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Cosmological observations have in the past few years become an increasingly powerful method for determining parameters within the neutrino sector, such as the presence of sterile states and the mass of neutrinos. I review the current status…

Astrophysics · Physics 2007-05-23 Steen Hannestad

Based on the community input at the National Academy of Sciences (NAS) Madison and Austin workshops in July and December 2017, respectively, this whitepaper was prepared and submitted to the NAS in the category of US fusion theory and…

We study neutrino and dark matter based on a gauged $U(1)_R$ symmetry in a framework of radiative seesaw scenario. Identifying dark matter as a bosoninc particle, it interacts with quark and lepton sectors through vector-like heavier quark…

High Energy Physics - Phenomenology · Physics 2021-05-27 Keiko I. Nagao , Hiroshi Okada

A search for a neutrino signal from WIMP pair annihilations in the centre of the Earth has been performed with the data collected with the ANTARES neutrino telescope from 2007 to 2012. The event selection criteria have been developed and…

High Energy Physics - Experiment · Physics 2017-04-20 ANTARES Collaboration , A. Albert , M. André , M. Anghinolfi , G. Anton , M. Ardid , J. -J. Aubert , T. Avgitas , B. Baret , J. Barrios-Martí , S. Basa , V. Bertin , S. Biagi , R. Bormuth , S. Bourret , M. C. Bouwhuis , R. Bruijn , J. Brunner , J. Busto , A. Capone , L. Caramete , J. Carr , S. Celli , T. Chiarusi , M. Circella , J. A. B. Coelho , A. Coleiro , R. Coniglione , H. Costantini , P. Coyle , A. Creusot , A. Deschamps , G. De Bonis , C. Distefano , I. Di Palma , C. Donzaud , D. Dornic , D. Drouhin , T. Eberl , I. El Bojaddaini , D. Elsässer , A. Enzenhöfer , I. Felis , L. A. Fusco , S. Galatà , P. Gay , S. Geißelsöder , K. Geyer , V. Giordano , A. Gleixner , H. Glotin , T. Grégoire , R. Gracia Ruiz , K. Graf , S. Hallmann , H. van Haren , A. J. Heijboer , Y. Hello , J. J. Hernández-Rey , J. Hößl , J. Hofestädt , C. Hugon , G. Illuminati , C. W. James , M. de Jong , M. Jongen , M. Kadler , O. Kalekin , U. Katz , D. Kießling , A. Kouchner , M. Kreter , I. Kreykenbohm , V. Kulikovskiy , C. Lachaud , R. Lahmann , D. Lefèvre , E. Leonora , M. Lotze , S. Loucatos , M. Marcelin , A. Margiotta , A. Marinelli , J. A. Martínez-Mora , A. Mathieu , R. Mele , K. Melis , T. Michael , P. Migliozzi , A. Moussa , C. Mueller , E. Nezri , G. E. Păvălaş , C. Pellegrino , C. Perrina , P. Piattelli , V. Popa , T. Pradier , L. Quinn , C. Racca , G. Riccobene , K. Roensch , A. Sánchez-Losa , M. Saldaña , I. Salvadori , D. F. E. Samtleben , M. Sanguineti , P. Sapienza , J. Schnabel , F. Schüssler , T. Seitz , C. Sieger , M. Spurio , Th. Stolarczyk , M. Taiuti , Y. Tayalati , A. Trovato , M. Tselengidou , D. Turpin , C. Tönnis , B. Vallage , C. Vallée , V. Van Elewyck , D. Vivolo , A. Vizzoca , S. Wagner , J. Wilms , J. D. Zornoza , J. Zúñiga

To answer the very interesting questions raised by the discovery of neutrino mass, an effective, coherent strategy is needed. To foster the development of such a strategy, the American Physical Society's Divisions of Nuclear Physics and of…

Popular Physics · Physics 2009-09-29 Stuart J. Freedman , Boris Kayser

I review progress that has been made in nuclear astrophysics over the past few years and summarize some of the questions that remain. Topics selected include solar neutrinos, supernovae (the explosion and associated nucleosynthesis),…

Nuclear Theory · Physics 2009-11-11 W. C. Haxton

This is a survey of the current experimental information on some of the interesting issues in neutrino physics: neutrino species, neutrino masses, neutrino magnetic moments, solar neutrinos, and the atmospheric neutrino anomaly.

