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The stellar astronomy has always been considered the fundamental source of knowledge about the basic building blocks of the universe - the stars. It has proved correctness of many physical theories - like e.g. the idea of nuclear fusion in…

Instrumentation and Methods for Astrophysics · Physics 2011-12-20 Petr Škoda

Astrophysics is gaining increased attention from the particle and nuclear physics communities, as budget cuts, delays, and cancellations limit opportunities for breakthrough research at accelerator laboratories. Observations of cosmic rays…

Astrophysics · Physics 2009-10-22 R. Jeffrey Wilkes

Nuclear astrophysics, the union of nuclear physics and astronomy, went through an impressive expansion during the last twenty years. This could be achieved thanks to milestone improvements in astronomical observations, cross section…

Nuclear Astrophysics is a field at the intersection of nuclear physics and astrophysics, which seeks to understand the nuclear engines of astronomical objects and the origin of the chemical elements. This white paper summarizes progress and…

Nuclear Experiment · Physics 2022-11-30 H. Schatz , A. D. Becerril Reyes , A. Best , E. F. Brown , K. Chatziioannou , K. A. Chipps , C. M. Deibel , R. Ezzeddine , D. K. Galloway , C. J. Hansen , F. Herwig , A. P. Ji , M. Lugaro , Z. Meisel , D. Norman , J. S. Read , L. F. Roberts , A. Spyrou , I. Tews , F. X. Timmes , C. Travaglio , N. Vassh , C. Abia , P. Adsley , S. Agarwal , M. Aliotta , W. Aoki , A. Arcones , A. Aryan , A. Bandyopadhyay , A. Banu , D. W. Bardayan , J. Barnes , A. Bauswein , T. C. Beers , J. Bishop , T. Boztepe , B. Côté , M. E. Caplan , A. E. Champagne , J. A. Clark , M. Couder , A. Couture , S. E. de Mink , S. Debnath , R. J. deBoer , J. den Hartogh , P. Denissenkov , V. Dexheimer , I. Dillmann , J. E. Escher , M. A. Famiano , R. Farmer , R. Fisher , C. Fröhlich , A. Frebel , C. Fryer , G. Fuller , A. K. Ganguly , S. Ghosh , B. K. Gibson , T. Gorda , K. N. Gourgouliatos , V. Graber , M. Gupta , W. Haxton , A. Heger , W. R. Hix , W C. G. Ho , E. M. Holmbeck , A. A. Hood , S. Huth , G. Imbriani , R. G. Izzard , R. Jain , H. Jayatissa , Z. Johnston , T. Kajino , A. Kankainen , G. G. Kiss , A. Kwiatkowski , M. La Cognata , A. M. Laird , L. Lamia , P. Landry , E. Laplace , K. D. Launey , D. Leahy , G. Leckenby , A. Lennarz , B. Longfellow , A. E. Lovell , W. G. Lynch , S. M. Lyons , K. Maeda , E. Masha , C. Matei , J. Merc , B. Messer , F. Montes , A. Mukherjee , M. Mumpower , D. Neto , B. Nevins , W. G. Newton , L. Q. Nguyen , K. Nishikawa , N. Nishimura , F. M. Nunes , E. O'Connor , B. W. O'Shea , W-J. Ong , S. D. Pain , M. A. Pajkos , M. Pignatari , R. G. Pizzone , V. M. Placco , T. Plewa , B. Pritychenko , A. Psaltis , D. Puentes , Y-Z. Qian , D. Radice , D. Rapagnani , B. M. Rebeiro , R. Reifarth , A. L. Richard , N. Rijal , I. U. Roederer , J. S. Rojo , J. S K , Y. Saito , A. Schwenk , M. L. Sergi , R. S. Sidhu , A. Simon , T. Sivarani , Á. Skúladóttir , M. S. Smith , A. Spiridon , T. M. Sprouse , S. Starrfield , A. W. Steiner , F. Strieder , I. Sultana , R. Surman , T. Szücs , A. Tawfik , F. Thielemann , L. Trache , R. Trappitsch , M. B. Tsang , A. Tumino , S. Upadhyayula , J. O. Valle Martínez , M. Van der Swaelmen , C. Viscasillas Vázquez , A. Watts , B. Wehmeyer , M. Wiescher , C. Wrede , J. Yoon , R G. T. Zegers , M. A. Zermane , M. Zingale

Solar neutrinos have been the subject of experimental study for almost half a century. The initial aim was '...to see into the interior of a star and thus verify directly the hypothesis of nuclear energy generation in stars'. Since then the…

High Energy Physics - Experiment · Physics 2015-04-17 Jeanne R. Wilson

Some of the means through which the possible presence of nearly deconfined quarks in neutron stars can be detected by astrophysical observations of neutron stars from their birth to old age are highlighted.

