Short-distance production of three particles with large scattering length
T. G. Backert, S. Dietz, H.-W. Hammer, S. König, and D. T. Son
Phys. Rev. C 113, 064001 (2026) - Published 18 June, 2026
S. Uthayakumaar, A. Spyrou, C. Harris, P. A. Denissenkov, D. Mücher, H. C. Berg, J. A. Clark, P. A. DeYoung, A. C. Dombos, B. Greaves, M. Guttormsen, F. Herwig, A. C. Larsen, S. N. Liddick, S. Lyons, J. Owens-Fryar, A. Palmisano-Kyle, G. Perdikakis, A. L. Richard, D. Santiago-Gonzalez, G. Savard, S. Siem, M. K. Smith, W. W. von Seeger, and M. Wiedeking
Phys. Rev. C 113, 065801 (2026) - Published 1 June, 2026
A key goal in nuclear astrophysics is explaining the abundance patterns of the elements in combination with observational astrophysical data and nuclear reaction networks. Although two nuclear reaction pathways—the slow ( process) and rapid ( process) neutron capture processes—are known to produce many heavy elements beyond iron, a process at intermediate neutron densities (the process) has been proposed. This process is an additional pathway that occurs in some stellar environments to explain observed elemental abundances. In this work, the authors utilized a Br beam that was implanted within a -ray total absorption spectrometer to produce the compound nucleus Kr through decay. The authors measured the constrained neutron radiative capture on Kr, showing that it plays an important role in the production of Rb in the conditions of the process. In addition, the results significantly reduce the uncertainty in the rate of this reaction by determining the -ray strength function in the compound nucleus Kr. This work demonstrates that reducing experimental uncertainties in a single neutron-capture reaction can significantly affect comparisons with theoretical predictions of element abundance patterns.
Grigor Atoian et al. (EPIOS Scientific Consortium)
Phys. Rev. C 113, 060501 (2026) - Published 9 June, 2026
Spin utilization in large particle accelerators is a young quantum technology, with practical realization only emerging in the late twentieth century. Polarized ion beams at the future Electron Ion Collider (EIC) are essential to address some of the most important open questions at the twenty-first-century frontiers of our understanding of the fundamental structure of matter. How does the proton spin of arise from the highly relativistic constituent quarks and gluons and their interactions via QCD? Are the quark and gluon nucleon spin distributions modified inside the nucleus? Can exotic gluons exist in the nucleus? Beyond these questions, polarized electron and ion beams are crucial for unravelling the full three-dimensional structure of the nucleon and of nuclei. This Perspective paper summarizes the science case and identifies polarized ion beams as the critical technology enabling the experiments that address these questions. The authors further discuss the required ion polarimetry and spin manipulation at the EIC, and identify a significant R&D effort, involving both national laboratories and universities, that will be required over roughly a decade to realize the polarized ion beams.
