English
Related papers

Related papers: WIMP Dark Matter from Gravitino Decays and Leptoge…

200 papers

In supersymmetric axion models, if the gravitino or axino is the lightest SUSY particle (LSP), the other is often the next-to-LSP (NLSP). We investigate the cosmology of such a scenario and point out that the lifetime of the NLSP naturally…

High Energy Physics - Phenomenology · Physics 2017-07-12 Koichi Hamaguchi , Kazunori Nakayama , Yong Tang

Properties of neutrinos may be the origin of the matter-antimatter asymmetry of the universe. In the seesaw model for neutrino masses this leads to important constraints on the properties of light and heavy neutrinos. In particular, an…

High Energy Physics - Phenomenology · Physics 2011-08-17 W. Buchmuller , P. Di Bari , M. Plumacher

We study supersymmetric scenarios in which the gluino is the next-to-lightest supersymmetric particle (NLSP), with a mass sufficiently close to that of the lightest supersymmetric particle (LSP) that gluino coannihilation becomes important.…

High Energy Physics - Phenomenology · Physics 2016-03-23 John Ellis , Jason L. Evans , Feng Luo , Keith A. Olive

In the present work the primordial Big-Bang Nucleosynthesis (BBN) and weakly interacting massive particle (WIMP) dark matter are discussed in a certain class of modified gravitational theories, namely $f(R) \sim R^n$ gravity. The new…

Astrophysics · Physics 2010-05-28 Jin U Kang , Grigoris Panotopoulos

We review here the status of different dark matter candidates in the context of supersymmetric models, in particular the neutralino as a realization of the WIMP-mechanism and the gravitino. We give a summary of the recent bounds in direct…

High Energy Physics - Phenomenology · Physics 2015-06-17 Riccardo Catena , Laura Covi

The electroweak (EW) sector of the Minimal Supersymmetric Standard Model (MSSM) can account for a variety of experimental data. In particular, it can explain the persistent 3-4 sigma discrepancy between the experimental result for the…

High Energy Physics - Phenomenology · Physics 2021-12-22 Manimala Chakraborti , Sven Heinemeyer , Ipsita Saha

We present a search for an excess of neutrino interactions due to dark matter in the form of Weakly Interacting Massive Particles (WIMPs) annihilating in the galactic center or halo based on the data set of Super-Kamiokande-I, -II, -III and…

