JINA - Virtual Journal of Nuclear Astrophysics,
3 January 2025
Volume 23, Issue 1 (23 Articles)
- # 1 - Bayesian analysis of hybrid neutron star EoS constraints within a nonlocal color superconducting quark matter model
- # 2 - Impact of QCD sum rules coupling constants on neutron stars structure
- # 3 - Investigating chemical variations between interstellar gas clouds in the Solar neighbourhood
- # 4 - Neutron star stability beyond the mass peak: assessing the role of out-of-equilibrium perturbations
- # 5 - Thermal Contributions to Primordial Nucleosynthesis
- # 6 - Timescales of Solar System Formation Based on Al-Ti Isotope Correlation by Supernova Ejecta
- # 7 - Angular differential and elemental fragmentation cross sections of a $400,text{MeV/nucleon}$ $^{16}text{O}$ beam on a graphite target with the FOOT experiment
- FOOT Collaboration, R. Ridolfi (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), M. Toppi (University of Rome La Sapienza, Department of Scienze di Base e Applicate per l'Ingegneria, INFN Section of Roma 1, Rome, Italy), A. Mengarelli (INFN Section of Bologna, Bologna, Italy), M. Dondi (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), A. Alexandrov (INFN Section of Napoli, Napoli, Italy), B. Alpat (INFN Section of Perugia, Perugia, Italy), G. Ambrosi (INFN Section of Perugia, Perugia, Italy), S. Argir`o (University of Torino, Department of Physics, Torino, Italy, INFN Section of Torino, Torino, Italy), M. Barbanera (INFN Section of Perugia, Perugia, Italy), N. Bartosik (INFN Section of Torino, Torino, Italy), G. Battistoni (INFN Section of Milano, Milano, Italy), M. G. Bisogni (University of Pisa, Department of Physics, Pisa, Italy, INFN Section of Pisa, Pisa, Italy), V. Boccia (University of Napoli, Department of Physics "E. Pancini", Napoli, Italy, INFN Section of Napoli, Napoli, Italy), F. Cavanna (INFN Section of Torino, Torino, Italy), P. Cerello (INFN Section of Torino, Torino, Italy), E. Ciarrocchi (University of Pisa, Department of Physics, Pisa, Italy, INFN Section of Pisa, Pisa, Italy), A. De Gregorio (University of Rome La Sapienza, Department of Physics, Rome, Italy, INFN Section of Roma 1, Rome, Italy), G. De Lellis (University of Napoli, Department of Physics "E. Pancini", Napoli, Italy, INFN Section of Napoli, Napoli, Italy), A. Di Crescenzo (University of Napoli, Department of Physics "E. Pancini", Napoli, Italy, INFN Section of Napoli, Napoli, Italy), B. Di Ruzza (University of Foggia, Foggia, Italy, INFN Section of Bari, Bari, Italy), M. Donetti (CNAO Centro Nazionale di Adroterapia Oncologica, Pavia, Italy, INFN Section of Torino, Torino, Italy), Y. Dong (INFN Section of Milano, Milano, Italy), M. Durante (University of Napoli, Department of Physics "E. Pancini", Napoli, Italy, Biophysics Department, GSI Helmholtzzentrum f"ur Schwerionenforschung, Darmstadt, Germany), R. Faccini (University of Rome La Sapienza, Department of Physics, Rome, Italy, INFN Section of Roma 1, Rome, Italy), V. Ferrero (INFN Section of Torino, Torino, Italy), C. Finck (Universit'e de Strasbourg, CNRS, IPHC UMR 7871, F-67000 Strasbourg, France), E. Fiorina (INFN Section of Torino, Torino, Italy), M. Francesconi (INFN Section of Napoli, Napoli, Italy), M. Franchini (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), G. Franciosini (University of Rome La Sapienza, Department of Scienze di Base e Applicate per l'Ingegneria, INFN Section of Roma 1, Rome, Italy), G. Galati (University of Bari, Department of Physics, Bari, Italy, INFN Section of Bari, Bari, Italy), L. Galli (INFN Section of Pisa, Pisa, Italy), M. Ionica (INFN Section of Perugia, Perugia, Italy), A. Iuliano (University of Napoli, Department of Physics "E. Pancini", Napoli, Italy, INFN Section of Napoli, Napoli, Italy), K. Kanxheri (INFN Section of Perugia, Perugia, Italy, University of Perugia, Department of Physics, Geology, Perugia, Italy), A. C. Kraan (INFN Section of Pisa, Pisa, Italy), C. La Tessa (University of Miami, Radiation Oncology, Miami, FL, United States, Trento