Y. M. Wang, Q. B. Chen, and Z. P. Li
Phys. Rev. C 113, L061301 (2026) - Published 11 June, 2026
Weijie Du, Yangguang Yang, Zixin Liu, Chao Yang, and James P. Vary
Phys. Rev. C 113, L061302 (2026) - Published 12 June, 2026
H. Y. Shang, R. Z. Hu, X. Y. Xu, Z. C. Xu, J. C. Pei, and S. M. Wang
Phys. Rev. C 113, L061303 (2026) - Published 12 June, 2026
H. F. Bai (白洪斐) et al.
Phys. Rev. C 113, L061304 (2026) - Published 22 June, 2026
L. M. Robledo
Phys. Rev. C 113, L061305 (2026) - Published 26 June, 2026
N. Muramatsu et al. (BGOegg Collaboration)
Phys. Rev. C 113, L062201 (2026) - Published 25 June, 2026
M. Ablikim et al. (BESIII Collaboration)
Phys. Rev. C 113, L062202 (2026) - Published 29 June, 2026
Z. Kóródi, G. G. Kiss, P. Mohr, T. N. Szegedi, C. Marshall, R. Nunes, L. Csedreki, Gy. Gyürky, Z. Halász, T. Szücs, S. R. Kovács, Zs. Mátyus, Á. Tóth, G. L. Guardo, M. La Cognata, A. Tumino, A. Di Pietro, A. Nurmukhanbetova, L. Balliet, and C. Fougères
Phys. Rev. C 113, L062801 (2026) - Published 8 June, 2026
M. Abubakar, J. S. Randhawa, S. R. Carmichael, P. D. O'Malley, D. W. Bardayan, J. J. Kolata, R. Longland, C. Dembski, W. S. Porter, W. W. von Seeger, M. Sorensen, T. Psaltis, R. Zite, and M. A. Zubair
Phys. Rev. C 113, L062802 (2026) - Published 17 June, 2026
T. G. Backert, S. Dietz, H.-W. Hammer, S. König, and D. T. Son
Phys. Rev. C 113, 064001 (2026) - Published 18 June, 2026
F. Marino, C. Barbieri, and G. Colò
Phys. Rev. C 113, 064301 (2026) - Published 1 June, 2026
Guo-peng Li, Ji-you Fu, Jin Zhou, Xin-le Shang, Jian-min Dong, and Wei Zuo
Phys. Rev. C 113, 064302 (2026) - Published 1 June, 2026
Jizheng Bo
Phys. Rev. C 113, 064303 (2026) - Published 2 June, 2026
A. Sehovic, K. Fossez, and H. Hergert
Phys. Rev. C 113, 064304 (2026) - Published 2 June, 2026
Urban Vernik, Kai Hebeler, and Achim Schwenk
Phys. Rev. C 113, 064305 (2026) - Published 4 June, 2026
M. Homma and K. Nomura
Phys. Rev. C 113, 064306 (2026) - Published 4 June, 2026
Rohit M. Shinde and Praveen C. Srivastava
Phys. Rev. C 113, 064307 (2026) - Published 4 June, 2026
I. Dickenson, B. Longfellow, T. Beck, A. Gade, D. Weisshaar, B. A. Brown, D. Bazin, K. W. Brown, R. J. Charity, P. J. Farris, S. A. Gillespie, A. M. Hill, J. Li, W. Reviol, and D. Rhodes
Phys. Rev. C 113, 064308 (2026) - Published 8 June, 2026
Kaizhong Tan, Jian Liu, and Chuan Wang
Phys. Rev. C 113, 064309 (2026) - Published 8 June, 2026
W. F. Li (李伟峰), T. Sun (孙婷), Z. M. Niu (牛中明), and H. Z. Liang (梁豪兆)
Phys. Rev. C 113, 064310 (2026) - Published 9 June, 2026
R. W. Fearick, O. Le Noan, H. Matsubara, P. von Neumann-Cosel, K. Sieja, and A. Tamii
Phys. Rev. C 113, 064311 (2026) - Published 12 June, 2026
M. Begala et al.
Phys. Rev. C 113, 064312 (2026) - Published 17 June, 2026
A. Bahini, V. O. Nesterenko, P. von Neumann-Cosel, P.-G. Reinhard, J. Carter, N. A. Ashurko, R. Neveling, A. Repko, and I. T. Usman
Phys. Rev. C 113, 064313 (2026) - Published 18 June, 2026
D. J. Hartley, F. G. Kondev, G. J. Lane, R. V. F. Janssens, G. D. Dracoulis, A. P. Byrne, M. P. Carpenter, P. Chowdhury, T. Lauritsen, D. Seweryniak, and H. Watanabe
Phys. Rev. C 113, 064314 (2026) - Published 22 June, 2026
Teng Wang, Xu Feng, and Bing-Nan Lu
Phys. Rev. C 113, 064315 (2026) - Published 22 June, 2026
Yuma Kikuchi, Kiyoshi Katō, and Takayuki Myo
Phys. Rev. C 113, 064316 (2026) - Published 22 June, 2026
H. Zidani and H. Naïdja
Phys. Rev. C 113, 064317 (2026) - Published 24 June, 2026
Mengyao Huang, Tobias Frederico, Peng Yin, Robert A. M. Basili, Patrick J. Fasano, and James P. Vary
Phys. Rev. C 113, 064318 (2026) - Published 25 June, 2026
Tongqi Liang, Dong Bai, and Zhongzhou Ren
Phys. Rev. C 113, 064319 (2026) - Published 29 June, 2026
Carole Chatel et al. (Nu-Ball Collaboration)
