JINA - Virtual Journal of Nuclear Astrophysics,
10 January 2025
Volume 23, Issue 2 (32 Articles)
- # 1 - Enabling high mass accretion rates onto massive main sequence stars by outer envelope mass removal
- # 2 - The joint detection rate of short gamma-ray bursts and gravitational waves from binary neutron star mergers
- # 3 - Cross Section Measurements of Large Angle Fragments Production in the Interaction of Carbon Ion Beams with Thin Targets
- The FOOT Collaboration, Y. Dong (INFN Section of Milano, Milano, Italy), I. Mattei (INFN Section of Milano, Milano, 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 (INFN Section of Napoli, Napoli, Italy, University of Napoli, Department of Physics "E. Pancini", 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 (INFN Section of Napoli, Napoli, Italy, University of Napoli, Department of Physics "E. Pancini", Napoli, Italy), A. Di Crescenzo (INFN Section of Napoli, Napoli, Italy, University of Napoli, Department of Physics "E. Pancini", Napoli, Italy), B. Di Ruzza (University of Foggia, Foggia, Italy, INFN Section of Bari, Bari, Italy), M. Dondi (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), M. Donetti (INFN Section of Torino, Torino, Italy, CNAO Centro Nazionale di Adroterapia Oncologica, Pavia, 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 (INFN Section of Roma 1, Rome, Italy, University of Rome La Sapienza, Department of Scienze di Base e Applicate per l'Ingegneria), 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 (INFN Section of Napoli, Napoli, Italy, University of Napoli, Department of Physics "E. Pancini", 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 (INFN Section of Napoli, Napoli, Italy, University of Napoli, Department of Physics "E. Pancini", Napoli, Italy), E. Lopez Torres (INFN Section of Torino, Torino, Italy, CEADEN, Centro de Aplicaciones Tecnologicas y Desarrollo Nuclear, Havana, Cuba), M. Magi (INFN Section of Roma 1, Rome, Italy, University of Rome La Sapienza, Department of Scienze di Base e Applicate per l'Ingegneria), A. Manna (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), M. Marafini (INFN Section of Roma 1, Rome, Italy, Museo Storico della Fisica e Centro Studi e Ricerche Enrico Fermi, 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), A. Mengarelli (INFN Section of Bologna, Bologna, 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 (INFN Section of Roma 1, Rome, Italy, University of Rome La Sapienza, Department of Scienze di Base e Applicate per l'Ingegneria), 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), R. Ridolfi (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), 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), O. Sato (Nagoya University, Department of Physics, Nagoya, Japan), S. Savazzi (CNAO Centro Nazionale di Adroterapia Oncologica, Pavia, Italy), L. Scavarda (Nagoya University, Department of Physics, Nagoya, Japan), A. Schiavi (INFN Section of Roma 1, Rome, Italy, Universit'e de Strasbourg, CNRS, IPHC UMR 7871, F-67000 Strasbourg, France), C. Schuy (CNAO Centro Nazionale di Adroterapia Oncologica, Pavia, Italy), E. Scifoni (University of Miami, Radiation Oncology, Miami, FL, United States), L. Servoli (INFN Section of Perugia, Perugia, Italy), G. Silvestre (INFN Section of Perugia, Perugia, Italy), M. Sitta (INFN Section of Torino, Torino, Italy, ALTEC, Aerospace Logistic Technology Engineering Company, Corso Marche 79, 10146 Torino, Italy), R. Spighi (INFN Section of Bari, Bari, Italy), E. Spiriti (University of Piemonte Orientale, Department for Sustainable Development, Ecological Transition, Vercelli, Italy), L. Testa (University of Rome La Sapienza, Department of Physics, Rome, Italy, INFN Section of Roma 1, Rome, Italy), V. Tioukov (INFN Section of Napoli, Napoli, Italy), S. Tomassini (INFN Laboratori Nazionali di Frascati, Frascati, Italy), F. Tommasino (University of Miami, Radiation Oncology, Miami, FL, United States, University of Trento, Department of Physics, Trento, Italy), M. Toppi (INFN Section of Roma 1, Rome, Italy, University of Rome La Sapienza, Department of Scienze di Base e Applicate per l'Ingegneria), 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), M. Villa (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), 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), A. Sarti (INFN Section of Roma 1, Rome, Italy, University of Rome La Sapienza, Department of Scienze di Base e Applicate per l'Ingegneria)
- https://arxiv.org/abs/2501.04392
- # 4 - Interplay of shell evolution and configuration mixing in the single-hole-like states of $^{99-131}$In
- # 5 - Isolated one-phonon mixed-symmetry 2+ state of the radioactive neutron-rich nuclide 132Te
- T. Stetz, H. Mayr, V. Werner, N. Pietralla, Y. Tsunoda, T. Otsuka, G. Rainovski, T. Beck, R. Borcea, S. Calinescu, C. Costache, I. E. Dinescu, K. E. Ide, A. N. Ionescu, P. Koseoglou, R. Lica, N. Mu{a}rginean, R. E. Mihai, C. M. Nickel, C. R. Nita, L. Stan, S. Toma, R. Zidarova