Institute for Fundamental Physics, Applications, Istituto Nazionale di Fisica Nucleare), A. Lauria (University of Napoli, Department of Physics "E. Pancini", Napoli, Italy, INFN Section of Napoli, Napoli, Italy), E. Lopez Torres (CEADEN, Centro de Aplicaciones Tecnologicas y Desarrollo Nuclear, Havana, Cuba, INFN Section of Torino, Torino, Italy), M. Magi (University of Rome La Sapienza, Department of Scienze di Base e Applicate per l'Ingegneria, INFN Section of Roma 1, Rome, Italy), A. Manna (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), M. Marafini (Museo Storico della Fisica e Centro Studi e Ricerche Enrico Fermi, Rome, Italy, INFN Section of Roma 1, Rome, Italy), M. Massa (INFN Section of Pisa, Pisa, Italy), C. Massimi (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), I. Mattei (INFN Section of Milano, Milano, Italy), A. Mereghetti (CNAO Centro Nazionale di Adroterapia Oncologica, Pavia, Italy), T. Minniti (University of Rome Tor Vergata, Department of Physics, Rome, Italy, INFN Section of Roma Tor Vergata, Rome, Italy), A. Moggi (INFN Section of Pisa, Pisa, Italy), M. C. Montesi (INFN Section of Napoli, Napoli, Italy, University of Napoli, Department of Chemistry, Napoli, Italy), M. C. Morone (University of Rome Tor Vergata, Department of Physics, Rome, Italy, INFN Section of Roma Tor Vergata, Rome, Italy), M. Morrocchi (University of Pisa, Department of Physics, Pisa, Italy, INFN Section of Pisa, Pisa, Italy), S. Muraro (INFN Section of Milano, Milano, Italy), N. Pastrone (INFN Section of Torino, Torino, Italy), V. Patera (University of Rome La Sapienza, Department of Scienze di Base e Applicate per l'Ingegneria, INFN Section of Roma 1, Rome, Italy), F. Peverini (INFN Section of Perugia, Perugia, Italy, University of Perugia, Department of Physics, Geology, Perugia, Italy), F. Pennazio (INFN Section of Torino, Torino, Italy), C. Pisanti (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), P. Placidi (INFN Section of Perugia, Perugia, Italy, University of Perugia, Department of Engineering, Perugia, Italy), M. Pullia (CNAO Centro Nazionale di Adroterapia Oncologica, Pavia, Italy), L. Ramello (INFN Section of Torino, Torino, Italy, University of Piemonte Orientale, Department for Sustainable Development, Ecological Transition, Vercelli, Italy), C. Reidel (Biophysics Department, GSI Helmholtzzentrum f"ur Schwerionenforschung, Darmstadt, Germany), L. Sabatini (INFN Laboratori Nazionali di Frascati, Frascati, Italy), L. Salvi (INFN Section of Perugia, Perugia, Italy, University of Perugia, Department of Physics, Geology, Perugia, Italy), C. Sanelli (INFN Laboratori Nazionali di Frascati, Frascati, Italy), A. Sarti (University of Rome La Sapienza, Department of Scienze di Base e Applicate per l'Ingegneria, INFN Section of Roma 1, Rome, Italy), O. Sato (Nagoya University, Department of Physics, Nagoya, Japan), S. Savazzi (CNAO Centro Nazionale di Adroterapia Oncologica, Pavia, Italy), L. Scavarda (ALTEC, Aerospace Logistic Technology Engineering Company, Corso Marche 79, 10146 Torino, Italy), A. Schiavi (University of Rome La Sapienza, Department of Scienze di Base e Applicate per l'Ingegneria, INFN Section of Roma 1, Rome, Italy), C. Schuy (Biophysics Department, GSI Helmholtzzentrum f"ur Schwerionenforschung, Darmstadt, Germany), E. Scifoni (Trento Institute for Fundamental Physics, Applications, Istituto Nazionale di Fisica Nucleare), L. Servoli (INFN Section of Perugia, Perugia, Italy), G. Silvestre (INFN Section of Perugia, Perugia, Italy), M. Sitta (INFN Section of Torino, Torino, Italy, University of Piemonte Orientale, Department of Science, Technological Innovation, Alessandria, Italy), R. Spighi (INFN Section of Bologna, Bologna, Italy), E. Spiriti (INFN Laboratori Nazionali di Frascati, Frascati, Italy), L. Testa (INFN Section of Roma 1, Rome, Italy, University of Rome La Sapienza, Department of Physics, Rome, Italy), V. Tioukov (INFN Section of Napoli, Napoli, Italy), S. Tomassini (INFN Laboratori Nazionali di Frascati, Frascati, Italy), F. Tommasino (University of Trento, Department of Physics, Trento, Italy, Trento Institute for Fundamental Physics, Applications, Istituto Nazionale di Fisica Nucleare), A. Trigilio (INFN Laboratori Nazionali di Frascati, Frascati, Italy), G. Traini (INFN Section of Roma 1, Rome, Italy), G. Ubaldi (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), A. Valetti (University of Torino, Department of Physics, Torino, Italy, INFN Section of Torino, Torino, Italy), M. Vanstalle (Universit'e de Strasbourg, CNRS, IPHC UMR 7871, F-67000 Strasbourg, France), U. Weber (Biophysics Department, GSI Helmholtzzentrum f"ur Schwerionenforschung, Darmstadt, Germany), R. Zarrella (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), A. Zoccoli (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), M. Villa (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy)
- https://arxiv.org/abs/2501.00553
- # 8 - Improved measurements of neutron lifetime with cold neutron beam at J-PARC
- Y. Fuwa, T. Hasegawa, K. Hirota, T. Hoshino, R. Hosokawa, G. Ichikawa, S. Ieki, T. Ino, Y. Iwashita, M. Kitaguchi, R. Kitahara, S. Makise, K. Mishima, T. Mogi, N. Nagakura, H. Oide, H. Okabe, H. Otono, Y. Seki, D. Sekiba, T. Shima, H. E. Shimizu, H. M. Shimizu, N. Sumi, H. Sumino, M. Tanida, H. Uehara, T. Yamada, S. Yamashita, K. Yano, T. Yoshioka
- https://arxiv.org/abs/2412.19519
- # 9 - The Felsenkeller shallow-underground laboratory for nuclear astrophysics
- Daniel Bemmerer, Axel Boeltzig, Marcel Grieger, Katharina Gudat, Thomas Hensel, Eliana Masha, Max Osswald, Bruno Poser, Simon R"ummler, Konrad Schmidt, Jos'e Luis Ta'in, Ariel Tarife~no-Saldivia, Steffen Turkat, Anup Yadav, Kai Zuber
- https://arxiv.org/abs/2412.19874
- # 10 - Excitation of the isoscalar giant monopole resonance using 6Li inelastic scattering
- J. Arroyo, U. Garg, H. Akimune, G. P. A. Berg, D. C. Cuong, M. Fujiwara, M. N. Harakeh, M. Itoh, T. Kawabata, K. Kawase, J. T. Matta, D. Patel, M. Uchida, M. Yosoi
- https://arxiv.org/abs/2412.18658
- # 11 - Impacts of dineutrons on nuclear compositions and neutrino reactions of the core-collapse supernova
- # 12 - Measurement of $rm ^{6}H$ ground state energy in an electron scattering experiment at MAMI-A1
- Tianhao Shao, Jinhui Chen, Josef Pochodzalla, Patrick Achenbach, Mirco Christmann, Michael O. Distler, Luca Doria, Anselm Esser, Julian Geratz, Christian Helmel, Matthias Hoek, Ryoko Kino, Pascal Klag, Yu-Gang Ma, David Markus, Harald Merkel, Miha Mihoviloviv{c}, Ulrich M"uller, Sho Nagao, Satoshi N. Nakamura, Kotaro Nishi, Ken Nishida, Fumiya Oura, Jonas P"atschke, Bj"orn S"oren Schlimme, Concettina Sfienti, Daniel Steger, Marcell Steinen, Michaela Thiel, Andrzej Wilczek, Luca Wilhelm
- https://arxiv.org/abs/2501.01232
- # 13 - Tracing the Milky Way spiral arms with 26Al
- # 14 - α-induced total reaction cross sections based on the intranuclear cascade model
- # 15 - Experimental study of $α$-induced reactions on $^{113}mathrm{In}$ for the astrophysical $p$ process
- # 16 - Quadrupole dynamics of carbon isotopes and $^{10}mathrm{Be}$
- # 17 - Gamow shell model for dynamic Thomas-Ehrman shift in $^{16}mathrm{Ne}/^{16}mathrm{C}$ and $^{18}mathrm{Mg}/^{18}mathrm{C}$
- # 18 - Neutron stars and the cosmological constant problem
- # 19 - Nucleon-Nucleon Short-Range Correlations: A Hidden Driver in Binary Neutron Star Inspiral Gravitational Waves
- # 20 - Diversity in Hydrogen-rich Envelope Mass of Type II Supernovae. I. Plateau Phase Light-curve Modeling
- # 21 - Diversity in Hydrogen-rich Envelope Mass of Type II Supernovae. II. SN 2023ixf as Explosion of Partially Stripped Intermediate Massive Star
- # 22 - Laboratory Studies on Absolute n-resolved Charge-exchange Cross Sections and Modeling X-Ray Emissions for Ne8+ Colliding with H2 and He
- # 23 - Equation of State Independent Determination on the Radius of a 1.4 M⊙ Neutron Star Using Mass–Radius Measurements
This material is based upon work supported in part by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under Award Number DE-SC0026204.
