Resonances and collisional properties of neutron-rich helium isotopes in the adiabatic hyperspherical representation
Michael D. Higgins and Chris H. Greene
Phys. Rev. C 111, 014001 (2025) - Published 16 January, 2025
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, and I. T. Yandow
Phys. Rev. C 111, 014314 (2025) - Published 9 January, 2025
Sn is often regarded as the holy grail of nuclear structure studies as it is the heaviest proton-bound nucleus with equal numbers of protons and neutrons; and with it is also expected to be doubly magic. Aside from the proximity to the proton dripline, the region of the nuclear chart near Sn also harbors nuclei at the end of the process which powers x-ray bursts on the surface of accreting neutron stars. The nuclear mass is a telltale observable for nuclear structure studies and nuclear astrophysics. Just three neutrons heavier than Sn, Sn had been identified as an outlier with a seriously irregular mass deduced from its -decay value and the decay-daughter mass. An international research team performed high-precision Penning-trap mass measurements of Sn at the Facility for Rare Isotope Beams (FRIB). Their measured mass value is more than an order of magnitude more precise than that of a previous storage ring measurement. The team’s reported result reestablishes the smoothness of the nuclear mass surface and provides reevaluated values for the masses of several other important isotopes connected to Sn via decays.
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, and F. Wienholtz
Phys. Rev. C 111, 014315 (2025) - Published 9 January, 2025
Expected to be doubly magic, Sn is the heaviest proton-bound, self-conjugate () nucleus. Its mass and those of nearby nuclei are key to understanding nuclear structure and reactions near the proton dripline, including neutron-star-surface nucleosynthesis. The mass of Sn, previously an outlier due to a discrepant -decay measurement, was precisely determined by an international team at CERN ISOLDE using multireflection time-of-flight mass spectrometry, their results agreeing well with those from another, complementary technique at FRIB. This new value enables re-evaluating the masses of five parent nuclei connected via decays. Comparing their results with theory calculations, the authors recovered a smooth trend of the local nuclear mass surface for tin, tellurium, and xenon isotopes, with possible impact on nuclear structure and astrophysics. Insights into ISOL target and source performances also suggest a path toward improved production of lighter tin isotopes for future studies.
L. Xayavong and Y. Lim
Phys. Rev. C 111, 015501 (2025) - Published 13 January, 2025
decays provide important tests of the Standard Model, but the precision is limited by model dependencies and small but crucial corrections such as isospin breaking. By comparing theoretical and experimental ratios of mirror decays, the authors find cancellation of many of the model dependencies, allowing constraints on the remaining corrections and ultimately on possible new physics.
Nicolas Miró Fortier, Sangyong Jeon, and Charles Gale
Phys. Rev. C 111, L011901 (2025) - Published 6 January, 2025
Michael D. Higgins and Chris H. Greene
Phys. Rev. C 111, 014001 (2025) - Published 16 January, 2025
Shi Yuan Ding (丁士缘), Bao Yuan Sun (孙保元), and Ting-Ting Sun (孙亭亭)
