Zobrazeno 1 - 10
of 244
pro vyhledávání: '"Rauscher Thomas"'
Autor:
Rizzuti, Federico, Hirschi, Raphael, Varma, Vishnu, Arnett, William David, Georgy, Cyril, Meakin, Casey, Mocák, Miroslav, Murphy, Alexander St. John, Rauscher, Thomas
One-dimensional (1D) stellar evolution models are widely used across various astrophysical fields, however they are still dominated by important uncertainties that deeply affect their predictive power. Among those, the merging of independent convecti
Externí odkaz:
http://arxiv.org/abs/2407.15544
Autor:
Michalopoulou Veatriki, Diakaki Maria, Vlastou Rosa, Kokkoris Michael, Stamatopoulos Athanasios, Tsinganis Andrea, Eleme Zinovia, Patronis Nikolas, Heyse Jan, Schillebeeckx Peter, Tassan-Got Laurent, Barbagallo Massimo, Colonna Nicola, Urlass Sebastian, Macina Daniela, Chiaveri Enrico, Aberle Oliver, Alcayne Victor, Amaducci Simone, Andrzejewski Józef, Audouin Laurent, Babiano-Suarez Victor, Bacak Michael, Bennett Samuel, Berthoumieux Eric, Billowes Jon, Bosnar Damir, Brown Adam, Busso Maurizio, Caamaño Manuel, Caballero-Ontanaya Luis, Calviño Francisco, Calviani Marco, Cano-Ott Daniel, Casanovas Adria, Cerutti Francesco, Cortés Guillem, Cortés-Giraldo Miguel, Cosentino Luigi, Cristallo Sergio, Damone Lucia-Anna, Davies Paul-John, Dietz Mirco, Domingo-Pardo César, Dressler Rugard, Ducasse Quentin, Dupont Emmeric, Durán Ignacio, Fernández-Domínguez Beatriz, Ferrari Alfredo, Finocchiaro Paolo, Göbel Kathrin, Garg Ruchi, Gawlik-Ramięga Aleksandra, Gilardoni Simone, Gonçalves Isabel, González-Romero Enrique, Guerrero Carlos, Gunsing Frank, Harada Hideo, Heinitz Stephan, Jenkins David, Junghans Arnd, Käppeler† Franz, Kadi Yacine, Kimura Atsushi, Knapová Ingrid, Krtička Milan, Kurtulgil Deniz, Ladarescu Ion, Lederer-Woods Claudia, Leeb Helmut, Lerendegui-Marco Jorge, Lonsdale Sarah-Jane, Manna Alice, Martínez Trinitario, Masi Alessandro, Massimi Cristian, Mastinu Pierfrancesco, Mastromarco Mario, Maugeri Emilio-Andrea, Mazzone Annamaria, Mendoza Emilio, Mengoni Alberto, Milazzo Paolo, Mingrone Federica, Moreno-Soto Javier, Musumarra Agatino, Negret Alexandru, Nolte Ralf, Ogállar Francisco, Oprea Andreea, Pavlik Andreas, Perkowski Jarosław, Piersanti Luciano, Petrone Cristina, Pirovano Elisa, Porras Ignacio, Praena Javier, Quesada José-Manuel, Ramos-Doval Diego, Rauscher Thomas, Reifarth René, Rochman Dimitri, Rubbia Carlo, Sabaté-Gilarte Marta, Saxena Alok, Schumann Dorothea, Sekhar Adhitya, Smith Gavin, Sosnin Nikolay, Sprung Peter, Tagliente Giuseppe, Tain José, Tarifeño-Saldivia Ariel, Thomas Benedikt, Torres-Sánchez Pablo, Ulrich Jiri, Valenta Stanislav, Vannini Gianni, Variale Vincenzo, Vaz Pedro, Ventura Alberto, Vescovi Diego, Vlachoudis Vasilis, Wallner Anton, Woods Philip-John, Wright Tobias, Žugec Petar
Publikováno v:
EPJ Web of Conferences, Vol 284, p 01030 (2023)
Neutron cross section measurements are often made relative to a neutron cross section standard. Thus, the accuracy of the neutron standards determines the best possible accuracy of the neutron measurements. The 235U(n,f) cross section is widely used
Externí odkaz:
