Results 21 to 30 of about 61,479 (226)

Search for bosonic super-weakly interacting massive particles at COSINE-100 [PDF]

Physical Review D, 2023
We present results of a search for bosonic super-weakly interacting massive particles (BSW) as keV scale dark matter candidates that is based on an exposure of 97.7 kg$\cdot$year from the COSINE experiment.
G. Adhikari, N. Carlin, J. J. Choi, S. Choi, A. Ezeribe, L. E. França, C. Ha, I. Hahn, S. J. Hollick, E. Jeon, J. Jo, H. Joo, W. Kang, M. Kauer, B. Kim, H. J. Kim, J. Kim, K. Kim, S. H. Kim, S. K. Kim, W. Kim, Y. Kim, Y. H. Kim, Y. Ko, D. Lee, E. K. Lee, H. Lee, H. Lee, H. Y. Lee, I. Lee, J. Lee, J. Lee, M. H. Lee, S. H. Lee, S. M. Lee, Y. J. Lee, D. Leonard, N. Luan, B. B. Manzato, R. Maruyama, R. J. Neal, J. Nikkel, S. Olsen, B. Park, H. Park, H. S. Park, K. Park, S. Park, R. Pitta, H. Prihtiadi, S. Ra, C. Rott, K. Shin, D. Cavalcante, A. Scarff, N. Spooner, W. Thompson, L. Yang, G. Yu   +58 more
semanticscholar   +1 more source

Results on low-mass weakly interacting massive particles from a 11 kg d target exposure of DAMIC at SNOLAB [PDF]

International Conference on Rebooting Computing, 2021
Experimental efforts of the last decades have been unsuccessful in detecting WIMPs (Weakly Interacting Massive Particles) in the 10-to-10$^4$ GeV/$c^2$ range, thus motivating the search for lighter dark matter.
A. Aguilar-Arevalo, D. Amidei, D. Baxter, G. Cancelo, B. Vergara, A. Chavarria, J. D'Olivo, J. Estrada, F. Favela-Pérez, R. Gaïor, Y. Guardincerri, E. Hoppe, T. Hossbach, B. Kilminster, I. Lawson, S. J. Lee, A. Letessier-Selvon, A. Matalon, P. Mitra, C. Overman, A. Piers, P. Privitera, K. Ramanathan, J. Da Rocha, Youssef Sarkis Mobarak, M. Settimo, R. Smida, R. Thomas, J. Tiffenberg, M. Traina, R. Vilar, A. Virto   +31 more
semanticscholar   +1 more source

Weakly interacting massive particle cross section limits from LOFAR observations of dwarf spheroidal galaxies [PDF]

Astronomy & Astrophysics, 2023
Weakly interacting massive particles (WIMPs) can self-annihilate, thus providing us with a way to indirectly detect dark matter (DM). Dwarf spheroidal (dSph) galaxies are excellent places to search for annihilation signals because they are rich in DM and
L. Gajovi'c, F. Welzmuller, V. Heesen, F. Gasperin, M. Vollmann, M. Bruggen, A. Basu, R. Beck, D. Schwarz, D. Bomans, A. Drabent   +10 more
semanticscholar   +1 more source

Improved Limits on Scattering of Weakly Interacting Massive Particles from Reanalysis of 2013 LUX Data. [PDF]