Phys. Rev. C 111, 014301 (2025) - Published 2 January, 2025
K. H. Li, J. G. Li, N. Michel, H. H. Li, N. Chen, C. W. Ma, and W. Zuo
Phys. Rev. C 111, 014302 (2025) - Published 2 January, 2025
P. M. Jodidar et al.
Phys. Rev. C 111, 014303 (2025) - Published 3 January, 2025
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, and F. R. Xu
Phys. Rev. C 111, 014304 (2025) - Published 3 January, 2025
R. B. Cakirli, K. Blaum, and R. F. Casten
Phys. Rev. C 111, 014305 (2025) - Published 3 January, 2025
N. Cieplicka-Oryńczak, C. Michelagnoli, S. Leoni, B. Fornal, A. Gargano, G. Benzoni, A. Blanc, S. Bottoni, F. C. L. Crespi, Ł.W. Iskra, M. Jentschel, U. Köster, P. Mutti, N. Pietralla, E. Ruiz-Martinez, and V. Werner
Phys. Rev. C 111, 014306 (2025) - Published 6 January, 2025
A. Petrovici and O. Andrei
Phys. Rev. C 111, 014307 (2025) - Published 6 January, 2025
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, and M. Yosoi
Phys. Rev. C 111, 014308 (2025) - Published 8 January, 2025
Elina Kauppinen and Jouni Suhonen
Phys. Rev. C 111, 014309 (2025) - Published 8 January, 2025
H. Jia (贾慧), B. Qi (亓斌), L. Liu (刘雷), and E. H. Wang (王恩宏)
Phys. Rev. C 111, 014310 (2025) - Published 9 January, 2025
Pietro Klausner, Gianluca Colò, Xavier Roca-Maza, and Enrico Vigezzi
Phys. Rev. C 111, 014311 (2025) - Published 9 January, 2025
R. Schwengner, R. Massarczyk, R. Beyer, N. Benouaret, A. Ferrari, A. Hartmann, T. Hensel, E. Masha, S. E. Müller, K. Römer, M. Scheck, K. Schmidt, S. Turkat, S. Urlaß, A. Wagner, and A. Yadav
Phys. Rev. C 111, 014312 (2025) - Published 9 January, 2025
Shuichiro Ebata and Wataru Horiuchi
Phys. Rev. C 111, 014313 (2025) - Published 9 January, 2025
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, and I. T. Yandow
Phys. Rev. C 111, 014314 (2025) - Published 9 January, 2025
Sn is often regarded as the holy grail of nuclear structure studies as it is the heaviest proton-bound nucleus with equal numbers of protons and neutrons; and with it is also expected to be doubly magic. Aside from the proximity to the proton dripline, the region of the nuclear chart near Sn also harbors nuclei at the end of the process which powers x-ray bursts on the surface of accreting neutron stars. The nuclear mass is a telltale observable for nuclear structure studies and nuclear astrophysics. Just three neutrons heavier than Sn, Sn had been identified as an outlier with a seriously irregular mass deduced from its -decay value and the decay-daughter mass. An international research team performed high-precision Penning-trap mass measurements of Sn at the Facility for Rare Isotope Beams (FRIB). Their measured mass value is more than an order of magnitude more precise than that of a previous storage ring measurement. The team’s reported result reestablishes the smoothness of the nuclear mass surface and provides reevaluated values for the masses of several other important isotopes connected to Sn via decays.
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, and F. Wienholtz
Phys. Rev. C 111, 014315 (2025) - Published 9 January, 2025
Expected to be doubly magic, Sn is the heaviest proton-bound, self-conjugate () nucleus. Its mass and those of nearby nuclei are key to understanding nuclear structure and reactions near the proton dripline, including neutron-star-surface nucleosynthesis. The mass of Sn, previously an outlier due to a discrepant -decay measurement, was precisely determined by an international team at CERN ISOLDE using multireflection time-of-flight mass spectrometry, their results agreeing well with those from another, complementary technique at FRIB. This new value enables re-evaluating the masses of five parent nuclei connected via decays. Comparing their results with theory calculations, the authors recovered a smooth trend of the local nuclear mass surface for tin, tellurium, and xenon isotopes, with possible impact on nuclear structure and astrophysics. Insights into ISOL target and source performances also suggest a path toward improved production of lighter tin isotopes for future studies.
N. Fotiades, J. A. Cizewski, P. Fallon, P. G. Kevrekidis, R. Krücken, and I. Y. Lee
Phys. Rev. C 111, 014316 (2025) - Published 13 January, 2025
H. Fujita, Y. Fujita, P. Adsley, J. W. Brümmer, A. Fujimoto, D. Houngbo, M. Kohne, K. C. W. Li, P. Z. Mabika, A. Negret, R. Neveling, P. Papka, L. Pellegri, F. D. Smit, and S. Triambak
Phys. Rev. C 111, 014317 (2025) - Published 14 January, 2025
Dhananjaya Sahoo, A. Y. Deo, Madhu, Khamosh Yadav, S. S. Tiwary, P. C. Srivastava, R. Palit, S. K. Tandel, Anil Kumar, P. Dey, Biswajit Das, Vishal Malik, A. Kundu, A. Sindhu, S. V. Jadhav, B. S. Naidu, and A. V. Thomas
