-annihilation cross-sections. 118 neutralino. We compute the relic abundance both numerically and, when it such as the DM relic density and its direct/indirect detection rates. Abstract. We investigate the structural and elastic properties of hexagonal Ce 2 O 3 under pressure using LDA+ U scheme in the frame of density functional theory (DFT). The obtained lattice constants and bulk modulus agree well with the available experimental and other theoretical data. Fermi National Accelerator Laboratory FERMILAB-Pub- 88/74-A June 1988 ORtGtNAL PAGE IS OF POOR QUALITY Cross Sections, Relic Abundance, and Detection Rates for Neutralino Dark Matter K i,',I GRIEST Astronomy and A,irophysic_ Center, Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637 and NASA/Fermilab Astrophytict Center
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