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Star formation involves the flow of gas and dust within molecular clouds into protostars and young stellar objects (YSOs) due to gravity. Along the way, these flows are shaped significantly by many other mechanisms, including pressure,…

Starting from the early works by Weizsaecker and Bethe about fusion cycles and energy conversion in stars, a brief survey of thermonuclear processes in stars leading to contemporary research problems in this field is given. Special emphasis…

Astrophysics · Physics 2007-05-23 G. Wolschin

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

The first phase of stellar evolution in the history of the universe may be Dark Stars, powered by dark matter heating rather than by fusion. Weakly interacting massive particles, which are their own antiparticles, can annihilate and provide…

Cosmology and Nongalactic Astrophysics · Physics 2010-02-17 Paolo Gondolo , Katherine Freese , Douglas Spolyar , Anthony Aguirre , Peter Bodenheimer , Jeremy A. Sellwood , Naoki Yoshida

Neutron stars offer powerful astrophysical laboratories to probe the properties of dark matter. Gradual accumulation of heavy, non-annihilating dark matter in neutron stars can lead to the formation of comparable-mass black holes, and…

High Energy Physics - Phenomenology · Physics 2025-04-23 Anupam Ray

We discuss different exotic phases and components of matter from the crust to the core of neutron stars based on theoretical models for equations of state relevant to core collapse supernova simulations and neutron star merger. Parameters…

High Energy Astrophysical Phenomena · Physics 2017-09-27 Debades Bandyopadhyay

The prediction of neutron stars properties is strictly connected to the employed nuclear interactions. The appearance of hyperons in the inner core of the star is strongly dependent on the details of the underlying hypernuclear force. We…

Nuclear Theory · Physics 2018-07-20 Diego Lonardoni , Alessandro Lovato , Stefano Gandolfi , Francesco Pederiva

The first phase of stellar evolution in the history of the universe may be Dark Stars, powered by dark matter heating rather than by fusion. Weakly interacting massive particles, which are their own antiparticles, can annihilate and provide…

The neutrino is the most elusive particle that we know and for many years physicists doubted that neutrinos might never be revealed. Today we know and we reveal neutrinos produced by different astrophysical objects and by interactions of…

History and Philosophy of Physics · Physics 2016-09-23 Maurizio Spurio

During this last decade our knowledge of the evolutionary properties of stars has significantly improved. This result has been achieved thanks to our improved understanding of the physical behavior of stellar matter in the thermal regimes…

Solar and Stellar Astrophysics · Physics 2015-05-14 Santi Cassisi

Star formation is a multi-scale, multi-physics problem ranging from the size scale of molecular clouds ($\sim$10s pc) down to the size scales of dense prestellar cores ($\sim$0.1 pc) that are the birth sites of stars. Several physical…

Solar and Stellar Astrophysics · Physics 2020-05-27 Anna L. Rosen , Stella S. R. Offner , Sarah I. Sadavoy , Asmita Bhandare , Enrique Vázquez-Semadeni , Adam Ginsburg

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

As the Stars and Stellar Evolution (SSE) panel is fully aware, the next decade will see major advances in our understanding of these areas of research. To quote from their charge, these advances will occur in studies of the Sun as a star,…

Instrumentation and Methods for Astrophysics · Physics 2012-08-27 AAS WGLA , : , Nancy Brickhouse , John Cowan , Paul Drake , Steven Federman , Gary Ferland , Adam Frank , Eric Herbst , Keith Olive , Farid Salama , Daniel Wolf Savin , Lucy Ziurys

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

An emerging theme in modern astrophysics is the connection between astronomical observations and the underlying physical phenomena that drive our cosmos. Both the mechanisms responsible for the observed astrophysical phenomena and the tools…

The presence of dark matter has been ascertained through a wealth of astrophysical and cosmological phenomena and its nature is a central puzzle in modern science. Elementary particles stand as the most compelling explanation. They have…

High Energy Physics - Phenomenology · Physics 2019-10-02 Daniel A. Camargo , Farinaldo S. Queiroz , Riccardo Sturani

Underground laboratories provide the low radioactive background environment necessary to explore the highest energy scales that cannot be reached with accelerators, by searching for extremely rare phenomena. I have requested to the…

High Energy Physics - Experiment · Physics 2007-12-10 Alessandro Bettini

A mechanism of creation of stellar-like objects in the very early universe, from the QCD phase transition till BBN and somewhat later, is studied. It is argued that in the considered process primordial black holes with masses above a few…

Cosmology and Nongalactic Astrophysics · Physics 2014-01-15 A. D. Dolgov , S. I. Blinnikov

In the past four decades a new type of astronomy has emerged, where instead of looking up into the sky "telescopes" are buried miles underground or deep under water or ice and search not for photons (that is, light), but rather for…

Astrophysics · Physics 2008-11-26 E. Waxman

While ALMA and JWST are revolutionizing our view of star and planet formation with their unprecedented sensitivity and resolution at submillimeter and near-IR wavelengths, many outstanding questions can only be answered with observations in…

Instrumentation and Methods for Astrophysics · Physics 2023-03-15 Floris van der Tak
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