High Energy Physics - Phenomenology · Physics 2009-10-28 K. V. L. Sarma

The connection between cosmological observations and neutrino physics is discussed in detail. Neutrinos decouple from thermal contact in the early Universe at a temperature of order 1 MeV which coincides with the temperature where light…

High Energy Physics - Phenomenology · Physics 2008-11-26 Steen Hannestad

Considering $Z_4$ symmetry in Type I seesaw scenario, one could obtain mass-squared differences of light neutrinos, mixings and $CP$ violating phase within $3 \sigma$ confidence level based on neutrino oscillation data. This is possible…

High Energy Physics - Phenomenology · Physics 2026-04-07 Kunal Pandey , Rathin Adhikari

A thorough understanding of neutrino cross sections in a wide range of energies is crucial for the successful execution of the entire neutrino physics program. In order to extract neutrino properties, long-baseline experiments need an…

Dark matter candidates arising in models of particle physics incorporating weak scale supersymmetry may produce detectable signals through their annihilation into neutrinos, photons, or positrons. A large number of relevant experiments are…

Astrophysics · Physics 2009-10-09 Jonathan L. Feng , Konstantin T. Matchev , Frank Wilczek

Nuclear reactors are uniquely powerful, abundant, and flavor-pure sources of antineutrinos that continue to play a vital role in the US neutrino physics program. The US reactor antineutrino physics community is a diverse interest group…

About 40 years ago, the neutrino was ruled out as the dark matter particle based on several arguments. Here I use the well-established concept of quantum uncertainties of position and momentum to describe the decoupling of neutrinos from…

High Energy Physics - Phenomenology · Physics 2023-08-28 Roman Schnabel

There is a puzzling contradiction: direct observations favor a low-mass density universe, but the only model which fits universe structure over more than three orders of magnitude in distance scale has a mix of hot (neutrino) and cold dark…

High Energy Physics - Phenomenology · Physics 2007-05-23 David O. Caldwell

Review talk presented at the Texas/PASCOS Symposium, Berkeley, CA, Dec 1992. We review the status of experiments and ideas relevant for the detection of the dark matter which is suspected to be the dominant constituent of the Universe.…

High Energy Physics - Phenomenology · Physics 2009-10-22 Kim Griest

I review the physics of axions, paying attention to the role as dark matter. This paper is based on talks given at the workshops ``Thinking, Observing and Mining the Universe'' held in Sorrento (Italy), September 22-27, 2003, and at…

High Energy Physics - Phenomenology · Physics 2007-05-23 Eduard Masso

Status of determination of the neutrino masses and mixing is formulated and possible uncertainties, especially due to presence of the sterile neutrinos, are discussed. The data hint an existence of special ``neutrino'' symmetries. If not…

High Energy Physics - Phenomenology · Physics 2009-11-11 Alexei Yu. Smirnov

The field of neutrino physics was covered at DPF 2013 in 32 talks, including three on theoretical advances and the remainder on experiments that spanned at least 17 different detectors. This summary of those talks cannot do justice to the…

High Energy Physics - Experiment · Physics 2013-10-28 Deborah A. Harris

This white paper addresses the hypothesis of light sterile neutrinos based on recent anomalies observed in neutrino experiments and the latest astrophysical data.