https://doaj.org/article/5f59104300154ae68199dc8b36867a38
Autor:
Angus Cameron, Williams Matthew, Andreyev Andrei, Bhattacharjee Soumendu, Buck Samantha, Chakraborty Soham, Davids Barry, Diget Christian, Garnsworthy Adam, Griffin Chris, Fernandez Asunción, Hackman Greg, Hudson Kevan, Hufschmidt Dirk, Karayonchev Vasil, Kim Yong, Laird Alison, Lennarz Annika, Mashtakov Konstantin, Machule Peter, Natzke Connor, Pak Kihong, Psaltis Athanasios, Radich Allison, Rauscher Thomas, Rhodes Daniel, Sauvage Thierry, Simon Anna, Svensson Carl, Upadhyayula Sriteja, Williams Jonathan, Yates Daniel, Zidar Tammy
Publikováno v:
EPJ Web of Conferences, Vol 279, p 11003 (2023)
The r-process has been shown to be robust in reproducing the abundance distributions of heavy elements, such as europium, seen in ultra-metal poor stars. In contrast, observations of elements 26 < Z < 47 display overabundances relative to r-process m
Externí odkaz:
https://doaj.org/article/58e2332026c24651b095ac5e860f8402
Publikováno v:
Handbook of Nuclear Physics 2023
This chapter will go through the important nuclear reactions in stellar evolution and explosions, passing through the individual stellar burning stages and also explosive burning conditions. To follow the changes in the composition of nuclear abundan
Externí odkaz:
http://arxiv.org/abs/2307.14391
Autor:
Carenza, Pierluca, Co', Giampaolo, Giannotti, Maurizio, Lella, Alessandro, Lucente, Giuseppe, Mirizzi, Alessandro, Rauscher, Thomas
Publikováno v:
Phys. Rev. C 109, 015501 (2024)
Axions coupled to nucleons might be copiously emitted from core-collapse supernovae (SNe). If the axion-nucleon coupling is strong enough, axions would be emitted from the SN as a burst and, reaching Earth, may excite the oxygen nuclei in water Chere
Externí odkaz:
http://arxiv.org/abs/2306.17055
Autor:
Lella, Alessandro, Carenza, Pierluca, Co', Giampaolo, Lucente, Giuseppe, Giannotti, Maurizio, Mirizzi, Alessandro, Rauscher, Thomas
Publikováno v:
Phys. Rev. D 109, 023001 (2024)
Axion-like particles (ALPs) coupled to nucleons might be copiously emitted from a supernova (SN) core. We extend existing bounds on free-streaming ALPs to the case in which these are so strongly-interacting with the nuclear matter to be trapped in th
Externí odkaz:
http://arxiv.org/abs/2306.01048
Autor:
Rauscher, Thomas
Publikováno v:
Eur. Phys. J. A 58 (2022) 214
The determination of astrophysical reaction rates requires different approaches depending on the conditions in hydrostatic and explosive burning. The focus here is on astrophysical reaction rates for radiative neutron capture reactions. Relevant nucl
Externí odkaz:
http://arxiv.org/abs/2209.11480
Autor:
Battino, Umberto, Pignatari, Marco, Travaglio, Claudia, Lederer-Woods, Claudia, Denissenkov, Pavel, Herwig, Falk, Thielemann, Friedrich-Karl, Rauscher, Thomas
The origin of the proton-rich trans-iron isotopes in the solar system is still uncertain. Single-degenerate thermonuclear supernovae (SNIa) with n-capture nucleosynthesis seeds assembled in the external layers of the progenitor's rapidly accreting wh
Externí odkaz:
http://arxiv.org/abs/2007.13677