Physical Review Letters, 2015
We present constraints on weakly interacting massive particles (WIMP)-nucleus scattering from the 2013 data of the Large Underground Xenon dark matter experiment, including 1.4×10^{4}  kg day of search exposure.
D. Akerib, H. Araújo, X. Bai, A. Bailey, J. Balajthy, P. Beltrame, E. Bernard, A. Bernstein, T. P. Biesiadzinski, E. Boulton, A. Bradley, R. Bramante, S. Cahn, M. Carmona-Benitez, C. Chan, J. Chapman, A. A. Chiller, C. Chiller, A. Currie, J. Cutter, T. Davison, L. de Viveiros, A. Dobi, J. Dobson, E. Druszkiewicz, B. Edwards, C. Faham, S. Fiorucci, R. Gaitskell, V. Gehman, C. Ghag, K. Gibson, M. Gilchriese, C. Hall, M. Hanhardt, S. Haselschwardt, S. Hertel, D. Hogan, M. Horn, D. Huang, C. Ignarra, M. Ihm, R. Jacobsen, Wei Ji, K. Kazkaz, D. Khaitan, R. Knoche, N. Larsen, C. Lee, B. Lenardo, K. Lesko, A. Lindote, M. Lopes, D. Malling, A. Manalaysay, R. Mannino, M. F. Marzioni, D. McKinsey, D. Mei, J. Mock, M. Moongweluwan, J. Morad, A. Murphy, C. Nehrkorn, H. Nelson, F. Neves, K. O'Sullivan, K. Oliver-Mallory, R. Ott, K. Palladino, M. Pangilinan, E. K. Pease, P. Phelps, L. Reichhart, C. Rhyne, S. Shaw, T. Shutt, C. Silva, V. Solovov, P. Sorensen, S. Stephenson, T. Sumner, M. Szydagis, D. Taylor, W. Taylor, B. Tennyson, P. Terman, D. Tiedt, W. To, M. Tripathi, L. Tvrznikova, S. Uvarov, J. Verbus, R. Webb, J. White, T. Whitis, M. Witherell, F. Wolfs, K. Yazdani, S. Young, C. Zhang   +100 more
semanticscholar   +1 more source

Simulations of the Angular Kinetic-Energy Distribution of Halo Weakly Interacting Massive Particles for Directional Dark Matter Detection Experiments

, 2022
In this paper, as the second step of our study on developing data analysis procedures for using 3-dimensional information offered by directional Dark Matter detection experiments in the future, we investigate the patterns of the angular distribution of
Chung-Lin Shan
semanticscholar   +1 more source

Limits on Light Weakly Interacting Massive Particles from the First 102.8 kg×day Data of the CDEX-10 Experiment. [PDF]

Physical Review Letters, 2018
We report the first results of a light weakly interacting massive particles (WIMPs) search from the CDEX-10 experiment with a 10 kg germanium detector array immersed in liquid nitrogen at the China Jinping Underground Laboratory with a physics data size ...
H. Jiang, L. Jia, Q. Yue, K. Kang, J. Cheng, Y. J. Li, H. Wong, M. Ağartioğlu, H. An, J. Chang, J. Chen, Y. H. Chen, Z. Deng, Q. Du, H. Gong, L. He, J. Hu, Q. Hu, H. Huang, H. Li, H. Li, J. Li, J. Li, X. Li, X. Li, Y. Li, B. Liao, F. Lin, S. Lin, S. K. Liu, Y. Liu, Y. Liu, Z. Liu, H. Ma, J. Ma, H. Pan, J. Ren, X. Ruan, B. Sevda, V. Sharma, M. Shen, L. Singh, M. Singh, T. Sun, C. Tang, W. Tang, Y. Tian, G. Wang, J. M. Wang, L. Wang, Q. Wang, Y. Wang, S. Y. Wu, Y. C. Wu, H. Xing, Y. Xu, T. Xue, L. Yang, S. Yang, N. Yi, C. Yu, H. Yu, J. Yue, X. Zeng, M. Zeng, Z. Zeng, F. Zhang, Y. Zhang, M. Zhao, J. Zhou, Z. Zhou, J. Zhu, Zheng Hong Zhu   +72 more
semanticscholar   +1 more source

Response of mica to weakly interacting massive particles [PDF]

Physical Review C, 1995
We calculate spin-dependent cross sections for the scattering from mica of hypothetical weakly interacting dark-matter particles such as neutralinos. The most abundant odd-A isotopes in mica, Al27 and K39, require different shell-model treatments. The calculated cross sections will allow the interpretation of ongoing experiments that look for tracks ...
Engel, J., Ressell, M. T., Towner, I. S., Ormand, W. E   +3 more
openaire   +3 more sources

New Results from the Search for Low-Mass Weakly Interacting Massive Particles with the CDMS Low Ionization Threshold Experiment. [PDF]

