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Research in neutrino physics has been very active, both in experimental advances, with a new generation of detectors in operation and planning, and in theoretical discussions regarding the fundamental nature of the neutrino. This scientific…

High Energy Physics - Phenomenology · Physics 2024-12-24 Adriano Cherchiglia , Macello Jales , Guilherme Nogueira , Maressa P. Sampaio , Pedro C. de Holanda

The manuscript reviews progress achieved in recent years in various aspects of nuclear astrophysics, including stellar nucleosynthesis, nuclear aspects of supernova collapse and explosion, neutrino-induced reactions and their possible role…

Nuclear Theory · Physics 2008-11-26 K. Langanke

A brief sketch is made of the present observational status of neutrino physics, with emphasis on the hints that follow from solar and atmospheric neutrino observations, as well as cosmological data on the amplitude of primordial density…

High Energy Physics - Phenomenology · Physics 2009-09-17 J. W. F. Valle

Understanding the physics of neutrinos is of paramount relevance for the development of high energy physics, cosmology and astrophysics, thanks to their characteristics and phenomenology. In particular, the property of changing flavor while…

High Energy Physics - Experiment · Physics 2018-12-13 Mario A. Acero

A review of the problem of neutrino mass, mixing and oscillations is given. Possible phenomenological schemes of neutrino mixing are discussed. The most important consequences of neutrino mixing--neutrino oscillations are considered in some…

High Energy Physics - Phenomenology · Physics 2007-05-23 W. M. Alberico , S. M. Bilenky

The Proceedings of the 2011 workshop on Fundamental Physics at the Intensity Frontier. Science opportunities at the intensity frontier are identified and described in the areas of heavy quarks, charged leptons, neutrinos, proton decay, new…

