Results 1 to 10 of about 61,445 (192)

Weakly-Interacting Massive Particles in Non-supersymmetric SO(10) Grand Unified Models [PDF]

Journal of High Energy Physics, 2015
Non-supersymmetric SO(10) grand unified theories provide a framework in which the stability of dark matter is explained while gauge coupling unification is realized. In this work, we systematically study this possibility by classifying weakly interacting
Nagata, Natsumi, Olive, Keith A., Zheng, Jiaming   +2 more
core   +5 more sources

Detectability of Weakly Interacting Massive Particles in the Sagittarius Dwarf Tidal Stream [PDF]

Physical Review D, 2003
Tidal streams of the Sagittarius dwarf spheroidal galaxy (Sgr) may be showering dark matter onto the solar system and contributing approx (0.3--23)% of the local density of our Galactic Halo. If the Sagittarius galaxy contains WIMP dark matter, the extra
A. Ali, D. W. Evans, F. Comerón, F. Mignard, G. Marconi, H. Wang, M. Feast, M. Mateo, M. W. Goodman, N. J. T. Smith, N. Padmanabhan, P. Gondolo, R. A. Ibata, R. Bernabei, R. Bernabei   +14 more
core   +6 more sources

Event Rates for the Scattering of Weakly Interacting Massive Particles from ²³Na and ⁴⁰Ar [PDF]

Particles, 2021
Detection rates for the elastic and inelastic scattering of weakly interacting massive particles (WIMPs) off 23Na are calculated within the framework of Deformed Shell Model (DSM) based on Hartree-Fock states.
R. Sahu, V. K. B. Kota, T. S. Kosmas
doaj   +2 more sources

Light weakly interacting massive particles [PDF]

Reports on Progress in Physics, 2016
Light weakly interacting massive particles (WIMPs) are dark matter particle candidates with weak scale interaction with the known particles, and mass in the GeV to tens of GeV range.
G. Gelmini
semanticscholar   +5 more sources

Limits on interactions between weakly interacting massive particles and nucleons obtained with NaI(Tl) crystal detectors [PDF]

Journal of High Energy Physics, 2019
Limits on the cross section for weakly interacting massive particles (WIMPs) elastic scattering on nuclei in NaI(Tl) detectors at the Yangyang Underground Laboratory are obtained from a 2967.4 kg·day data exposure.
The KIMS collaboration, K. W. Kim, G. Adhikari, P. Adhikari, S. Choi, C. Ha, I. S. Hahn, E. J. Jeon, H. W. Joo, W. G. Kang, H. J. Kim, N. Y. Kim, S. K. Kim, Y. D. Kim, Y. H. Kim, Y. J. Ko, H. S. Lee, J. S. Lee, J. Y. Lee, M. H. Lee, D. S. Leonard, S. L. Olsen, B. J. Park, H. K. Park, H. S. Park, K. S. Park   +25 more
doaj   +2 more sources

Does Solar Physics Provide Constraints to Weakly Interacting Massive Particles? [PDF]

Physical Review D, 2002
We investigate whether present data on helioseismology and solar neutrino fluxes may constrain WIMP--matter interactions in the range of WIMP parameters under current exploration in WIMP searches.
A. Bottino, A. Bottino, A. Bottino, A. Bottino, A. Bottino, A. Bottino, A. Bottino, A. Bottino, A. Bottino, A. Bottino, A. Bouquet, A. Gould, A. Gould, A. Gould, A. Morales, A.K. Drukier, B. Ricci, D. Dearborn, D.G. Cerdeño, D.N. Spergel, E. Accomando, E. Gabrielli, E. Lisi, F. Ciacio, F. L. Villante, F.L. Villante, G. Fiorentini, G. Fiorentini, G. Fiorentini, G.L. Fogli, G.L. Fogli, G.L. Fogli, I. Lopes, I.P. Lopes, J. Christensen-Dalsgaard, J. Kaplan, J.L. Feng, J.N. Bahcall, J.N. Bahcall, J.N. Bahcall, K. Freese, K. Griest, M.E. Gómez, N. Fornengo, N. Fornengo, P. Belli, P. Belli, Q.R. Ahmad, Q.R. Ahmad, R. Arnowitt, R. Bernabei, R. Bernabei, R. Bernabei, R. Gilliland, S. Basu, S. Degl’Innocenti, S. Esposito, S. Fukuda, S. Scopel, S. Turck-Chieze, S. Turck-Chieze, T.K. Gaisser, W.A. Dziembowski, W.H. Press   +63 more
core   +4 more sources

Search for low-mass weakly interacting massive particles with SuperCDMS. [PDF]

Physical Review Letters, 2014
We report a first search for weakly interacting massive particles (WIMPs) using the background rejection capabilities of SuperCDMS. An exposure of 577 kg days was analyzed for WIMPs with mass
R. Agnese, A. Anderson, M. Asai, D. Balakishiyeva, R. Basu Thakur, D. Bauer, J. Beaty, J. Billard, A. Borgland, M. Bowles, D. Brandt, P. Brink, R. Bunker, B. Cabrera, D. Caldwell, D. Cerdeño, H. Chagani, Y. Chen, M. Cherry, J. Cooley, B. Cornell, C. Crewdson, P. Cushman, M. Daal, D. DeVaney, P. Di Stefano, E. Silva, T. Doughty, L. Esteban, S. Fallows, E. Figueroa-Feliciano, G. Godfrey, S. Golwala, J. Hall, S. Hansen, H. R. Harris, S. Hertel, B. Hines, T. Hofer, D. Holmgren, L. Hsu, M. E. Huber, A. Jastram, O. Kamaev, B. Kara, M. Kelsey, S. Kenany, A. Kennedy, M. Kiveni, K. Koch, A. Leder, B. Loer, E. Lopez Asamar, R. Mahapatra, V. Mandic, C. Martinez, K. McCarthy, N. Mirabolfathi, R. Moffatt, R. Nelson, L. Novak, K. Page, R. Partridge, M. Pepin, A. Phipps, M. Platt, K. Prasad, M. Pyle, H. Qiu, W. Rau, P. Redl, A. Reisetter, R. Resch, Y. Ricci, M. Ruschman, T. Saab, B. Sadoulet, J. Sander, R. Schmitt, K. Schneck, R. Schnee, S. Scorza, D. Seitz, B. Serfass, B. Shank, D. Speller, A. Tomada, S. Upadhyayula, A. Villano, B. Welliver, D. Wright, S. Yellin, J. Yen, B. Young, J. Zhang   +94 more
semanticscholar   +5 more sources

Baryogenesis for weakly interacting massive particles [PDF]

Physical Review D, 2012
We propose a robust, unified framework, in which the similar baryon and dark matter cosmic abundances both arise from the physics of weakly interacting massive particles (WIMPs), with the rough quantitative success of the so-called "WIMP miracle".
Yanou Cui, R. Sundrum
semanticscholar   +3 more sources

Calculating the annihilation rate of weakly interacting massive particles. [PDF]

Physical Review Letters, 2014
We develop a formalism that allows one to systematically calculate the weakly interacting massive particle (WIMP) annihilation rate into gamma rays whose energy far exceeds the weak scale.
M. Baumgart, I. Rothstein, V. Vaidya
semanticscholar   +4 more sources

Coherence in Scattering of Massive Weakly Interacting Neutral Particles of Nuclei [PDF]

Physics of Particles and Nuclei, 2023
The paper presents a novel approach to the description of the nonrelativistic weak interaction of a massive neutral particle (lepton) and a nucleus, in which the latter retains its integrity.
V. Bednyakov
semanticscholar   +3 more sources