High Energy Physics - Experiment · Physics 2020-10-14 Kamiokande Collaboration , K. Abe , C. Bronner , Y. Haga , Y. Hayato , M. Ikeda , S. Imaizumi , H. Ito , K. Iyogi , J. Kameda , Y. Kataoka , Y. Kato , Y. Kishimoto , Ll. Marti , M. Miura , S. Moriyama , T. Mochizuki , Y. Nagao , M. Nakahata , Y. Nakajima , T. Nakajima , S. Nakayama , T. Okada , K. Okamoto , A. Orii , G. Pronost , H. Sekiya , M. Shiozawa , Y. Sonoda , A. Takeda , A. Takenaka , H. Tanaka , S. Tasaka , T. Tomura , K. Ueno , T. Yano , T. Yokozawa , R. Akutsu , S. Han , T. Irvine , T. Kajita , I. Kametani , K. P. Lee , T. McLachlan , K. Okumura , E. Richard , T. Tashiro , R. Wang , J. Xia , D. Bravo-Berguño , L. Labarga , P. Fernandez , F. d. M. Blaszczyk , J. Gustafson , C. Kachulis , E. Kearns , J. L. Raaf , J. L. Stone , L. R. Sulak , S. Sussman , L. Wan , T. Wester , S. Berkman , S. Tobayama , J. Bian , G. Carminati , M. Elnimr , N. J. Griskevich , W. R. Kropp , S. Locke , S. Mine , A. Renshaw , M. B. Smy , H. W. Sobel , V. Takhistov , P. Weatherly , B. L. Hartfiel , J. Hill , W. E. Keig , N. Hong , J. Y. Kim , I. T. Lim , R. G. Park , T. Akiri , B. Bodur , A. Himmel , Z. Li , E. O'Sullivan , K. Scholberg , C. W. Walter , T. Wongjirad , A. Coffani , O. Drapier , S. El Hedri , A. Giampaolo , M. Gonin , J. Imber , Th. A. Mueller , P. Paganini , B. Quilain , T. Ishizuka , T. Nakamura , J. S. Jang , K. Choi , J. G. Learned , S. Matsuno , S. N. Smith , J. Amey , L. H. V. Anthony , R. P. Litchfield , W. Y. Ma , A. A. Sztuc , Y. Uchida , M. O. Wascko , V. Berardi , M. G. Catanesi , R. A. Intonti , E. Radicioni , N. F. Calabria , L. N. Machado , G. De Rosa , G. Collazuol , F. Iacob , M. Lamoureux , N. Ospina , L. Ludovici , T. Boschi , F. Di Lodovico , S. Molina Sedgwick , S. Zsoldos , Y. Nishimura , S. Cao , M. Friend , T. Hasegawa , T. Ishida , T. Ishii , T. Kobayashi , T. Nakadaira , K. Nakamura , Y. Oyama , K. Sakashita , T. Sekiguchi , T. Tsukamoto , KE. Abe , M. Hasegawa , Y. Isobe , H. Miyabe , Y. Nakano , T. Shiozawa , T. Sugimoto , A. T. Suzuki , Y. Takeuchi , S. Yamamoto , A. Ali , Y. Ashida , T. Hayashino , T. Hiraki , S. Hirota , K. Huang , K. Ieki , M. Jiang , T. Kikawa , M. Mori , A. Murakami , KE. Nakamura , T. Nakaya , N. D. Patel , K. Suzuki , S. Takahashi , K. Tateishi , R. A. Wendell , N. McCauley , P. Mehta , A. Pritchard , K. M. Tsui , Y. Fukuda , Y. Itow , H. Menjo , G. Mitsuka , M. Murase , F. Muto , T. Niwa , K. Sato , T. Suzuki , M. Taani , z M. Tsukada , P. Mijakowski , K. Frankiewicz , J. Hignight , C. K. Jung , X. Li , J. L. Palomino , G. Santucci , C. Vilela , M. J. Wilking , C. Yanagisawa , D. Fukuda , K. Hagiwara , M. Harada , T. Horai , H. Ishino , S. Ito , T. Kayano , A. Kibayashi , Y. Koshio , W. Ma , T. Mori , H. Nagata , N. Piplani , M. Sakuda , S. Seiya , Y. Takahira , C. Xu , R. Yamaguchi , Y. Kuno , G. Barr , D. Barrow , L. Cook , C. Simpson , D. Wark , F. Nova , R. Tacik , J. Y. Yang , A. Cole , S. J. Jenkins , J. McElwee , M. Thiesse , L. Thompson , H. Okazawa , S. B. Kim , Y. Choi , K. Ito , K. Nishijima , K. Iwamoto , M. Koshiba , Y. Suda , M. Yokoyama , R. G. Calland , A. Goldsack , K. Martens , M. Murdoch , Y. Suzuki , M. R. Vagins , D. Hamabe , M. Kuze , Y. Okajima , M. Tanaka , T. Yoshida , M. Inomoto , M. Ishitsuka , R. Matsumoto , K. Ohta , M. Shinoki , J. F. Martin , C. M. Nantais , H. A. Tanaka , T. Towstego , M. Hartz , A. Konaka , P. de Perio , N. W. Prouse , S. Chen , B. D. Xu , Y. Zhang , B. Richards , K. Connolly , R. J. Wilkes , B. Jamieson , J. Walker , P. Giorgio , A. Minamino , K. Okamoto , G. Pintaudi

Within the Minimal Supersymmetric Standard Model (MSSM), LHC bounds suggest that scalar superpartner masses are far above the electroweak scale. Given a high superpartner mass, nonthermal dark matter is a viable alternative to WIMP dark…

High Energy Physics - Phenomenology · Physics 2014-02-05 Richard Easther , Richard Galvez , Ogan Ozsoy , Scott Watson