High Energy Physics - Phenomenology · Physics 2012-04-25 K. N. Abazajian , M. A. Acero , S. K. Agarwalla , A. A. Aguilar-Arevalo , C. H. Albright , S. Antusch , C. A. Arguelles , A. B. Balantekin , G. Barenboim , V. Barger , P. Bernardini , F. Bezrukov , O. E. Bjaelde , S. A. Bogacz , N. S. Bowden , A. Boyarsky , A. Bravar , D. Bravo Berguno , S. J. Brice , A. D. Bross , B. Caccianiga , F. Cavanna , E. J. Chun , B. T. Cleveland , A. P. Collin , P. Coloma , J. M. Conrad , M. Cribier , A. S. Cucoanes , J. C. D'Olivo , S. Das , A. de Gouvea , A. V. Derbin , R. Dharmapalan , J. S. Diaz , X. J. Ding , Z. Djurcic , A. Donini , D. Duchesneau , H. Ejiri , S. R. Elliott , D. J. Ernst , A. Esmaili , J. J. Evans , E. Fernandez-Martinez , E. Figueroa-Feliciano , B. T. Fleming , J. A. Formaggio , D. Franco , J. Gaffiot , R. Gandhi , Y. Gao , G. T. Garvey , V. N. Gavrin , P. Ghoshal , D. Gibin , C. Giunti , S. N. Gninenko , V. V. Gorbachev , D. S. Gorbunov , R. Guenette , A. Guglielmi , F. Halzen , J. Hamann , S. Hannestad , W. Haxton , K. M. Heeger , R. Henning , P. Hernandez , P. Huber , W. Huelsnitz , A. Ianni , T. V. Ibragimova , Y. Karadzhov , G. Karagiorgi , G. Keefer , Y. D. Kim , J. Kopp , V. N. Kornoukhov , A. Kusenko , P. Kyberd , P. Langacker , Th. Lasserre , M. Laveder , A. Letourneau , D. Lhuillier , Y. F. Li , M. Lindner , J. M. Link , B. L. Littlejohn , P. Lombardi , K. Long , J. Lopez-Pavon , W. C. Louis , L. Ludhova , J. D. Lykken , P. A. N. Machado , M. Maltoni , W. A. Mann , D. Marfatia , C. Mariani , V. A. Matveev , N. E. Mavromatos , A. Melchiorri , D. Meloni , O. Mena , G. Mention , A. Merle , E. Meroni , M. Mezzetto , G. B. Mills , D. Minic , L. Miramonti , D. Mohapatra , R. N. Mohapatra , C. Montanari , Y. Mori , Th. A. Mueller , H. P. Mumm , V. Muratova , A. E. Nelson , J. S. Nico , E. Noah , J. Nowak , O. Yu. Smirnov , M. Obolensky , S. Pakvasa , O. Palamara , M. Pallavicini , S. Pascoli , L. Patrizii , Z. Pavlovic , O. L. G. Peres , H. Pessard , F. Pietropaolo , M. L. Pitt , M. Popovic , J. Pradler , G. Ranucci , H. Ray , S. Razzaque , B. Rebel , R. G. H. Robertson , W. Rodejohann , S. D. Rountree , C. Rubbia , O. Ruchayskiy , P. R. Sala , K. Scholberg , T. Schwetz , M. H. Shaevitz , M. Shaposhnikov , R. Shrock , S. Simone , M. Skorokhvatov , M. Sorel , A. Sousa , D. N. Spergel , J. Spitz , L. Stanco , I. Stancu , A. Suzuki , T. Takeuchi , I. Tamborra , J. Tang , G. Testera , X. C. Tian , A. Tonazzo , C. D. Tunnell , R. G. Van de Water , L. Verde , E. P. Veretenkin , C. Vignoli , M. Vivier , R. B. Vogelaar , M. O. Wascko , J. F. Wilkerson , W. Winter , Y. Y. Y. Wong , T. T. Yanagida , O. Yasuda , M. Yeh , F. Yermia , Z. W. Yokley , G. P. Zeller , L. Zhan , H. Zhang

Despite direct observations favoring a low mass density, a critical density universe with a neutrino component of dark matter provides the best existing model to explain the observed structure of the universe over more than three orders of…

Astrophysics · Physics 2009-10-31 David O. Caldwell
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