English
Related papers

Related papers: An ERC Starting Grant project on p-process nucleos…

200 papers

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

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

Photon-induced reactions play a key role in the nucleosynthesis of rare neutron-deficient p-nuclei. The paper focuses on (gamma,alpha), (gamma,p), and (gamma,n) reactions which define the corresponding p-process path. The relation between…

Nuclear Experiment · Physics 2007-12-31 P. Mohr , Zs. Fulop , H. Utsunomiya

The NURE (NUclear REactions for neutrinoless double beta decay) project has been selected for receiving funding in the call Starting Grant 2016 of European Research Council (ERC). The project, which takes advantage of nuclear physics…

Nuclear Experiment · Physics 2020-01-28 M. Cavallaro

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 cross sections of 151Eu(alpha,gamma)155Tb and 151Eu(alpha,n)154Tb reactions have been measured with the activation method. Some aspects of the measurement are presented here to illustrate the requirements of experimental techniques…

Photon-induced reactions play a key role in the nucleosynthesis of heavy neutron-deficient nuclei, the so-called p-nuclei. In this paper we review the present status of experiments on photon-induced reactions at energies of astrophysical…

Nuclear Experiment · Physics 2009-11-11 H. Utsunomiya , P. Mohr , A. Zilges , M. Rayet

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

I describe in very simple terms the theoretical tools needed to investigate ultra-peripheral nuclear reactions for nuclear astrophysics purposes. For a more detailed account, see arXiv:0908.4307.

Nuclear Theory · Physics 2015-05-14 C. A. Bertulani

The quest to comprehend how nuclear processes influence astrophysical phenomena is driving experimental and theoretical research programs worldwide. One of the main goals in nuclear astrophysics is to understand how energy is generated in…

Nuclear Theory · Physics 2015-05-14 C. A. Bertulani , A. Gade

In this review, we emphasize the interplay between astrophysical observations, modeling, and nuclear physics laboratory experiments. Several important nuclear cross sections for astrophysics have long been identified e.g.…

Nuclear Experiment · Physics 2016-05-26 Alain Coc , Fairouz Hammache , Juergen Kiener

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

I discuss the recent progress in our understanding of nucleosynthesis via rapid neutron capture, the r-process, based on meteoritic data for the early solar system and observations of stars at low metallicities. At present, all data require…

Astrophysics · Physics 2009-10-31 Yong-Zhong Qian

The nucleosynthesis of elements beyond iron is dominated by neutron captures in the s and r processes. However, 32 stable, proton-rich isotopes cannot be formed during those processes, because they are shielded from the s-process flow and…