In the supersymmetric (SUSY) standard model, the lightest neutralino may be the lightest SUSY particle (LSP), and it is is a candidate of the dark matter in the universe. The LSP dark matter might be produced by the non-thermal process such…

High Energy Physics - Phenomenology · Physics 2009-10-31 J. Hisano , K. Kohri , M. M. Nojiri

Neutrino mass generation may affect the basic structure of the electroweak symmetry breaking sector. We consider a broad class of elementary particle theories where neutrinos get mass at a low mass scale. We show how these can be made…

High Energy Physics - Phenomenology · Physics 2007-05-23 F. Bazzocchi , J. W. F. Valle

Recently, the CoGeNT collaboration reported the WIMP candidate signal events exceeding the known backgrounds where the light WIMP with large cross section is supported. Motivated by this issue, we analyze a light neutralino dark matter…

High Energy Physics - Phenomenology · Physics 2010-12-30 Kyu Jung Bae , Hyung Do Kim , Seodong Shin

We show that in supersymmetric models with gauged B-L symmetry, there is a new source for cosmological lepton asymmetry. The Higgs bosons responsible for B-L gauge symmetry breaking decay dominantly into right-handed sneutrinos \tilde{N}…

High Energy Physics - Phenomenology · Physics 2010-01-05 K. S. Babu , Yanzhi Meng , Zurab Tavartkiladze

We present supersymmetric scenarios with gravitino LSP and stau NLSP in the case of a non-standard model of cosmology with the addition of a dark component in the pre-BBN era. In the context of the standard model of cosmology, gravitino LSP…

High Energy Physics - Phenomenology · Physics 2011-03-24 Sean Bailly

Supersymmetric models with low electroweak fine-tuning contain light higgsinos with mass not too far from m_h\simeq 125 GeV, while other sparticles can be much heavier. In the R-parity conserving MSSM, the lightest neutralino is then a…

High Energy Physics - Phenomenology · Physics 2013-06-19 Howard Baer , Vernon Barger , Dan Mickelson , Xerxes Tata

We consider the phenomenological implications of gravitino dark matter in the context of the $\mu\nu$SSM. The latter is an R-parity breaking model which provides a solution to the $\mu$-problem of the MSSM and explains the origin of…

High Energy Physics - Phenomenology · Physics 2009-12-10 Carlos Munoz

In supersymmetric models with gravity-mediated SUSY breaking and gaugino mass unification, the predicted relic abundance of neutralinos usually exceeds the strict limits imposed by the WMAP collaboration. One way to obtain the correct relic…

High Energy Physics - Phenomenology · Physics 2010-02-03 Howard Baer , Azar Mustafayev , Eun-Kyung Park , Stefano Profumo

We consider leptogenesis induced by soft supersymmetry breaking terms ("soft leptogenesis"), in the context of the inverse seesaw mechanism. In this model there are lepton number (L) conserving and L-violating soft supersymmetry-breaking…

High Energy Physics - Phenomenology · Physics 2010-10-27 J. Garayoa , M. C. Gonzalez-Garcia , N. Rius

We suggest a hybrid seesaw model where relatively ``light''right-handed neutrinos give no contribution to the neutrino mass matrix due to a special symmetry. This allows their Yukawa couplings to the standard model particles to be…

High Energy Physics - Phenomenology · Physics 2009-04-29 Pei-Hong Gu , M. Hirsch , Utpal Sarkar , J. W. F. Valle

The cosmological moduli problem is discussed in the framework of sequestered sector/anomaly-mediated supersymmetry (SUSY) breaking. In this scheme, the gravitino mass (corresponding to the moduli masses) is naturally 10 - 100 TeV, and hence…

High Energy Physics - Phenomenology · Physics 2009-09-15 Takeo Moroi , Lisa Randall

Weakly interacting massive particles (WIMPs) constitute a paradigm in the search for particle dark matter. In contrast to supersymmetry (SUSY), we explore the possibility that WIMP dark-matter acts as mediator of neutrino mass generation.…

High Energy Physics - Phenomenology · Physics 2025-09-03 Victor Martin Lozano , G. Sanchez Garcia , J. W. F. Valle