Renormalization of a finite-range inverse-cube potential
D. Odell, A. Deltuva, J. Bonilla, and L. Platter
Phys. Rev. C 100, 054001 (2019) - Published 4 November, 2019
Jing Geng (耿晶), Jia Jie Li (李佳杰), Wen Hui Long (龙文辉), Yi Fei Niu (牛一斐), and Shi Yao Chang (常士尧)
Phys. Rev. C 100, 051301(R) (2019) - Published 4 November, 2019
Relativistic mean-field calculations (pure Hartree calculations) have problems reproducing the single-particle energies for some pseudo-spin doublets (orbits with , , and , , ) and can lead to incorrect magic numbers. The authors show how this can be corrected in a relativistic Hartree-Fock calculation. In particular, the -tensor coupling plays an important role. The results provide qualitative guidance for treating the delicate balance between attractive and repulsive interactions in the dynamic nuclear medium.
Junjie Yang, Jesse A. Hernandez, and J. Piekarewicz
Phys. Rev. C 100, 054301 (2019) - Published 1 November, 2019
The weak nuclear force is a crucial probe of both fundamental physics and nuclear structure. This paper reviews the idea of using precision electroweak probes to measure the neutron skin of nuclei. This, in turn, is used to tune parameters in density functional theory not otherwise tightly constrained in finite nuclei—but which have a critical impact on the equation of state for neutron stars.
A. S. Schneider, L. F. Roberts, C. D. Ott, and E. O'Connor
Phys. Rev. C 100, 055802 (2019) - Published 7 November, 2019
Stars heavier than several times the mass of the Sun undergo a core-collapse event at the end of their lives. The dynamics of this process, which may lead to a supernova explosion, is mainly determined by the equation of state of dense matter, which also determines whether the collapse gives birth to a neutron star or a black hole. Whereas it is relatively well understood how the properties of neutron stars are affected by variations in the nuclear equation of state, the authors probe the rather unexplored effects of such variations on supernova dynamics and their neutrino signals. The authors demonstrate that the core collapse is mainly affected by changes in the nucleon effective masses which, within the Skyrme model employed, control the yet poorly constrained finite temperature dependence of the equation of state.
Jing Geng (耿晶), Jia Jie Li (李佳杰), Wen Hui Long (龙文辉), Yi Fei Niu (牛一斐), and Shi Yao Chang (常士尧)
Phys. Rev. C 100, 051301(R) (2019) - Published 4 November, 2019
Relativistic mean-field calculations (pure Hartree calculations) have problems reproducing the single-particle energies for some pseudo-spin doublets (orbits with , , and , , ) and can lead to incorrect magic numbers. The authors show how this can be corrected in a relativistic Hartree-Fock calculation. In particular, the -tensor coupling plays an important role. The results provide qualitative guidance for treating the delicate balance between attractive and repulsive interactions in the dynamic nuclear medium.
Sam Bailey, Tzany Kokalova, Martin Freer, Carl Wheldon, Robin Smith, Joseph Walshe, Neil Curtis, Neven Soić, Lovro Prepolec, Vedrana Tokić, Francisco Miguel Marqués, Lynda Achouri, Franck Delaunay, Quentin Deshayes, Marian Parlog, Beatriz Fernández-Dominguez, Bertrand Jacquot, and Asim Soylu
Phys. Rev. C 100, 051302(R) (2019) - Published 15 November, 2019
X. Xu et al.
Phys. Rev. C 100, 051303(R) (2019) - Published 27 November, 2019
Andrei V. Afanasev, D. V. Karlovets, and V. G. Serbo
Phys. Rev. C 100, 051601(R) (2019) - Published 25 November, 2019
Partha Pratim Bhaduri, Nicolas Borghini, Amaresh Jaiswal, and Michael Strickland
Phys. Rev. C 100, 051901(R) (2019) - Published 12 November, 2019
Adam Bzdak and Volker Koch
Phys. Rev. C 100, 051902(R) (2019) - Published 15 November, 2019
S. Adhikari et al. (The GlueX Collaboration)
Phys. Rev. C 100, 052201(R) (2019) - Published 27 November, 2019
D. Odell, A. Deltuva, J. Bonilla, and L. Platter
Phys. Rev. C 100, 054001 (2019) - Published 4 November, 2019
Junjie Yang, Jesse A. Hernandez, and J. Piekarewicz
Phys. Rev. C 100, 054301 (2019) - Published 1 November, 2019
The weak nuclear force is a crucial probe of both fundamental physics and nuclear structure. This paper reviews the idea of using precision electroweak probes to measure the neutron skin of nuclei. This, in turn, is used to tune parameters in density functional theory not otherwise tightly constrained in finite nuclei—but which have a critical impact on the equation of state for neutron stars.