Astrophysics · Physics 2009-06-23 M Prakash

Supernovae are the most powerful cosmic sources of MeV neutrinos. These elementary particles play a crucial role when the evolution of a massive star is terminated by the collapse of its core to a neutron star or a black hole and the star…

High Energy Astrophysical Phenomena · Physics 2018-04-25 H. -Th. Janka

Neutron stars are fascinating astrophysical objects immersed in strong gravitational and electromagnetic fields, at the edge of our current theories. These stars manifest themselves mostly as pulsars, emitting a timely very stable and…

High Energy Astrophysical Phenomena · Physics 2016-09-28 J. Pétri

The most energetic neutron stars, powered by their rotation, are capable of producing pulsed radiation from the radio up to gamma rays with nearly TeV energies. These pulsars are part of the universe of energetic and powerful particle…

High Energy Astrophysical Phenomena · Physics 2015-09-30 Isabelle A. Grenier , Alice K. Harding

Our current knowledge of neutron star formation, progenitors, and natal masses, spins, magnetic fields, and space velocities is briefly reviewed from a theorist's perspective. More observational information is badly needed to constrain…

Astrophysics · Physics 2007-05-23 Hans-Thomas Janka

Neutron stars, the compact stellar remnants of core-collapse supernova explosions, are unique cosmic laboratories for exploring novel phases of matter under extreme conditions. In particular, the occurrence of superfluidity and…

High Energy Astrophysical Phenomena · Physics 2017-09-22 N. Chamel

Neutrinos are produced by a variety of sources that comprise our Sun, explosive environments such as core-collapse supernovae, the Earth and the Early Universe. The precise origin of the recently discovered ultra-high energy neutrinos is to…

High Energy Physics - Phenomenology · Physics 2014-11-25 Cristina Volpe

We discuss selected topics in the field of particle- and astrophysics with neutrons. They have a direct link with our understanding of the history of the Universe and are related to recent, ongoing or future measurements. They deal with the…

High Energy Physics - Experiment · Physics 2012-05-14 Stephan Paul

Neutron stars are excellent emitters of gravitational waves. Squeezing matter beyond nuclear densities invites exotic physical processes, many of which violently transfer large amounts of mass at relativistic velocities, disrupting…

High Energy Astrophysical Phenomena · Physics 2015-11-20 Paul D. Lasky

Selected topics in neutrino astrophysics are reviewed. These include the production of low energy neutrino flux from cores of collapsing stars and the expected high energy neutrino flux from some other astrophysical sites such as the…

High Energy Physics - Phenomenology · Physics 2007-05-23 H. Athar

The masses and radii of neutron stars are discussed in general relativity and scalar-tensor theory of gravity and the differences are compared with the current uncertainties stemming from the nuclear equation of state in the relativistic…

General Relativity and Quantum Cosmology · Physics 2019-07-16 F. J. Fattoyev

(transcript of a talk given by Prof.~Feshbach:) Nuclear physics has been and will be a major factor in science and technology. It makes unique and important contributions to medicine, to industry and to other sciences. Interaction with…

Nuclear Theory · Physics 2009-09-25 Herman Feshbach

Astrophysics and cosmology can be used to test the standard model of particle physics under conditions and over distance and time scales not accessible to laboratory experiments. Most of the astrophysical observations are in good agreement…

High Energy Physics - Phenomenology · Physics 2016-09-01 Arnon Dar

Formed in the aftermath of gravitational core-collapse supernova explosions, neutron stars are unique cosmic laboratories for probing the properties of matter under extreme conditions that cannot be reproduced in terrestrial laboratories.…

Nuclear Theory · Physics 2019-03-06 David Blaschke , Nicolas Chamel

Recent observations of neutron star masses close to the maximum predicted by nucleonic equations of state begin to challenge our understanding of dense matter in neutron stars, and constrain the possible presence of quark matter in their…

Nuclear Theory · Physics 2008-11-26 Gordon Baym
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