Phys. Rev. C 111, 014318 (2025) - Published 14 January, 2025
Jun Zhang, Hai-Qian Zhang, T. M. Shneidman, R. V. Jolos, and Xiao-Tao He
Phys. Rev. C 111, 014319 (2025) - Published 14 January, 2025
K. D. Duan, H. B. Zhang, and X. L. Shang
Phys. Rev. C 111, 014320 (2025) - Published 16 January, 2025
B. F. Lv et al.
Phys. Rev. C 111, 014321 (2025) - Published 16 January, 2025
M. Mukai, Y. Hirayama, P. Schury, Y. X. Watanabe, T. Hashimoto, N. Hinohara, S. C. Jeong, H. Miyatake, J. Y. Moon, T. Niwase, M. Reponen, M. Rosenbusch, H. Ueno, and M. Wada
Phys. Rev. C 111, 014322 (2025) - Published 17 January, 2025
De-Ye Tao (陶德晔), Bo Zhou (周波), Si-Min Wang (王思敏), and Yu-Gang Ma (马余刚)
Phys. Rev. C 111, 014323 (2025) - Published 21 January, 2025
Yu Zhang and Wei Teng
Phys. Rev. C 111, 014324 (2025) - Published 21 January, 2025
Yanhua Lu, Tianshuai Shang, Pengxiang Du, Jian Li, Haozhao Liang, and Zhongming Niu
Phys. Rev. C 111, 014325 (2025) - Published 21 January, 2025
S. Sarkar, Y. Iwata, K. Jha, and R. Chatterjee
Phys. Rev. C 111, 014326 (2025) - Published 22 January, 2025
Z. Hockenbery et al.
Phys. Rev. C 111, 014327 (2025) - Published 23 January, 2025
Shabir Dar, Soumik Bhattacharya, S. Bhattacharyya, G. H. Bhat, S. Jehangir, J. A. Sheikh, R. Banik, S. Nandi, G. Mukherjee, Sajad Ali, S. Chakraborty, S. Chatterjee, S. Das, S. Das Gupta, A. Dhal, S. S. Ghugre, A. Goswami, D. Mondal, S. Mukhopadhyay, S. Pal, D. Pandit, R. Raut, and P. Ray
Phys. Rev. C 111, 014328 (2025) - Published 28 January, 2025
B. van den Borne et al.
Phys. Rev. C 111, 014329 (2025) - Published 30 January, 2025
Joona Kasurinen, Pekka Pirinen, and Jouni Suhonen
Phys. Rev. C 111, 014601 (2025) - Published 6 January, 2025
S. T. Sun, T. Depastas, H. B. He, H. Zheng, and A. Bonasera
Phys. Rev. C 111, 014602 (2025) - Published 8 January, 2025
Gen Zhang and Feng-Shou Zhang
Phys. Rev. C 111, 014603 (2025) - Published 8 January, 2025
A. Gómez Camacho, J. Rangel, and J. Lubian
Phys. Rev. C 111, 014604 (2025) - Published 9 January, 2025
N. P. Giha, S. Marin, I. A. Tolstukhin, M. B. Oberling, R. A. Knaack, C. Mueller-Gatermann, A. Korichi, K. Bhatt, M. P. Carpenter, C. Fougères, V. Karayonchev, B. P. Kay, T. Lauritsen, D. Seweryniak, N. Watwood, D. L. Duke, S. Mosby, K. B. Montoya, D. S. Connolly, W. Loveland, I. E. Hernandez, S. D. Clarke, S. A. Pozzi, and F. Tovesson
Phys. Rev. C 111, 014605 (2025) - Published 13 January, 2025
Lei Shen (沈雷), Bo-Song Huang (黄勃松), and Yu-Gang Ma (马余刚)
Phys. Rev. C 111, 014606 (2025) - Published 16 January, 2025
Ban Zhang and Zhao-Qing Feng
Phys. Rev. C 111, 014607 (2025) - Published 17 January, 2025
Resmi K. Bharathan, Midhun C. V., M. M. Musthafa, Sreena M., Silpa Ajaykumar, Farhana Thesni M. P., Swapna B., Vafiya Thaslim T. T., Shaima A., Nived K., Akhil R., Anagha P. K., Arunima Dev T. V., Keerthi E. S., Akshay K. S., Arun P. V., and S. Ghugre
Phys. Rev. C 111, 014608 (2025) - Published 21 January, 2025
L. Shvedov, S. Burrello, M. Colonna, and H. Zheng
Phys. Rev. C 111, 014609 (2025) - Published 21 January, 2025
Gayatri Sarkar and Pooja Kaushal
Phys. Rev. C 111, 014610 (2025) - Published 22 January, 2025
I. Gheorghe, T. Ari-izumi, S. Goriely, D. Filipescu, S. Belyshev, K. Stopani, H. Wang, G. Fan, H. Scheit, D. Symochko, M. Krzysiek, T. Renstrøm, G. M. Tveten, S. Miyamoto, and H. Utsunomiya