Phys. Rev. C 113, 064320 (2026) - Published 30 June, 2026
V. I. Bondarenko and M. H. Urin
Phys. Rev. C 113, 064321 (2026) - Published 29 June, 2026
E. S. Paul et al.
Phys. Rev. C 113, 064322 (2026) - Published 30 June, 2026
Xudong Wang, Bin Qi, Shouyu Wang, and Chen Liu
Phys. Rev. C 113, 064323 (2026) - Published 30 June, 2026
W.-L. Lv (吕万里), Y.-F. Niu (牛一斐), and G. Coló
Phys. Rev. C 113, 064324 (2026) - Published 30 June, 2026
C. De Lucia, A. Martone, F. A. D'Aniello, A. Mastroianni, G. Nunziata, G. De Gregorio, R. Folprecht, F. Knapp, N. Lo Iudice, and P. Veselý
Phys. Rev. C 113, 064325 (2026) - Published 30 June, 2026
W. Horiuchi, Y. Suzuki, and R. B. Wiringa
Phys. Rev. C 113, 064601 (2026) - Published 1 June, 2026
Teck-Ghee Lee, Orhan Bayrak, and Cheuk-Yin Wong
Phys. Rev. C 113, 064602 (2026) - Published 4 June, 2026
B. Mauss, J. Taïeb, B. Laurent, G. Bélier, A. Chatillon, D. Étasse, P. Morfouace, O. Roig, M. Devlin, R. C. Haight, and K. J. Kelly
Phys. Rev. C 113, 064603 (2026) - Published 5 June, 2026
Zu-Xing Yang, Xiao-Hua Fan, Peng-Hui Chen, and Shunji Nishimura
Phys. Rev. C 113, 064604 (2026) - Published 10 June, 2026
Shiva Prasad Nayak, E. Prasad, D. J. Hinde, M. Dasgupta, C. Simenel, K. J. Cook, E. C. Simpson, J. Walshe, D. Y. Jeung, C. Sengupta, K. Vo-Phuoc, J. F. Smith, I. P. Carter, H. Albers, J. Khuyagbaatar, and Ch. E. Düllmann