Masayuki Yamagami
Phys. Rev. C 100, 054302 (2019) - Published 4 November, 2019
W. Zhang (张炜) and S. Q. Zhang (张双全)
Phys. Rev. C 100, 054303 (2019) - Published 4 November, 2019
Zhao-Wen Zhang and Lie-Wen Chen
Phys. Rev. C 100, 054304 (2019) - Published 4 November, 2019
P. Sarriguren
Phys. Rev. C 100, 054306 (2019) - Published 6 November, 2019
Benjamin K. Luna and T. Papenbrock
Phys. Rev. C 100, 054307 (2019) - Published 6 November, 2019
F. S. Babra, R. Palit, S. Rajbanshi, S. Jehangir, B. Das, G. H. Bhat, J. A. Sheikh, S. Biswas, U. Garg, Md. S. R. Laskar, C. Palshetkar, S. Saha, J. Sethi, and P. Singh
Phys. Rev. C 100, 054308 (2019) - Published 7 November, 2019
C. Liu (刘晨) et al.
Phys. Rev. C 100, 054309 (2019) - Published 7 November, 2019
Z. M. Niu (牛中明), J. Y. Fang (方基宇), and Y. F. Niu (牛一斐)
Phys. Rev. C 100, 054311 (2019) - Published 8 November, 2019
M. Bhuyan, B. V. Carlson, S. K. Patra, and Raj K. Gupta
Phys. Rev. C 100, 054312 (2019) - Published 8 November, 2019
J. G. Li, N. Michel, B. S. Hu, W. Zuo, and F. R. Xu
Phys. Rev. C 100, 054313 (2019) - Published 11 November, 2019
Shen Yang (杨申), Bo Nan Zhang (张博楠), and Bao Yuan Sun (孙保元)
Phys. Rev. C 100, 054314 (2019) - Published 11 November, 2019
Y. Y. Zong, M. Q. Lin, M. Bao, Y. M. Zhao, and A. Arima
Phys. Rev. C 100, 054315 (2019) - Published 12 November, 2019
E. V. Tkalya
Phys. Rev. C 100, 054316 (2019) - Published 12 November, 2019
A. Goldkuhle et al. (AGATA Collaboration)
Phys. Rev. C 100, 054317 (2019) - Published 18 November, 2019
C. M. Petrache et al.
Phys. Rev. C 100, 054319 (2019) - Published 15 November, 2019
R. Schwengner and G. Rusev
Phys. Rev. C 100, 054320 (2019) - Published 18 November, 2019
S. Cruz et al.
Phys. Rev. C 100, 054321 (2019) - Published 18 November, 2019
T. Furuno, T. Kawabata, S. Adachi, Y. Ayyad, Y. Kanada-En'yo, Y. Fujikawa, K. Inaba, M. Murata, H. J. Ong, M. Sferrazza, Y. Takahashi, T. Takeda, I. Tanihata, D. T. Tran, and M. Tsumura
