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Related papers: Astrophysics with radioactive isotopes

200 papers

Massive stars and their supernovae are prominent sources of radioactive isotopes, the observations of which thus can help to improve our astrophysical models of those. Our understanding of stellar evolution and the final explosive endpoints…

High Energy Astrophysical Phenomena · Physics 2010-08-13 Friedrich-Karl Thielemann , Raphael Hirschi , Matthias Liebendörfer , Roland Diehl

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

Among all nuclear ground-state properties, atomic masses are highly specific for each particular combination of N and Z and the data obtained apply to a variety of physics topics. One of the most crucial questions to be addressed in mass…

Astrophysics · Physics 2008-12-10 Christine Weber , Klaus Blaum , Hendrik Schatz

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

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

I present both a history of radioactivity in astrophysics and an introduction to the major applications of radioactive abundances to astronomy.

Instrumentation and Methods for Astrophysics · Physics 2010-09-13 Donald Clayton

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

Reactions with radioactive nuclear beams at relativistic energies have opened new doors to clarify the mechanisms of stellar evolution and cataclysmic events involving stars and during the big bang epoch. Numerous nuclear reactions of…

Nuclear Theory · Physics 2020-04-22 Thomas Aumann , Carlos A. Bertulani

The book covers the certain questions of nuclear physics and nuclear astrophysics of light atomic nuclei and their processes at low and ultralow energies. Some methods of calculation of nuclear characteristics of the thermonuclear processes…

Nuclear Theory · Physics 2012-01-18 S. B. Dubovichenko

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

Nuclear reactions in stars are difficult to measure directly in the laboratory at the small astrophysical energies. In recent years indirect methods with rare isotopes have been developed and applied to extract low-energy astrophysical…

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

Explosive nuclear burning in astrophysical environments produces unstable nuclei which again can be targets for subsequent reactions. In addition, it involves a large number of stable nuclides which are not fully explored by experiments,…

Nuclear Theory · Physics 2017-08-23 T. Rauscher , C. Froehlich , K. H. Guber

Physics of radioactive nuclear beams is one of the main frontiers of nuclear science today. Experimentally, thanks to technological developments, we are on the verge of invading the territory of extreme N/Z ratios in an unprecedented way.…

Nuclear Theory · Physics 2009-10-30 Jacek Dobaczewski , Witold Nazarewicz

Radioactive nuclei are the key to understanding the circumstances of the birth of our Sun because meteoritic analysis has proven that many of them were present at that time. Their origin, however, has been so far elusive. The ERC-CoG-2016…

We study particle decay as the origin of dark radiation. After elaborating general properties and useful parametrisations we provide model-independent and easy-to-use constraints from nucleosynthesis, the cosmic microwave background and…

High Energy Physics - Phenomenology · Physics 2014-02-14 Jasper Hasenkamp , Jörn Kersten

Radioactive molecules provide a powerful new platform in the search for new physics at energy scales complementary to high-energy particle colliders. By combining enhancements from nuclear properties with the sensitivity and control offered…

Atomic Physics · Physics 2026-05-14 A. Jadbabaie , S. Ebadi , R. F. Garcia Ruiz , N. R. Hutzler , A. M. Jayich , J. T. Singh

The last decades brought an impressive progress in synthesizing and studying properties of nuclides located very far from the beta stability line. Among the most fundamental properties of such exotic nuclides, usually established first, is…

Nuclear Experiment · Physics 2015-06-03 M. Pfützner , L. V. Grigorenko , M. Karny , K. Riisager

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 brief overview of the importance of photodisintegration reactions in astrophysical environments is given and the relevance of photonuclear experiments for nucleosynthesis studies is discussed.

High Energy Astrophysical Phenomena · Physics 2018-09-06 T. Rauscher

A brief summary of some highlights in the study of high energy astrophysical sources over the past decade is presented. It is argued that the great progress that has been made derives largely from the application of new technology to…

Astrophysics · Physics 2007-05-23 R. D. Blandford