Phys. Rev. C 113, 064605 (2026) - Published 11 June, 2026
Xilong Xiang, Manzi Nan, Pengcheng Li, Yongjia Wang, Ling Liu, and Qingfeng Li
Phys. Rev. C 113, 064606 (2026) - Published 10 June, 2026
Xu Han, Jie Liu, Zhen-Peng Chen, Tie-Jun Zu, and Tao Ye
Phys. Rev. C 113, 064607 (2026) - Published 10 June, 2026
J. Casal and J. Gómez-Camacho
Phys. Rev. C 113, 064608 (2026) - Published 12 June, 2026
T. Mello, G. C. Hillhouse, and J. P. W. Diener
Phys. Rev. C 113, 064609 (2026) - Published 15 June, 2026
X. G. Deng (邓先概), Jin-Mei Wang (汪金梅), and Y. G. Ma (马余刚)
Phys. Rev. C 113, 064610 (2026) - Published 15 June, 2026
A. B. Larionov
Phys. Rev. C 113, 064611 (2026) - Published 15 June, 2026
N. Nhu Le, N. Ngoc Duy, and C. N. Phuoc Tai
Phys. Rev. C 113, 064612 (2026) - Published 15 June, 2026
G. R. Araujo et al. (MONUMENT Collaboration)
Phys. Rev. C 113, 064613 (2026) - Published 16 June, 2026
A. Sultana et al.
Phys. Rev. C 113, 064614 (2026) - Published 17 June, 2026
Anjali Merin, S. Nath, J. Gehlot, Gonika, Chandra Kumar, B. Ashna, K. V. Varsha, P. P. Panchami, Shiva Prasad Nayak, Alankar Singh, Rishabh Kumar, A. M. Vinodkumar, K. V. Jinu, S. Appannababu, K. Prameela, S. Ramakrishna Reddy, Sunil Kalkal, Rayees Ahmad Yatoo, P. Manju, and E. Prasad
Phys. Rev. C 113, 064615 (2026) - Published 17 June, 2026
C. Chang, L. Yang, C. J. Lin, W. D. Chen, Y. Y. Yang, P. W. Wen, T. P. Luo, D. Y. Pang, J. B. Ma, S. W. Xu, K. Wang, F. F. Duan, N. R. Ma, H. M. Jia, F. Yang, D. H. Huang, M. H. Zhang, G. Yang, Y. Yang, T. H. Mo, and D. X. Wang
Phys. Rev. C 113, 064616 (2026) - Published 17 June, 2026
Stefano Burrello, Carmelo Piazza, Rui Wang, and Maria Colonna
Phys. Rev. C 113, 064617 (2026) - Published 18 June, 2026
Jin Lei
Phys. Rev. C 113, 064618 (2026) - Published 22 June, 2026
Tiago Custódio, Francesca Gulminelli, Alex Rebillard-Soulié, Diego Gruyer, Rémi Bougault, Tuhin Malik, Helena Pais, and Constança Providência
Phys. Rev. C 113, 064619 (2026) - Published 22 June, 2026
M. Dondi et al. (FOOT Collaboration)
Phys. Rev. C 113, 064620 (2026) - Published 25 June, 2026
Arati Chavan, S. Rathi, K. Mahata, S. K. Pandit, V. V. Parkar, A. Shrivastava, K. Ramachandran, A. M. Moro, H. Liu, Jin Lei, Sangeeta Dhuri, Satbir Kaur, Prasanna M., and Vineet Kumar
Phys. Rev. C 113, 064621 (2026) - Published 25 June, 2026
S. Piantelli, A. Camaiani, G. Poggi, A. Ono, L. Baldesi, S. Barlini, B. Borderie, R. Bougault, G. Casini, C. Ciampi, Q. Fable, C. Frosin, J. A. Dueñas, D. Gruyer, B. Hong, A. Kordyasz, N. Le Neindre, T. Marchi, S. H. Nam, J. Park, M. Pârlog, G. Pasquali, S. Valdré, G. Verde, and E. Vient (FAZIA Collaboration)
Phys. Rev. C 113, 064622 (2026) - Published 26 June, 2026
Jingde Chen, Yuta Mukobara, Kazuki Fujio, Satoshi Chiba, Tatsuya Katabuchi, and Chikako Ishizuka
Phys. Rev. C 113, 064623 (2026) - Published 30 June, 2026
Jianing Li, Weiyao Ke, and Jin Hu
Phys. Rev. C 113, 064901 (2026) - Published 4 June, 2026
Jie Wan, Chun-Zheng Wang, Qi-Ye Shou, and Yu-Gang Ma
Phys. Rev. C 113, 064902 (2026) - Published 5 June, 2026
Craig S. Wright
Phys. Rev. C 113, 064903 (2026) - Published 8 June, 2026
Bijun Fan, Shusu Shi, Chao Zhang, and Liang Zheng
Phys. Rev. C 113, 064904 (2026) - Published 11 June, 2026
Claude Pruneau, Victor Gonzalez, Oveis Sheibani, Chun Shen, Yash Patley, Basanta Nandi, and Ana Marin
Phys. Rev. C 113, 064905 (2026) - Published 12 June, 2026
Yuri B. Ivanov
Phys. Rev. C 113, 064906 (2026) - Published 17 June, 2026
Liang Zhang (张良), Song Zhang (张松), Kai-Jia Sun (孙开佳), and Yu-Gang Ma (马余刚)
Phys. Rev. C 113, 064907 (2026) - Published 22 June, 2026
Guojun Wei, Hao Xu, Zhilong Li, Pengcheng Li, Qing Zhao, Yongjia Wang, and Qingfeng Li
Phys. Rev. C 113, 064908 (2026) - Published 23 June, 2026
