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The rapid neutron capture process (r process) is believed to be responsible for about half of the production of the elements heavier than iron and contributes to abundances of some lighter nuclides as well. A universal pattern of r-process…

High Energy Astrophysical Phenomena · Physics 2019-06-26 T. Kajino , W. Aoki , A. B. Balantekin , R. Diehl , M. A. Famiano , G. J. Mathews

The astrophysical rapid neutron capture process or `$r$ process' of nucleosynthesis is believed to be responsible for the production of approximately half the heavy element abundances found in nature. This multifaceted problem remains one…

Nuclear Theory · Physics 2016-01-20 M. R. Mumpower , R. Surman , G. C. McLaughlin , A. Aprahamian

Nuclear astrophysics aims at unraveling the cosmic origins of chemical elements and the physical processes powering stars. It constitutes a truly multidisciplinary field, that integrates tools, advancements, and accomplishments from…

Solar and Stellar Astrophysics · Physics 2026-01-23 Jordi Jose

For the better part of a century the field of nuclear astrophysics has aimed to answer fundamental questions about nature, such as the origin of the elements and the behavior of high-density, low-temperature matter. Sustained and concerted…

Nuclear Experiment · Physics 2016-10-06 Zach Meisel

Neutrino-driven winds following core collapse supernovae have been proposed as a suitable site where the so-called light heavy elements (between Sr to Ag) can be synthetized. For moderately neutron-rich winds, ($\alpha,n$) reactions play a…

Solar and Stellar Astrophysics · Physics 2020-12-09 Jorge Pereira , Almudena Arcones , Julia Bliss , Fernando Montes

The quest for the origin of matter in the Universe had been the subject of philosophical and theological debates over the history of mankind, but quantitative answers could be found only by the scientific achievements of the last century. A…

Instrumentation and Methods for Astrophysics · Physics 2014-03-25 R. Reifarth , C. Lederer , F. Käppeler

A small number of naturally occurring, proton-rich nuclides (the p-nuclei) cannot be made in the s- and r-process. Their origin is not well understood. Massive stars can produce p-nuclei through photodisintegration of pre-existing…

Solar and Stellar Astrophysics · Physics 2013-05-14 T. Rauscher , N. Dauphas , I. Dillmann , C. Fröhlich , Zs. Fülöp , Gy. Gyürky

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

The existence of neutron star mergers has been supported since the discovery of the binary pulsar and the observation of its orbital energy loss, consistent with General Relativity. They are considered nucleosynthesis sites of the rapid…

High Energy Astrophysical Phenomena · Physics 2017-10-09 F. -K. Thielemann , M. Eichler , I. V. Panov , B. Wehmeyer

Radioactivity was discovered as a by-product of searching for elements with suitable chemical properties. Understanding its characteristics led to the development of nuclear physics, understanding that unstable configurations of nucleons…

High Energy Astrophysical Phenomena · Physics 2018-11-28 Roland Diehl

Nuclear reactions generate energy in nuclear reactors, in stars, and are responsible for the existence of all elements heavier than hydrogen in the universe. Nuclear reactions denote reactions between nuclei, and between nuclei and other…

Nuclear Theory · Physics 2010-07-15 C. A. Bertulani

Nuclear masses play a fundamental role in understanding how the heaviest elements in the Universe are created in the $r$-process. We predict $r$-process nucleosynthesis yields using neutron capture and photodissociation rates that are based…

Nuclear Theory · Physics 2016-03-30 Dirk Martin , Almudena Arcones , Witold Nazarewicz , Erik Olsen

Nuclear astrophysics is an interdisciplinary research field of nuclear physics and astrophysics, seeking for the answer to a question, how to understand the evolution of the Universe with the nuclear processes which we learn. We review the…

After a successful core-collapse supernova, a neutrino-driven wind develops where it is possible to synthesize lighter heavy elements ($30<Z<45$). In the early galaxy, the origin of these elements is associated to the r-process and to an…

Solar and Stellar Astrophysics · Physics 2017-04-05 Julia Bliss , Almudena Arcones , Fernando Montes , Jorge Pereira

A long-standing scientific puzzle has been to explain the origin of the heaviest elements in the Universe and, more particularly, the production of the elements heavier than iron up to uranium. The rapid neutron capture process (or…

High Energy Astrophysical Phenomena · Physics 2023-03-14 Ina K. B. Kullmann

This review focuses on nuclear reactions in astrophysics and, more specifically, on reactions with light ions (nucleons and alpha particles) proceeding via the strong interaction. It is intended to present the basic definitions essential…

Nuclear Theory · Physics 2015-03-17 T. Rauscher

Neutrino-driven ejecta in core collapse supernovae (CCSNe) offer an interesting astrophysical scenario where lighter heavy elements between Sr and Ag can be synthesized. Previous studies emphasized the important role that ($\alpha,n$)…

Nuclear Experiment · Physics 2020-06-10 J. Bliss , A. Arcones , F. Montes , J. Pereira

Nuclear astrophysics is a multi-disciplinary field with a huge demand for nuclear data. Among its various fields, stellar evolution and nucleosynthesis are clearly the most closely related to nuclear physics. The need for nuclear data for…

Nuclear Theory · Physics 2022-12-06 S. Goriely , A. Choplin , W. Ryssens , I. Kullmann

Neutrinos produced during a supernova explosion induce reactions on abundant nuclei in the outer stellar shells and contribute in this way to the synthesis of the elements in the Universe. This neutrino nucleosynthesis process has been…

High Energy Astrophysical Phenomena · Physics 2019-06-25 Karlheinz Langanke , Gabriel Martinez-Pinedo , Andre Sieverding

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