Phys. Rev. C 111, 014611 (2025) - Published 27 January, 2025
I. A. Muzalevskii et al.
Phys. Rev. C 111, 014612 (2025) - Published 30 January, 2025
Nicolas Miro Fortier, Sangyong Jeon, and Charles Gale
Phys. Rev. C 111, 014901 (2025) - Published 6 January, 2025
Junlee Kim, Jaebeom Park, Byungsik Hong, Juhee Hong, Eun-Joo Kim, Yongsun Kim, MinJung Kweon, Su Houng Lee, Sanghoon Lim, and Jinjoo Seo
Phys. Rev. C 111, 014902 (2025) - Published 6 January, 2025
K. Werner, J. Jahan, I. Karpenko, T. Pierog, M. Stefaniak, and D. Vintache
Phys. Rev. C 111, 014903 (2025) - Published 6 January, 2025
X. G. Deng (邓先概) and Y. G. Ma (马余刚)
Phys. Rev. C 111, 014904 (2025) - Published 8 January, 2025
Banajit Barman, Nur Hussain, and Buddhadeb Bhattacharjee
Phys. Rev. C 111, 014905 (2025) - Published 8 January, 2025
M. I. Abdulhamid et al. (STAR Collaboration)
Phys. Rev. C 111, 014906 (2025) - Published 9 January, 2025
Jiaxing Zhao, Joerg Aichelin, Pol Bernard Gossiaux, and Klaus Werner
Phys. Rev. C 111, 014907 (2025) - Published 13 January, 2025
A. Pop and M. Petrovici
Phys. Rev. C 111, 014908 (2025) - Published 14 January, 2025
M. I. Abdulhamid et al. (STAR Collaboration)
Phys. Rev. C 111, 014909 (2025) - Published 16 January, 2025
Zhiyi Wang, Jinhui Chen, Diyu Shen, Aihong Tang, and Gang Wang
Phys. Rev. C 111, 014910 (2025) - Published 17 January, 2025
Yoshini Bailung, Sudhir Pandurang Rode, Neha Shah, and Ankhi Roy
Phys. Rev. C 111, 014911 (2025) - Published 22 January, 2025
Faisal Etminan
Phys. Rev. C 111, 014912 (2025) - Published 22 January, 2025
Tau Hoshino and Tetsufumi Hirano
Phys. Rev. C 111, 014913 (2025) - Published 24 January, 2025
Eduardo Grossi, Andrea Palermo, and Ismail Zahed
Phys. Rev. C 111, 014914 (2025) - Published 29 January, 2025
Shanjin Wu
Phys. Rev. C 111, 014915 (2025) - Published 30 January, 2025
Yifan Shen, Wei Chen, Xiang-Yu Wu, Kun Xu, and Mei Huang
Phys. Rev. C 111, 014916 (2025) - Published 31 January, 2025
S. Acharya et al. (ALICE Collaboration)
Phys. Rev. C 111, 015201 (2025) - Published 14 January, 2025
Roland C. Farrell, Marc Illa, and Martin J. Savage
Phys. Rev. C 111, 015202 (2025) - Published 14 January, 2025
Abdussamad M., Rahul Verma, Nirbhay Kumar Behera, Sadhana Dash, and Basanta Kumar Nandi
Phys. Rev. C 111, 015203 (2025) - Published 16 January, 2025
L. Xayavong and Y. Lim
Phys. Rev. C 111, 015501 (2025) - Published 13 January, 2025
decays provide important tests of the Standard Model, but the precision is limited by model dependencies and small but crucial corrections such as isospin breaking. By comparing theoretical and experimental ratios of mirror decays, the authors find cancellation of many of the model dependencies, allowing constraints on the remaining corrections and ultimately on possible new physics.
Ryan Curry, Rahul Somasundaram, Stefano Gandolfi, Alexandros Gezerlis, and Ingo Tews
Phys. Rev. C 111, 015801 (2025) - Published 2 January, 2025
Steven P. Harris, Bryce Fore, and Sanjay Reddy
Phys. Rev. C 111, 015802 (2025) - Published 6 January, 2025
V. W. Ingeberg et al. (The ISOLDE Collaboration)
Phys. Rev. C 111, 015803 (2025) - Published 16 January, 2025
Aziz Rabhi, Olfa Boukari, Sidney S. Avancini, and Constança Providência
Phys. Rev. C 111, 015804 (2025) - Published 17 January, 2025
N. Chamel, N. N. Shchechilin, and A. I. Chugunov
Phys. Rev. C 111, 015805 (2025) - Published 21 January, 2025
Duncan Neill, David Tsang, Christian Drischler, Jeremy W. Holt, and William G. Newton
Phys. Rev. C 111, 015809 (2025) - Published 27 January, 2025
Dake Zhou
Phys. Rev. C 111, 015810 (2025) - Published 27 January, 2025
Kyoungsu Heo, Myung-Ki Cheoun, Ki-Seok Choi, K. S. Kim, and W. Y. So
Phys. Rev. C 111, 019901 (2025) - Published 7 January, 2025
H. Lu, M. J. Barlow, D. Basler, P. Gutfreund, O. Holderer, A. Ioffe, S. Pasini, P. Pistel, Z. Salhi, K. Zhernenkov, B. M. Goodson, W. M. Snow, and E. Babcock
Phys. Rev. C 111, 019902 (2025) - Published 24 January, 2025