Instrumentation and Methods for Astrophysics · Physics 2016-01-13 R. Reifarth , S. Altstadt , K. Göbel , T. Heftrich , M. Heil , A. Koloczek , C. Langer , R. Plag , M. Pohl , K. Sonnabend , M. Weigand , T. Adachi , F. Aksouh , J. Al-Khalili , M. AlGarawi , S. AlGhamdi , G. Alkhazov , N. Alkhomashi , H. Alvarez-Pol , R. Alvarez-Rodriguez , V. Andreev , B. Andrei , L. Atar , T. Aumann , V. Avdeichikov , C. Bacri , S. Bagchi , C. Barbieri , S. Beceiro , C. Beck , C. Beinrucker , G. Belier , D. Bemmerer , M. Bendel , J. Benlliure , G. Benzoni , R. Berjillos , D. Bertini , C. Bertulani , S. Bishop , N. Blasi , T. Bloch , Y. Blumenfeld , A. Bonaccorso , K. Boretzky , A. Botvina , A. Boudard , P. Boutachkov , I. Boztosun , A. Bracco , S. Brambilla , J. Briz Monago , M. Caamano , C. Caesar , F. Camera , E. Casarejos , W. Catford , J. Cederkall , B. Cederwall , M. Chartier , A. Chatillon , M. Cherciu , L. Chulkov , P. Coleman-Smith , D. Cortina-Gil , F. Crespi , R. Crespo , J. Cresswell , M. Csatlós , F. Déchery , B. Davids , T. Davinson , V. Derya , P. Detistov , P. Diaz Fernandez , D. DiJulio , S. Dmitry , D. Doré , J. Duenas , E. Dupont , P. Egelhof , I. Egorova , Z. Elekes , J. Enders , J. Endres , S. Ershov , O. Ershova , B. Fernandez-Dominguez , A. Fetisov , E. Fiori , A. Fomichev , M. Fonseca , L. Fraile , M. Freer , J. Friese , M. G. Borge , D. Galaviz Redondo , S. Gannon , U. Garg , I. Gasparic , L. Gasques , B. Gastineau , H. Geissel , R. Gernhäuser , T. Ghosh , M. Gilbert , J. Glorius , P. Golubev , A. Gorshkov , A. Gourishetty , L. Grigorenko , J. Gulyas , M. Haiduc , F. Hammache , M. Harakeh , M. Hass , M. Heine , A. Hennig , A. Henriques , R. Herzberg , M. Holl , A. Ignatov , A. Ignatyuk , S. Ilieva , M. Ivanov , N. Iwasa , B. Jakobsson , H. Johansson , B. Jonson , P. Joshi , A. Junghans , B. Jurado , G. Körner , N. Kalantar , R. Kanungo , A. Kelic-Heil , K. Kezzar , E. Khan , A. Khanzadeev , O. Kiselev , M. Kogimtzis , D. Körper , S. Kräckmann , T. Kröll , R. Krücken , A. Krasznahorkay , J. Kratz , D. Kresan , T. Krings , A. Krumbholz , S. Krupko , R. Kulessa , S. Kumar , N. Kurz , E. Kuzmin , M. Labiche , K. Langanke , I. Lazarus , T. Le Bleis , C. Lederer , A. Lemasson , R. Lemmon , V. Liberati , Y. Litvinov , B. Löher , J. Lopez Herraiz , G. Münzenberg , J. Machado , E. Maev , K. Mahata , D. Mancusi , J. Marganiec , M. Martinez Perez , V. Marusov , D. Mengoni , B. Million , V. Morcelle , O. Moreno , A. Movsesyan , E. Nacher , M. Najafi , T. Nakamura , F. Naqvi , E. Nikolski , T. Nilsson , C. Nociforo , P. Nolan , B. Novatsky , G. Nyman , A. Ornelas , R. Palit , S. Pandit , V. Panin , C. Paradela , V. Parkar , S. Paschalis , P. Pawłowski , A. Perea , J. Pereira , C. Petrache , M. Petri , S. Pickstone , N. Pietralla , S. Pietri , Y. Pivovarov , P. Potlog , A. Prokofiev , G. Rastrepina , T. Rauscher , G. Ribeiro , M. Ricciardi , A. Richter , C. Rigollet , K. Riisager , A. Rios , C. Ritter , T. Rodríguez Frutos , J. Rodriguez Vignote , M. Röder , C. Romig , D. Rossi , P. Roussel-Chomaz , P. Rout , S. Roy , P. Söderström , M. Saha Sarkar , S. Sakuta , M. Salsac , J. Sampson , J. Sanchez del Rio Saez , J. Sanchez Rosado , S. Sanjari , P. Sarriguren , A. Sauerwein , D. Savran , C. Scheidenberger , H. Scheit , S. Schmidt , C. Schmitt , L. Schnorrenberger , P. Schrock , R. Schwengner , D. Seddon , B. Sherrill , A. Shrivastava , S. Sidorchuk , J. Silva , H. Simon , E. Simpson , P. Singh , D. Slobodan , D. Sohler , M. Spieker , D. Stach , E. Stan , M. Stanoiu , S. Stepantsov , P. Stevenson , F. Strieder , L. Stuhl , T. Suda , K. Sümmerer , B. Streicher , J. Taieb , M. Takechi , I. Tanihata , J. Taylor , O. Tengblad , G. Ter-Akopian , S. Terashima , P. Teubig , R. Thies , M. Thoennessen , T. Thomas , J. Thornhill , G. Thungstrom , J. Timar , Y. Togano , U. Tomohiro , T. Tornyi , J. Tostevin , C. Townsley , W. Trautmann , T. Trivedi , S. Typel , E. Uberseder , J. Udias , T. Uesaka , L. Uvarov , Z. Vajta , P. Velho , V. Vikhrov , M. Volknandt , V. Volkov , P. von Neumann-Cosel , M. von Schmid , A. Wagner , F. Wamers , H. Weick , D. Wells , L. Westerberg , O. Wieland , M. Wiescher , C. Wimmer , K. Wimmer , J. S. Winfield , M. Winkel , P. Woods , R. Wyss , D. Yakorev , M. Yavor , J. Zamora Cardona , I. Zartova , T. Zerguerras , I. Zgura , A. Zhdanov , M. Zhukov , M. Zieblinski , A. Zilges , K. Zuber

The origin of the elements is a fascinating question that scientists have been trying to answer for the last seven decades. The formation of light elements in the primordial universe and heavier elements in astrophysical sources occurs…

Solar and Stellar Astrophysics · Physics 2019-01-30 V. Liccardo , M. Malheiro , M. S. Hussein , B. V. Carlson , T. Frederico

Nucleosynthesis beyond Fe poses additional challenges not encountered when studying astrophysical processes involving light nuclei. Astrophysical sites and conditions are not well known for some of the processes involved. On the nuclear…

Solar and Stellar Astrophysics · Physics 2014-03-12 T. Rauscher

In the model calculations of heavy element nucleosynthesis processes the nuclear reaction rates are taken from statistical model calculations which utilize various nuclear input parameters. It is found that in the case of reactions…

Nuclear Experiment · Physics 2014-12-01 Gy. Gyürky , Zs. Fülöp , Z. Halász , G. G. Kiss , T. Szücs

This is an exciting time for the study of r-process nucleosynthesis. Recently, a neutron star merger GW170817 was observed in extraordinary detail with gravitational waves and electromagnetic radiation from radio to gamma rays. The very red…

We show that a minimum-mass neutron star undergoes delayed explosion after mass removal from its surface. We couple the Newtonian hydrodynamics to a nuclear reaction network of $\sim4500$ isotopes to study the nucleosynthesis and neutrino…

High Energy Astrophysical Phenomena · Physics 2025-11-10 Chun-Ming Yip , Ming-Chung Chu , Shing-Chi Leung , Lap-Ming Lin

We present a new nucleosynthesis process that may take place on neutron-rich ejecta experiencing an intensive neutrino flux. The nucleosynthesis proceeds similarly to the standard $r$-process, a sequence of neutron-captures and beta-decays,…

High Energy Astrophysical Phenomena · Physics 2024-05-14 Zewei Xiong , Gabriel Martínez-Pinedo , Oliver Just , Andre Sieverding
‹ Prev 1 2 3 10 Next ›