High Energy Physics - Experiment · Physics 2012-05-14 J. L. Hewett , H. Weerts , R. Brock , J. N. Butler , B. C. K. Casey , J. Collar , A. de Gouvea , R. Essig , Y. Grossman , W. Haxton , J. A. Jaros , C. K. Jung , Z. T. Lu , K. Pitts , Z. Ligeti , J. R. Patterson , M. Ramsey-Musolf , J. L. Ritchie , A. Roodman , K. Scholberg , C. E. M. Wagner , G. P. Zeller , S. Aefsky , A. Afanasev , K. Agashe , C. Albright , J. Alonso , C. Ankenbrandt , M. Aoki , C. A. Arguelles , N. Arkani-Hamed , J. R. Armendariz , C. Armendariz-Picon , E. Arrieta Diaz , J. Asaadi , D. M. Asner , K. S. Babu , K. Bailey , O. Baker , B. Balantekin , B. Baller , M. Bass , B. Batell , J. Beacham , J. Behr , N. Berger , M. Bergevin , E. Berman , R. Bernstein , A. J. Bevan , M. Bishai , M. Blanke , S. Blessing , A. Blondel , T. Blum , G. Bock , A. Bodek , G. Bonvicini , F. Bossi , J. Boyce , R. Breedon , M. Breidenbach , S. J. Brice , R. A. Briere , S. Brodsky , C. Bromberg , A. Bross , T. E. Browder , D. A. Bryman , M. Buckley , R. Burnstein , E. Caden , P. Campana , R. Carlini , G. Carosi , C. Castromonte , R. Cenci , I. Chakaberia , M. C. Chen , C. H. Cheng , B. Choudhary , N. H. Christ , E. Christensen , M. E. Christy , T. E. Chupp , E. Church , D. B. Cline , T. E. Coan , P. Coloma , J. Comfort , L. Coney , J. Cooper , R. J. Cooper , R. Cowan , D. F. Cowen , D. Cronin-Hennessy , A. Datta , G. S. Davies , M. Demarteau , D. P. DeMille , A. Denig , R. Dermisek , A. Deshpande , M. S. Dewey , R. Dharmapalan , J. Dhooghe , M. R. Dietrich , M. Diwan , Z. Djurcic , S. Dobbs , M. Duraisamy , B. Dutta , H. Duyang , D. A. Dwyer , M. Eads , B. Echenard , S. R. Elliott , C. Escobar , J. Fajans , S. Farooq , C. Faroughy , J. E. Fast , B. Feinberg , J. Felde , G. Feldman , P. Fierlinger , P. Fileviez Perez , B. Filippone , P. Fisher , B. T. Flemming , K. T. Flood , R. Forty , M. J. Frank , A. Freyberger , A. Friedland , R. Gandhi , K. S. Ganezer , A. Garcia , F. G. Garcia , S. Gardner , L. Garrison , A. Gasparian , S. Geer , V. M. Gehman , T. Gershon , M. Gilchriese , C. Ginsberg , I. Gogoladze , M. Gonderinger , M. Goodman , H. Gould , M. Graham , P. W. Graham , R. Gran , J. Grange , G. Gratta , J. P. Green , H. Greenlee , R. C. Group , E. Guardincerri , V. Gudkov , R. Guenette , A. Haas , A. Hahn , T. Han , T. Handler , J. C. Hardy , R. Harnik , D. A. Harris , F. A. Harris , P. G. Harris , J. Hartnett , B. He , B. R. Heckel , K. M. Heeger , S. Henderson , D. Hertzog , R. Hill , E. A Hinds , D. G. Hitlin , R. J. Holt , N. Holtkamp , G. Horton-Smith , P. Huber , W. Huelsnitz , J. Imber , I. Irastorza , J. Jaeckel , I. Jaegle , C. James , A. Jawahery , D. Jensen , C. P. Jessop , B. Jones , H. Jostlein , T. Junk , A. L. Kagan , M. Kalita , Y. Kamyshkov , D. M. Kaplan , G. Karagiorgi , A. Karle , T. Katori , B. Kayser , R. Kephart , S. Kettell , Y. K. Kim , M. Kirby , K. Kirch , J. Klein , J. Kneller , A. Kobach , M. Kohl , J. Kopp , M. Kordosky , W. Korsch , I. Kourbanis , A. D. Krisch , P. Krizan , A. S. Kronfeld , S. Kulkarni , K. S. Kumar , Y. Kuno , T. Kutter , T. Lachenmaier , M. Lamm , J. Lancaster , M. Lancaster , C. Lane , K. Lang , P. Langacker , S. Lazarevic , T. Le , K. Lee , K. T. Lesko , Y. Li , M. Lindgren , A. Lindner , J. Link , D. Lissauer , L. S. Littenberg , B. Littlejohn , C. Y. Liu , W. Loinaz , W. Lorenzon , W. C. Louis , J. Lozier , L. Ludovici , L. Lueking , C. Lunardini , D. B. MacFarlane , P. A. N. Machado , P. B. Mackenzie , J. Maloney , W. J. Marciano , W. Marsh , M. Marshak , J. W. Martin , C. Mauger , K. S. McFarland , C. McGrew , G. McLaughlin , D. McKeen , R. McKeown , B. T. Meadows , R. Mehdiyev , D. Melconian , H. Merkel , M. Messier , J. P. Miller , G. Mills , U. K. Minamisono , S. R. Mishra , I. Mocioiu , S. Moed Sher , R. N. Mohapatra , B. Monreal , C. D. Moore , J. G. Morfin , J. Mousseau , L. A. Moustakas , G. Mueller , P. Mueller , M. Muether , H. P. Mumm , C. Munger , H. Murayama , P. Nath , O. Naviliat-Cuncin , J. K. Nelson , D. Neuffer , J. S. Nico , A. Norman , D. Nygren , Y. Obayashi , T. P. O'Connor , Y. Okada , J. Olsen , L. Orozco , J. L. Orrell , J. Osta , B. Pahlka , J. Paley , V. Papadimitriou , M. Papucci , S. Parke , R. H. Parker , Z. Parsa , K. Partyka , A. Patch , J. C. Pati , R. B. Patterson , Z. Pavlovic , G. Paz , G. N. Perdue , D. Perevalov , G. Perez , R. Petti , W. Pettus , A. Piepke , M. Pivovaroff , R. Plunkett , C. C. Polly , M. Pospelov , R. Povey , A. Prakesh , M. V. Purohit , S. Raby , J. L. Raaf , R. Rajendran , S. Rajendran , G. Rameika , R. Ramsey , A. Rashed , B. N. Ratcliff , B. Rebel , J. Redondo , P. Reimer , D. Reitzner , F. Ringer , A. Ringwald , S. Riordan , B. L. Roberts , D. A. Roberts , R. Robertson , F. Robicheaux , M. Rominsky , R. Roser , J. L. Rosner , C. Rott , P. Rubin , N. Saito , M. Sanchez , S. Sarkar , H. Schellman , B. Schmidt , M. Schmitt , D. W. Schmitz , J. Schneps , A. Schopper , P. Schuster , A. J. Schwartz , M. Schwarz , J. Seeman , Y. K. Semertzidis , K. K. Seth , Q. Shafi , P. Shanahan , R. Sharma , S. R. Sharpe , M. Shiozawa , V. Shiltsev , K. Sigurdson , P. Sikivie , J. Singh , D. Sivers , T. Skwarnicki , N. Smith , J. Sobczyk , H. Sobel , M. Soderberg , Y. H. Song , A. Soni , P. Souder , A. Sousa , J. Spitz , M. Stancari , G. C. Stavenga , J. H. Steffen , S. Stepanyan , D. Stoeckinger , S. Stone , J. Strait , M. Strassler , I. A. Sulai , R. Sundrum , R. Svoboda , B. Szczerbinska , A. Szelc , T. Takeuchi , P. Tanedo , S. Taneja , J. Tang , D. B. Tanner , R. Tayloe , I. Taylor , J. Thomas , C. Thorn , X. Tian , B. G. Tice , M. Tobar , N. Tolich , N. Toro , I. S. Towner , Y. Tsai , R. Tschirhart , C. D. Tunnell , M. Tzanov , A. Upadhye , J. Urheim , S. Vahsen , A. Vainshtein , E. Valencia , R. G. Van de Water , R. S. Van de Water , M. Velasco , J. Vogel , P. Vogel , W. Vogelsang , Y. W. Wah , D. Walker , N. Weiner , A. Weltman , R. Wendell , W. Wester , M. Wetstein , C. White , L. Whitehead , J. Whitmore , E. Widmann , G. Wiedemann , J. Wilkerson , G. Wilkinson , P. Wilson , R. J. Wilson , W. Winter , M. B. Wise , J. Wodin , S. Wojcicki , B. Wojtsekhowski , T. Wongjirad , E. Worcester , J. Wurtele , T. Xin , J. Xu , T. Yamanaka , Y. Yamazaki , I. Yavin , J. Yeck , M. Yeh , M. Yokoyama , J. Yoo , A. Young , E. Zimmerman , K. Zioutas , M. Zisman , J. Zupan , R. Zwaska

