Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Avila, Melina L."'
Publikováno v:
Phys. Rev. C 109, L061601 (2024)
Indirect methods have become the predominant approach in experimental nuclear astrophysics for studying several low-energy nuclear reactions occurring in stars, as direct measurements of many of these relevant reactions are rendered infeasible due to
Externí odkaz:
http://arxiv.org/abs/2307.05636
Autor:
Raghavan, Krishnan, Avila, Melina L., Balaprakash, Prasanna, Jayatissa, Heshani, Santiago-Gonzalez, Daniel
The Multi-Sampling Ionization Chamber (MUSIC) detector is typically used to measure nuclear reaction cross sections relevant for nuclear astrophysics, fusion studies, and other applications. From the MUSIC data produced in one experiment scientists c
Externí odkaz:
http://arxiv.org/abs/2204.03137
Autor:
Psaltis Athanasios, Arcones Almudena, Avila Melina L., Jacobi Maximilian, Hansen Camilla Juul, Lombardo Linda, Meisel Zach, Mohr Peter, Montes Fernando, Ong Wei Jia, Schatz Hendrik
Publikováno v:
EPJ Web of Conferences, Vol 279, p 08002 (2023)
The lighter heavy elements of the first r-process peak, between strontium and silver, can be synthesized in the moderately neutron-rich neutrino–driven ejecta of either core–collapse supernovae or neutron star mergers via the weak r–process. Th
Externí odkaz:
https://doaj.org/article/d6f978bb6f354d339aff04d73a9f3bd6
Autor:
Psaltis Athanasios, Arcones Almudena, Avila Melina L., Jacobi Maximillian, Meisel Zach, Mohr Peter, Montes Fernando, Ong Wei Jia
Publikováno v:
EPJ Web of Conferences, Vol 260, p 07003 (2022)
“Light” heavy elements (Z = 38 − 47) can be synthesized in the neutrino–driven ejecta of core–collapse supernovae via the weak r–process. This nucleosynthesis scenario exhibits uncertainties from the absence of experimental data from (α,
Externí odkaz:
https://doaj.org/article/fb7712bbdc2b4ac9a514b6ec6f14584b
Autor:
Almaraz-Calderon Sergio, Rehm K. Ernst, Asher Benjamin W., Avila Melina L., Auranen Kalle, Back Birger B., Chen Jie, Dickerson Clayton, Jiang Cheng-Lie, Pardo Richard C., Santiago-Gonzalez Daniel, Savard Guy, Talwar Rashi
Publikováno v:
EPJ Web of Conferences, Vol 242, p 01005 (2020)
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 it may also contribute to abundances of some lighter nuclides. Great excitement was recently generated
Externí odkaz:
https://doaj.org/article/7d64da99b3974448a564ede251fb3dbf
Autor:
Kawano, T., Almaraz-Calderon, Sergio, Rehm, K. Ernst, Asher, Benjamin W., Avila, Melina L., Auranen, Kalle, Back, Birger B., Chen, Jie, Dickerson, Clayton, Jiang, Cheng-Lie, Pardo, Richard C., Santiago-Gonzalez, Daniel, Savard, Guy, Talwar, Rashi
Publikováno v:
EPJ Web of Conferences; 2020, Vol. 242, p1-5, 5p