Viktar Kireyeu, Vadim Voronyuk, Michael Winn, Susanne Gläßel, Jörg Aichelin, Christoph Blume, Elena Bratkovskaya, Gabriele Coci, and Jiaxing Zhao
Phys. Rev. C 113, 064909 (2026) - Published 26 June, 2026
Margaret E. Carrington and Stanisław Mrówczyński
Phys. Rev. C 113, 064910 (2026) - Published 29 June, 2026
Jun-Qi Tao, Xiang Fan, Yang Liu, Yu Sha, Kai Zhou, Hua Zheng, and Ben-Wei Zhang
Phys. Rev. C 113, 064911 (2026) - Published 29 June, 2026
Igor I. Strakovsky, William J. Briscoe, Philipp Gubler, Jackson R. Pybus, Axel Schmidt, and Alexander Somov
Phys. Rev. C 113, 065201 (2026) - Published 4 June, 2026
S. Prakhov et al. (A2 Collaboration)
Phys. Rev. C 113, 065202 (2026) - Published 5 June, 2026
P. Chatagnon et al. (CLAS Collaboration)
Phys. Rev. C 113, 065203 (2026) - Published 9 June, 2026
Ye Yan, Yuheng Wu, Yue Tan, Xiaohuang Hu, Qi Huang, Hongxia Huang, and Jialun Ping
Phys. Rev. C 113, 065204 (2026) - Published 17 June, 2026
Yu-Ying He and Xin-Jian Wen
Phys. Rev. C 113, 065205 (2026) - Published 29 June, 2026
S. Uthayakumaar, A. Spyrou, C. Harris, P. A. Denissenkov, D. Mücher, H. C. Berg, J. A. Clark, P. A. DeYoung, A. C. Dombos, B. Greaves, M. Guttormsen, F. Herwig, A. C. Larsen, S. N. Liddick, S. Lyons, J. Owens-Fryar, A. Palmisano-Kyle, G. Perdikakis, A. L. Richard, D. Santiago-Gonzalez, G. Savard, S. Siem, M. K. Smith, W. W. von Seeger, and M. Wiedeking
Phys. Rev. C 113, 065801 (2026) - Published 1 June, 2026
A key goal in nuclear astrophysics is explaining the abundance patterns of the elements in combination with observational astrophysical data and nuclear reaction networks. Although two nuclear reaction pathways—the slow ( process) and rapid ( process) neutron capture processes—are known to produce many heavy elements beyond iron, a process at intermediate neutron densities (the process) has been proposed. This process is an additional pathway that occurs in some stellar environments to explain observed elemental abundances. In this work, the authors utilized a Br beam that was implanted within a -ray total absorption spectrometer to produce the compound nucleus Kr through decay. The authors measured the constrained neutron radiative capture on Kr, showing that it plays an important role in the production of Rb in the conditions of the process. In addition, the results significantly reduce the uncertainty in the rate of this reaction by determining the -ray strength function in the compound nucleus Kr. This work demonstrates that reducing experimental uncertainties in a single neutron-capture reaction can significantly affect comparisons with theoretical predictions of element abundance patterns.
Gihwan Nam, Yeunhwan Lim, and Jeremy W. Holt
Phys. Rev. C 113, 065802 (2026) - Published 1 June, 2026
A. A. Valverde et al.
Phys. Rev. C 113, 065803 (2026) - Published 11 June, 2026
C. Boomershine, D. W. Bardayan, R. J. deBoer, P. D. O'Malley, S. R. Carmichael, L. Caves, A. Davis, A. Gula, K. Howard, R. Kelmar, A. Mitchell, L. Morales, S. Moylan, D. Robertson, and E. Stech
Phys. Rev. C 113, 065804 (2026) - Published 11 June, 2026
J. E. Alba-Arroyo, Daniel Pęcak, Michael McNeil Forbes, and Gabriel Wlazłowski
Phys. Rev. C 113, 065805 (2026) - Published 16 June, 2026
B. Greaves et al.
Phys. Rev. C 113, 065806 (2026) - Published 17 June, 2026
Nguyen Le Anh, Jasmine Sarahi Andrews, Bui Minh Loc, and Andre Sieverding
Phys. Rev. C 113, 065807 (2026) - Published 23 June, 2026
Joseph I. Kapusta
Phys. Rev. C 113, 069901 (2026) - Published 18 June, 2026
K. Neergård
Phys. Rev. C 113, 069902 (2026) - Published 25 June, 2026
R. Wada, Q. Hu, G. Y. Tian, X. Q. Liu, W. P. Lin, J. H. Tan, and H. Zheng
Phys. Rev. C 113, 069903 (2026) - Published 30 June, 2026