Neutrino astronomy is on the verge of discovering new sources, and this will lead to important advances in astrophysics, cosmology, particle physics, and nuclear physics. This paper is meant for non-experts, so that they might better…

Astrophysics · Physics 2007-06-14 John F. Beacom

In recent years precision cosmology has become an increasingly powerful probe of particle physics. Perhaps the prime example of this is the very stringent cosmological upper bound on the neutrino mass. However, other aspects of neutrino…

Cosmology and Nongalactic Astrophysics · Physics 2022-03-02 Steen Hannestad

The electromagnetic properties of neutrinos have attracted considerable attention from researchers for many decades (see [1] for a review). However, until recently, there was no indication in favour of nonzero electromagnetic properties of…

High Energy Physics - Phenomenology · Physics 2021-02-11 Alexander Studenikin

There has been much recent interest in nuclear fission, due in part to a new appreciation of its relevance to astrophysics, stability of superheavy elements, and fundamental theory of neutrino interactions. At the same time, there have been…

The widely accepted description of the present cosmic acceleration and the neutrino oscillations in terms of a cosmological constant and neutrino masses, respectively, seems conceptually not very satisfactory. From a phenomenological…

General Relativity and Quantum Cosmology · Physics 2010-02-05 Javier Indurain

There is a deep connection between cosmology -- the science of the infinitely large --and particle physics -- the science of the infinitely small. This connection is particularly manifest in neutron particle physics. Basic properties of the…

Cosmology and Nongalactic Astrophysics · Physics 2015-09-17 G. Pignol

The past few years have seen dramatic breakthroughs and spectacular and puzzling discoveries in astrophysics and cosmology. In many cases, the new observations can only be explained with the introduction of new fundamental physics. Here we…

High Energy Physics - Phenomenology · Physics 2010-12-09 Daniel S. Akerib , Sean M. Carroll , Marc Kamionkowski , Steven Ritz

Recent experimental results and developments in the theoretical treatment of neutrino-nucleus interactions in the energy range of 1-10 GeV are discussed. Difficulties in extracting neutrino-nucleon cross sections from neutrino-nucleus…

High Energy Physics - Experiment · Physics 2012-10-01 Jorge G. Morfin , Juan Nieves , Jan T. Sobczyk

This presentation reviews recent guiding themes in the broad context of nuclear physics, from developments in chiral effective field theory applied to nuclear systems, via the phases and structures of QCD, to matter under extreme conditions…

Nuclear Theory · Physics 2008-11-26 Wolfram Weise

This review provides an overview of many recent advances in detector technologies for particle physics experiments. Challenges for new technologies include increasing spatial and temporal sensitivity, speed, and radiation hardness while…

Instrumentation and Detectors · Physics 2010-03-16 James E. Brau

The phenomenon of neutrino oscillation has been firmly established: neutrinos change their flavor in their path from their source to observers. This paper is dedicated to the description of experimental results in the oscillation field, of…

High Energy Physics - Experiment · Physics 2009-11-05 U. Dore , D. Orestano

Understanding the properties and physical phase of the dense strongly interacting matter present in the cores of neutron stars or created in their binary mergers remains one of the most prominent open problems in nuclear astrophysics. While…

High Energy Physics - Phenomenology · Physics 2024-05-24 Aleksi Vuorinen

Background induced by neutrons in deep underground laboratories is a critical issue for all experiments looking for rare events, such as dark matter interactions or neutrinoless 2-beta decay. Neutrons can be produced either by natural…

Astrophysics · Physics 2009-06-23 V. A. Kudryavtsev , L. Pandola , V. Tomasello

Neutrino flow is the dominant mechanism of energy transfer in the latest stages of supernovae explosions and in compact stars. The Standard Model of particle physics and accelerator data, provide a satisfactory description of neutrino…

Solar and Stellar Astrophysics · Physics 2012-12-27 Andrea Cipollone
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