Phys. Rev. C 100, 054322 (2019) - Published 19 November, 2019
L. Hayen, J. Kostensalo, N. Severijns, and J. Suhonen
Phys. Rev. C 100, 054323 (2019) - Published 20 November, 2019
Li-Gang Cao, Shi-Sheng Zhang, and H. Sagawa
Phys. Rev. C 100, 054324 (2019) - Published 20 November, 2019
Z. X. Yang, X. L. Shang, G. C. Yong, W. Zuo, and Y. Gao
Phys. Rev. C 100, 054325 (2019) - Published 21 November, 2019
W. G. Jiang, G. Hagen, and T. Papenbrock
Phys. Rev. C 100, 054326 (2019) - Published 21 November, 2019
J. L. Pore et al.
Phys. Rev. C 100, 054327 (2019) - Published 25 November, 2019
H. T. Fortune
Phys. Rev. C 100, 054328 (2019) - Published 22 November, 2019
N. A. Smirnova, B. R. Barrett, Y. Kim, I. J. Shin, A. M. Shirokov, E. Dikmen, P. Maris, and J. P. Vary
Phys. Rev. C 100, 054329 (2019) - Published 26 November, 2019
M. Matejska-Minda et al.
Phys. Rev. C 100, 054330 (2019) - Published 26 November, 2019
J. Wiśniewski, W. Urban, M. Czerwiński, J. Kurpeta, A. Płochocki, M. Pomorski, T. Rząca-Urban, K. Sieja, L. Canete, T. Eronen, S. Geldhof, A. Jokinen, A. Kankainen, I. D. Moore, D. A. Nesterenko, H. Penttilä, I. Pohjalainen, S. Rinta-Antila, A. de Roubin, and M. Vilén
Phys. Rev. C 100, 054331 (2019) - Published 26 November, 2019
B. A. Brown, B. Blank, and J. Giovinazzo
Phys. Rev. C 100, 054332 (2019) - Published 26 November, 2019
M. Vilén, A. Kankainen, P. Bączyk, L. Canete, J. Dobaczewski, T. Eronen, S. Geldhof, A. Jokinen, M. Konieczka, J. Kostensalo, I. D. Moore, D. A. Nesterenko, H. Penttilä, I. Pohjalainen, M. Reponen, S. Rinta-Antila, A. de Roubin, W. Satuła, and J. Suhonen
Phys. Rev. C 100, 054333 (2019) - Published 26 November, 2019
S. N. Fedotkin, A. G. Magner, and M. I. Gorenstein
Phys. Rev. C 100, 054334 (2019) - Published 26 November, 2019
Jia-Jing Lu (陆家靖), Zeng-Hua Li (李增花), G. F. Burgio, A. Figura, and H.-J. Schulze
Phys. Rev. C 100, 054335 (2019) - Published 27 November, 2019
G. S. Li, J. G. Wang, J. Lubian, H. O. Soler, Y. D. Fang, M. L. Liu, N. T. Zhang, X. H. Zhou, Y. H. Zhang, B. S. Gao, Y. H. Qiang, S. Guo, S. C. Wang, K. L. Wang, K. K. Zheng, R. Li, and Y. Zheng
Phys. Rev. C 100, 054601 (2019) - Published 5 November, 2019
R. J. Peterson
Phys. Rev. C 100, 054602 (2019) - Published 6 November, 2019
Ibrahim Ulgen, Bulent Yilmaz, and Denis Lacroix
Phys. Rev. C 100, 054603 (2019) - Published 6 November, 2019
Pankaj K. Giri, Amritraj Mahato, D. Singh, Sneha B. Linda, Harish Kumar, Suhail A. Tali, M. Afzal Ansari, R. Kumar, S. Muralithar, and R. P. Singh
Phys. Rev. C 100, 054604 (2019) - Published 11 November, 2019
Xuwei Sun, Jing Chen, and Dinghui Lu
Phys. Rev. C 100, 054605 (2019) - Published 11 November, 2019
M. Murphy et al. (The Jefferson Lab Hall A Collaboration)
Phys. Rev. C 100, 054606 (2019) - Published 11 November, 2019
C. Hebborn and P. Capel
Phys. Rev. C 100, 054607 (2019) - Published 12 November, 2019
E. Crema, B. Paes, V. A. B. Zagatto, J. F. P. Huiza, J. Lubian, J. M. B. Shorto, R. F. Simões, D. S. Monteiro, N. Added, M. C. Morais, and P. R. S. Gomes
Phys. Rev. C 100, 054608 (2019) - Published 14 November, 2019
K. Yue, J. T. Zhang, X. L. Tu, C. J. Shao, H. X. Li, P. Ma, B. Mei, X. C. Chen, Y. Y. Yang, X. Q. Liu, Y. M. Xing, K. H. Fang, X. H. Li, Z. Y. Sun, M. Wang, P. Egelhof, Yu. A. Litvinov, K. Blaum, Y. H. Zhang, and X. H. Zhou
Phys. Rev. C 100, 054609 (2019) - Published 14 November, 2019
A. E. Lovell, I. Stetcu, P. Talou, G. Rusev, and M. Jandel
Phys. Rev. C 100, 054610 (2019) - Published 15 November, 2019
C. Karthika and M. Balasubramaniam
Phys. Rev. C 100, 054611 (2019) - Published 15 November, 2019
K. Godbey, Lu Guo (郭璐), and A. S. Umar
Phys. Rev. C 100, 054612 (2019) - Published 18 November, 2019
Ramandeep Gandhi, B. K. Nayak, S. V. Suryanarayana, A. Pal, G. Mohanto, S. De, A. Parihari, A. Kundu, P. C. Rout, S. Santra, K. Mahata, B. Srinivasan, E. T. Mirgule, and J. Pandey
Phys. Rev. C 100, 054613 (2019) - Published 18 November, 2019
P. Napolitani, A. Sainte-Marie, and M. Colonna
Phys. Rev. C 100, 054614 (2019) - Published 19 November, 2019
