Results 161 to 170 of about 66,893 (303)

Explosive Nucleosynthesis: What we learned and what we still do not understand

, 2018
This review touches on historical aspects, going back to the early days of nuclear astrophysics, initiated by B$^2$FH and Cameron, discusses (i) the required nuclear input from reaction rates and decay properties up to the nuclear equation of state ...
A Arcones, A Burrows, A Burrows, A Heger, A Khokhlov, A Perego, A Sobiczewski, AB McDonald, AGW Cameron, AGW Cameron, AL Sallaska, B Côté, B Paxton, B Wehmeyer, BS Meyer, C Angulo, C Georgy, C Iliadis, C Kobayashi, C Li, C Sneden, C Winteler, D Argast, D Bodansky, D Eichler, D Maoz, DA Goldstein, E Müller, EM Burbidge, F Hoyle, F Käppeler, F Matteucci, F Voort van de, F-K Thielemann, F-K Thielemann, F-K Thielemann, F-K Thielemann, FX Timmes, FX Timmes, G Cescutti, G Halevi, G Martínez-Pinedo, G Michaud, G Michaud, GM Fuller, GR Caughlan, H-T Janka, H-T Janka, HA Bethe, I Dillmann, I Iben Jr, I Iben Jr, I Petermann, IU Roederer, IV Panov, J Lippuner, J Pruet, JA Holmes, JA Morgan, JC Wheeler, JJ Cowan, JM Lattimer, JW Truran, JW Truran, JW Truran, JW Truran, JW Truran, K Farouqi, K Langanke, K Nakamura, K Nomoto, K Nomoto, K Nomoto, K Nomoto, K Nomoto, K Takahashi, K-C Pan, K-L Kratz, LF Roberts, M Arnould, M Arnould, M Arnould, M Arnould, M Eichler, M Limongi, M Oertel, M Ruffert, M Ugliano, M Zingale, MB Davies, N Nishimura, N Nishimura, P Hoeflich, P Möller, P Mösta, P Mösta, R Longland, RF Webbink, RH Cyburt, RJ deBoer, RM Cabezón, S Goriely, S Goriely, S Nishimura, S Rosswog, S Shen, S Wanajo, S-C Leung, S-I Fujimoto, SE Woosley, SE Woosley, SE Woosley, SE Woosley, SE Woosley, T Ertl, T Foglizzo, T Kuroda, T Marketin, T Mishenina, T Rauscher, T Rauscher, T Rauscher, T Sukhbold, T Tsujimoto, T Yoshida, TA Weaver, TT Hansen, UM Noebauer, WA Fowler, WA Fowler, WA Fowler, WD Arnett, WD Arnett, WD Arnett, WD Arnett, WD Arnett, WM Howard, WR Hix, Y Hirai, Y Xu, ZY Bao, ZY Bao   +141 more
core   +1 more source

Big Bang Nucleosynthesis constraints on Barrow entropy [PDF]

Physics Letters B, 2020
J. Barrow, S. Basilakos, E. Saridakis
semanticscholar   +1 more source

Production of Lithium and Heavy Elements in AGB Stars Experiencing PIEs

Galaxies
Asymptotic giant branch (AGB) stars can experience proton ingestion events (PIEs), leading to a rich nucleosynthesis. During a PIE, the intermediate neutron capture process (i-process) develops, leading to the production of trans-iron elements.
Arthur Choplin, Lionel Siess, Stephane Goriely, Sebastien Martinet   +3 more
doaj   +1 more source

Nucleosynthesis Around Black Holes [PDF]

, 1999
Study of nucleosynthesis in accretion disks around black holes was initiated by Chakrabarti et al. (1987). In the present work we do the similar analysis using the state-of-the-art disk model, namely, Advective Accretion Disks.
Mukhopadhyay, Banibrata
core   +1 more source

Quark-hadron phase transition in the early Universe: Isothermal baryon-number fluctuations and primordial nucleosynthesis [PDF]

, 1988
G. M. Fuller, G. J. Mathews, C. R. Alcock   +2 more
openalex   +1 more source

Explosive Nucleosynthesis

, 2022
Cosmic nucleosynthesis had been one of INTEGRAL’s major science targets. The SPI spectrometer delivered important measurements, both from targets of opportunity in the form of stellar explosions and their shortlived radionuclides, and from cumulative emission of long-lived radioactive isotopes. We review the lessons learned on explosive nucleosynthesis
openaire   +1 more source

Machine learning opportunities for nucleosynthesis studies

Frontiers in Astronomy and Space Sciences
Nuclear astrophysics is an interdisciplinary field focused on exploring the impact of nuclear physics on the evolution and explosions of stars and the cosmic creation of the elements.
Michael S. Smith, Dan Lu
doaj   +1 more source

Constraints on Tsallis Cosmology from Big Bang Nucleosynthesis and the Relic Abundance of Cold Dark Matter Particles. [PDF]

Entropy (Basel), 2023
Jizba P, Lambiase G.
europepmc   +1 more source

Direct and Indirect Measurements of the ¹⁹F(p,α)¹⁶O Reaction at Astrophysical Energies Using the LHASA Detector and the Trojan Horse Method

Universe
Fluorine is one of the most interesting elements in nuclear astrophysics. Its abundance can provide important hints to constrain the stellar models since fluorine production and destruction are strictly connected to the physical conditions inside the ...
Giovanni L. Guardo, Giuseppe G. Rapisarda, Dimiter L. Balabanski, Giuseppe D’Agata, Alessia Di Pietro, Pierpaolo Figuera, Marco La Cognata, Marco La Commara, Livio Lamia, Dario Lattuada, Catalin Matei, Marco Mazzocco, Alessandro A. Oliva, Sara Palmerini, Teodora Petruse, Rosario G. Pizzone, Stefano Romano, Maria Letizia Sergi, Roberta Spartá, Xuedou Su, Aurora Tumino, Nikola Vukman   +21 more
doaj   +1 more source

On relative supernova rates and nucleosynthesis roles [PDF]

, 1989
W. David Arnett, David N. Schramm, James W. Truran   +2 more
openalex   +1 more source