Physical Review Letters, 2015
The CDMS low ionization threshold experiment (CDMSlite) uses cryogenic germanium detectors operated at a relatively high bias voltage to amplify the phonon signal in the search for weakly interacting massive particles (WIMPs).
R. Agnese, A. Anderson, T. Aramaki, M. Asai, W. Baker, D. Balakishiyeva, D. Barker, R. Basu Thakur, D. Bauer, J. Billard, A. Borgland, M. Bowles, P. Brink, R. Bunker, B. Cabrera, D. Caldwell, R. Calkins, D. Cerdeño, H. Chagani, Y. Chen, J. Cooley, B. Cornell, P. Cushman, M. Daal, P. Di Stefano, T. Doughty, L. Esteban, S. Fallows, E. Figueroa-Feliciano, M. Ghaith, G. Godfrey, S. Golwala, J. Hall, H. R. Harris, T. Hofer, D. Holmgren, L. Hsu, M. E. Huber, D. Jardin, A. Jastram, O. Kamaev, B. Kara, M. Kelsey, A. Kennedy, A. Leder, B. Loer, E. Lopez Asamar, P. Lukens, R. Mahapatra, V. Mandic, N. Mast, N. Mirabolfathi, R. Moffatt, J. Morales Mendoza, S. Oser, K. Page, W. Page, R. Partridge, M. Pepin, A. Phipps, K. Prasad, M. Pyle, H. Qiu, W. Rau, P. Redl, A. Reisetter, Y. Ricci, A. Roberts, H. Rogers, T. Saab, B. Sadoulet, J. Sander, K. Schneck, R. Schnee, S. Scorza, B. Serfass, B. Shank, D. Speller, D. Toback, R. Underwood, S. Upadhyayula, A. Villano, B. Welliver, J. S. Wilson, D. Wright, S. Yellin, J. Yen, B. Young, J. Zhang   +88 more
semanticscholar   +1 more source

Capture rate of weakly interacting massive particles (WIMPs) in binary star systems [PDF]

, 2020
Distribution of dark matter (DM) inside galaxies is not uniform. Near the central regions, its density is the highest. Then, it seems logical to suppose that, DM affects the physics of stars of central regions more than other regions.
Ebrahim Hassani, H. Ebadi, R. Pazhouhesh, Mohammad Hosseinirad   +3 more
semanticscholar   +1 more source

Results on the Spin-Dependent Scattering of Weakly Interacting Massive Particles on Nucleons from the Run 3 Data of the LUX Experiment. [PDF]

Physical Review Letters, 2016
We present experimental constraints on the spin-dependent WIMP (weakly interacting massive particle)-nucleon elastic cross sections from LUX data acquired in 2013.
D. Akerib, H. Araújo, X. Bai, A. Bailey, J. Balajthy, P. Beltrame, E. Bernard, A. Bernstein, T. P. Biesiadzinski, E. Boulton, A. Bradley, R. Bramante, S. Cahn, M. Carmona-Benitez, C. Chan, J. Chapman, A. A. Chiller, C. Chiller, A. Currie, J. Cutter, T. Davison, L. D. Viveiros, A. Dobi, J. Dobson, E. Druszkiewicz, B. Edwards, C. Faham, S. Fiorucci, R. Gaitskell, V. Gehman, C. Ghag, K. Gibson, M. Gilchriese, C. Hall, M. Hanhardt, S. Haselschwardt, S. Hertel, D. Hogan, M. Horn, D. Huang, C. Ignarra, M. Ihm, R. Jacobsen, Wei Ji, K. Kazkaz, D. Khaitan, R. Knoche, N. Larsen, C. Lee, B. Lenardo, K. Lesko, A. Lindote, M. Lopes, D. Malling, A. Manalaysay, R. Mannino, M. F. Marzioni, D. McKinsey, D. Mei, J. Mock, M. Moongweluwan, J. Morad, A. Murphy, C. Nehrkorn, H. Nelson, F. Neves, K. O'Sullivan, K. Oliver-Mallory, R. Ott, K. Palladino, M. Pangilinan, E. K. Pease, P. Phelps, L. Reichhart, C. Rhyne, S. Shaw, T. Shutt, C. Silva, V. Solovov, P. Sorensen, S. Stephenson, T. Sumner, M. Szydagis, D. Taylor, W. Taylor, B. Tennyson, P. Terman, D. Tiedt, W. To, M. Tripathi, L. Tvrznikova, S. Uvarov, J. Verbus, R. Webb, J. White, T. Whitis, M. Witherell, F. Wolfs, K. Yazdani, S. Young, Chao Zhang   +100 more
semanticscholar   +1 more source