Nguyen Tri Toan Phuc, R. S. Mackintosh, Nguyen Hoang Phuc, and Dao T. Khoa
Phys. Rev. C 100, 054615 (2019) - Published 18 November, 2019
Shu Qing Guo, Xiao Jun Bao, Hong Fei Zhang, Jun Qing Li, and Nan Wang
Phys. Rev. C 100, 054616 (2019) - Published 19 November, 2019
Oleksandra Panova, Anton Motornenko, Mark I. Gorenstein, Jan Steinheimer, and Horst Stoecker
Phys. Rev. C 100, 054617 (2019) - Published 20 November, 2019
J. Hooker, G. V. Rogachev, E. Koshchiy, S. Ahn, M. Barbui, V. Z. Goldberg, C. Hunt, H. Jayatissa, E. C. Pollacco, B. T. Roeder, A. Saastamoinen, and S. Upadhyayula
Phys. Rev. C 100, 054618 (2019) - Published 21 November, 2019
B. Mei
Phys. Rev. C 100, 054619 (2019) - Published 25 November, 2019
Jan Ryckebusch, Wim Cosyn, Tom Vieijra, and Corneel Casert
Phys. Rev. C 100, 054620 (2019) - Published 25 November, 2019
Kayman J. Gonçalves, Andre V. Giannini, David D. Chinellato, and Giorgio Torrieri
Phys. Rev. C 100, 054901 (2019) - Published 4 November, 2019
Yasushi Nara and Horst Stoecker
Phys. Rev. C 100, 054902 (2019) - Published 5 November, 2019
Kishora Nayak, Shusu Shi, Nu Xu, and Zi-Wei Lin
Phys. Rev. C 100, 054903 (2019) - Published 7 November, 2019
R. V. Poberezhnyuk, V. Vovchenko, A. Motornenko, M. I. Gorenstein, and H. Stöcker
Phys. Rev. C 100, 054904 (2019) - Published 12 November, 2019
Fernando G. Gardim, Frédérique Grassi, Pedro Ishida, Matthew Luzum, and Jean-Yves Ollitrault
Phys. Rev. C 100, 054905 (2019) - Published 14 November, 2019
Volodymyr Vovchenko, Benjamin Dönigus, and Horst Stoecker
Phys. Rev. C 100, 054906 (2019) - Published 25 November, 2019
Wojciech Florkowski, Avdhesh Kumar, Aleksas Mazeliauskas, and Radoslaw Ryblewski
Phys. Rev. C 100, 054907 (2019) - Published 25 November, 2019
Aaron Park and Su Houng Lee
Phys. Rev. C 100, 055201 (2019) - Published 4 November, 2019
N. Muramatsu et al. (LEPS2/BGOegg Collaboration)
Phys. Rev. C 100, 055202 (2019) - Published 8 November, 2019
H. Osmanović, M. Hadžimehmedović, R. Omerović, J. Stahov, M. Gorchtein, V. Kashevarov, K. Nikonov, M. Ostrick, L. Tiator, and A. Švarc
Phys. Rev. C 100, 055203 (2019) - Published 21 November, 2019
Nodoka Yamanaka, Taiichi Yamada, and Yasuro Funaki
Phys. Rev. C 100, 055501 (2019) - Published 4 November, 2019
Hilla De-Leon, Lucas Platter, and Doron Gazit
Phys. Rev. C 100, 055502 (2019) - Published 13 November, 2019
N. Van Dessel, N. Jachowicz, and A. Nikolakopoulos
Phys. Rev. C 100, 055503 (2019) - Published 19 November, 2019
V. Cirigliano, W. Dekens, J. de Vries, M. L. Graesser, E. Mereghetti, S. Pastore, M. Piarulli, U. van Kolck, and R. B. Wiringa
Phys. Rev. C 100, 055504 (2019) - Published 25 November, 2019
Spencer Beloin, Sophia Han, Andrew W. Steiner, and Khorgolkhuu Odbadrakh
Phys. Rev. C 100, 055801 (2019) - Published 5 November, 2019
A. S. Schneider, L. F. Roberts, C. D. Ott, and E. O'Connor
Phys. Rev. C 100, 055802 (2019) - Published 7 November, 2019
Stars heavier than several times the mass of the Sun undergo a core-collapse event at the end of their lives. The dynamics of this process, which may lead to a supernova explosion, is mainly determined by the equation of state of dense matter, which also determines whether the collapse gives birth to a neutron star or a black hole. Whereas it is relatively well understood how the properties of neutron stars are affected by variations in the nuclear equation of state, the authors probe the rather unexplored effects of such variations on supernova dynamics and their neutrino signals. The authors demonstrate that the core collapse is mainly affected by changes in the nucleon effective masses which, within the Skyrme model employed, control the yet poorly constrained finite temperature dependence of the equation of state.
Thomas Carreau, Francesca Gulminelli, and Jérôme Margueron
Phys. Rev. C 100, 055803 (2019) - Published 11 November, 2019
R. Rizaldy, A. R. Alfarasyi, A. Sulaksono, and T. Sumaryada
Phys. Rev. C 100, 055804 (2019) - Published 26 November, 2019