- https://arxiv.org/abs/2501.01436
- # 6 - Near-threshold dipole strength in {^{10}}Be with isoscalar character
- J. Chen, Y. Ayyad, D. Bazin, W. Mittig, M. Z. Serikow, N. Keeley, S. M. Wang, B. Zhou, J. C. Zamora, S. Beceiro-Novo, M. Cortesi, M. DeNudt, S. Heinitz, S. Giraud, P. Gueye, C. R. Hoffman, B. P. Kay, E. A. Maugeri, B. G. Monteagudo, H. Li, W. P. Liu, A. Munoz, F. Ndayisabye, J. Pereira, N. Rijal, C. Santamaria, D. Schumann, N. Watwood, G. Votta, P. Yin, C. X. Yuan, Y. N. Zhang
- https://arxiv.org/abs/2501.05231
- # 7 - The Gallium Solar Neutrino Capture Cross Section Revisited
- # 8 - Analysis of clustering fragments of $^7$Li and $^7$Be in the microscopic cluster model
- # 9 - Direct observation of $beta$ and $gamma$ decay from a high-spin long-lived isomer in $^{187}$Ta
- J. L. Chen, H. Watanabe, P. M. Walker, Y. Hirayama, Y. X. Watanabe, M. Mukai, C. F. Jiao, M. Ahmed, M. Brunet, T. Hashimoto, S. Ishizawa, F. G. Kondev, G. J. Lane, Yu. A. Litvinov, H. Miyatake, J. Y. Moon, T. Niwase, J. H. Park, Zs. Podoly'ak, M. Rosenbusch, P. Schury, M. Wada, F. R. Xu
- https://arxiv.org/abs/2501.02848
- # 10 - Fast rotation of nuclei with extreme isospin in the vicinity of neutron and proton drip lines
- # 11 - Nuclear cross sections from low-energy interactions
- # 12 - Parity doubled nucleons can rapidly cool neutron stars
- # 13 - The impact of mass uncertainties on the r-process nucleosynthesis in neutron star mergers
- # 14 - Controlling few-body reaction pathways using a Feshbach resonance
- # 15 - Study of possible antimagnetic rotation in 100Ru
- # 16 - Direct observation of $β$ and $γ$ decay from a high-spin long-lived isomer in $^{187}mathrm{Ta}$
- J. L. Chen, H. Watanabe, P. M. Walker, Y. Hirayama, Y. X. Watanabe, M. Mukai, C. F. Jiao, M. Ahmed, M. Brunet, T. Hashimoto, S. Ishizawa, F. G. Kondev, G. J. Lane, Yu. A. Litvinov, H. Miyatake, J. Y. Moon, T. Niwase, J. H. Park, Zs. Podolyák, M. Rosenbusch, P. Schury, M. Wada,, F. R. Xu
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.111.014304
- # 17 - Excitation of the isoscalar giant monopole resonance using $^{6}mathrm{Li}$ 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
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.111.014308
- # 18 - High-precision mass measurement of $^{103}mathrm{Sn}$ restores smoothness of the mass surface
- C. M. Ireland, F. M. Maier, G. Bollen, S. E. Campbell, X. Chen, H. Erington, N. D. Gamage, M. J. Gutiérrez, C. Izzo, E. Leistenschneider, E. M. Lykiardopoulou, R. Orford, W. S. Porter, D. Puentes, M. Redshaw, R. Ringle, S. Rogers, S. Schwarz, L. Stackable, C. S. Sumithrarachchi, A. A. Valverde, A. C. C. Villari,, I. T. Yandow
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.111.014314
- # 19 - Influence of the capture of breakup fragments on the fusion of $^{8}mathrm{B}$ with several targets
- # 20 - Investigation of possible antimagnetic rotation with neutron “blades” in $^{140}mathrm{Sm}$ and $^{140}mathrm{Gd}$
- # 21 - Isoscalar and isovector multipole $L=0$ to 3 strength functions in even-even $^{90–94}mathrm{Zr}$ and $^{92–100}mathrm{Mo}$ nuclei
- # 22 - Multiple shape coexistence in $^{98}mathrm{Zr}$ and first-forbidden $β$ decay of $^{98}mathrm{Y}$
- # 23 - Natural solution of the low-lying level structure of $^{114}mathrm{I}$ from complementary measurements and new interpretation of the high-spin bands
- # 24 - One-proton-hole, one-neutron-hole excitations at low spins in $^{206}mathrm{Tl}$
- N. Cieplicka-OryÅczak, C. Michelagnoli, S. Leoni, B. Fornal, A. Gargano, G. Benzoni, A. Blanc, S. Bottoni, F. C. L. Crespi, Å.W. Iskra, M. Jentschel, U. Köster, P. Mutti, N. Pietralla, E. Ruiz-Martinez,, V. Werner
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.111.014306
- # 25 - Production of neutron-rich nuclei near $N=126$ in multinucleon transfer reactions with potential pockets
- # 26 - Refining the nuclear mass surface with the mass of $^{103}mathrm{Sn}$
- L. Nies, D. Atanasov, M. Athanasakis-Kaklamanakis, M. Au, C. Bernerd, K. Blaum, K. Chrysalidis, P. Fischer, R. Heinke, C. Klink, D. Lange, D. Lunney, V. Manea, B. A. Marsh, M. Müller, M. Mougeot, S. Naimi, Ch. Schweiger, L. Schweikhard,, F. Wienholtz
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.111.014315
- # 27 - Role of excited states in the sub-barrier fusion of light nuclei
- # 28 - Investigating the role of nuclear parameters on oscillation modes in hot neutron stars
- # 29 - Near-Threshold Dipole Strength in $^{10}mathrm{Be}$ with Isoscalar Character
- # 30 - The 18F()15O reaction: A textbook case in nuclear astrophysics
- # 31 - Using gravitational waves to see the first second of the Universe
- # 32 - Comparison of the Origin of Short Gamma-Ray Bursts with or without Extended Emission
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.
