Optical potentials derived from nucleon-nucleon chiral potentials at
Matteo Vorabbi, Paolo Finelli, and Carlotta Giusti
Phys. Rev. C 96, 044001 (2017) - Published 25 October, 2017
R. Utama and J. Piekarewicz
Phys. Rev. C 96, 044308 (2017) - Published 6 October, 2017
The masses of nuclei between the experimentally known region and the neutron drip line are key inputs for a variety of astrophysical applications. Particularly near the drip lines, unstable nuclei are also at the core of fundamental questions about the limits of nuclear binding. The authors use two existing mass models that capture the essential underlying physics and then refine their predictions by training an artificial neural network. The results significantly reduce the root-mean-square deviation relative to experiment. These newly refined mass tables are used to map the neutron drip lines and to study a few critical -process nuclei.
Jia-Jing Lu (陆家靖), Zeng-Hua Li (李增花), Chong-Yang Chen (陈重阳), M. Baldo, and H.-J. Schulze
Phys. Rev. C 96, 044309 (2017) - Published 6 October, 2017
The accurate computation of nuclear matter properties, such as its binding energy, is still a challenge to nuclear theory, largely because the quark substructure of nucleons creates a strong repulsion at short distances that renders a straightforward perturbative calculation impossible. In this work, the authors study the Brueckner-Bethe-Goldstone expansion of dense Fermi systems in terms of hole-line contributions, of the associated Goldstone diagrams, to the binding energy of nuclear matter. They use various modern nucleon-nucleon potentials of high precision. In all cases the three-hole-line contributions are sufficiently small suggesting that the expansion converges. Yet, the empirical saturation properties of nuclear matter are not reproduced for any potential. This means that very strong nuclear three-body forces are required in order to achieve satisfactory saturation properties of nuclear matter, and that such forces are essential for all considered potentials.
Scott Pratt
Phys. Rev. C 96, 044903 (2017) - Published 12 October, 2017
As the hot and dense matter created in relativistic heavy-ion collisions expands and cools, theory must accurately treat its thermodynamic properties as well as its transport behavior. Because gradient terms probe the local environment within the evolving system, they are important in modeling the growth of thermal fluctuations, especially near a critical point, where knowledge of the size and spread of correlations is crucial. This paper demonstrates how gradient terms can be incorporated into the hydrodynamic equations of motion and how those modifications can be consistently applied to all thermodynamic quantities.
L. Adamczyk et al. (STAR Collaboration)
Phys. Rev. C 96, 044904 (2017) - Published 13 October, 2017
The beam-energy scan at RHIC aims to discover whether a critical point exists in the phase diagram of QCD. This paper reports on the most comprehensive measurement of single-particle spectra for a multitude of hadrons from the first run, taken with the STAR experiment. From these the authors infer the kinetic and chemical freeze-out temperatures and the baryon chemical potential as functions of beam energy and centrality. The results provide an opportunity for the beam-energy scan program at RHIC to enlarge the () region of the phase diagram to search for the QCD critical point.
S. A. Kuvin, A. H. Wuosmaa, C. J. Lister, M. L. Avila, C. R. Hoffman, B. P. Kay, D. G. McNeel, C. Morse, E. A. McCutchan, D. Santiago-Gonzalez, and J. R. Winkelbauer
Phys. Rev. C 96, 041301(R) (2017) - Published 3 October, 2017
R. P. de Groote, J. Billowes, C. L. Binnersley, M. L. Bissell, T. E. Cocolios, T. Day Goodacre, G. J. Farooq-Smith, D. V. Fedorov, K. T. Flanagan, S. Franchoo, R. F. Garcia Ruiz, Á. Koszorús, K. M. Lynch, G. Neyens, F. Nowacki, T. Otsuka, S. Rothe, H. H. Stroke, Y. Tsunoda, A. R. Vernon, K. D. A. Wendt, S. G. Wilkins, Z. Y. Xu, and X. F. Yang
Phys. Rev. C 96, 041302(R) (2017) - Published 4 October, 2017
Ronen Weiss and Nir Barnea
Phys. Rev. C 96, 041303(R) (2017) - Published 25 October, 2017
Kouhei Washiyama and Takashi Nakatsukasa
Phys. Rev. C 96, 041304(R) (2017) - Published 30 October, 2017
Kazuyuki Sekizawa
Phys. Rev. C 96, 041601(R) (2017) - Published 30 October, 2017
S. X. Nakamura, H. Kamano, and T. Ishikawa
Phys. Rev. C 96, 042201(R) (2017) - Published 26 October, 2017
K. P. Hickerson et al. (UCNA Collaboration)
Phys. Rev. C 96, 042501(R) (2017) - Published 30 October, 2017
Matteo Vorabbi, Paolo Finelli, and Carlotta Giusti
Phys. Rev. C 96, 044001 (2017) - Published 25 October, 2017
A. Göök, C. Eckardt, J. Enders, M. Freudenberger, A. Oberstedt, and S. Oberstedt
Phys. Rev. C 96, 044301 (2017) - Published 2 October, 2017
J. M. K. Slotte, P. Granholm, R. Öhman, T. Lönnroth, S. Juutinen, J. Suhonen, P. M. Jones, R. Julin, J. Pakarinen, P. Rahkila, C. Scholey, J. Sorri, and J. Uusitalo
Phys. Rev. C 96, 044302 (2017) - Published 3 October, 2017
E. Bauer, G. Garbarino, and C. A. Rodríguez Peña
Phys. Rev. C 96, 044303 (2017) - Published 5 October, 2017
M. Bouhelal, M. Labidi, F. Haas, and E. Caurier
Phys. Rev. C 96, 044304 (2017) - Published 5 October, 2017
D. Kocheva et al.
Phys. Rev. C 96, 044305 (2017) - Published 5 October, 2017
G. J. Fu, L. Y. Jia, Y. M. Zhao, and A. Arima
Phys. Rev. C 96, 044306 (2017) - Published 5 October, 2017
S. M. Wang (王思敏), N. Michel, W. Nazarewicz, and F. R. Xu (许甫荣)
Phys. Rev. C 96, 044307 (2017) - Published 5 October, 2017
R. Utama and J. Piekarewicz
Phys. Rev. C 96, 044308 (2017) - Published 6 October, 2017
The masses of nuclei between the experimentally known region and the neutron drip line are key inputs for a variety of astrophysical applications. Particularly near the drip lines, unstable nuclei are also at the core of fundamental questions about the limits of nuclear binding. The authors use two existing mass models that capture the essential underlying physics and then refine their predictions by training an artificial neural network. The results significantly reduce the root-mean-square deviation relative to experiment. These newly refined mass tables are used to map the neutron drip lines and to study a few critical -process nuclei.
Jia-Jing Lu (陆家靖), Zeng-Hua Li (李增花), Chong-Yang Chen (陈重阳), M. Baldo, and H.-J. Schulze
Phys. Rev. C 96, 044309 (2017) - Published 6 October, 2017
The accurate computation of nuclear matter properties, such as its binding energy, is still a challenge to nuclear theory, largely because the quark substructure of nucleons creates a strong repulsion at short distances that renders a straightforward perturbative calculation impossible. In this work, the authors study the Brueckner-Bethe-Goldstone expansion of dense Fermi systems in terms of hole-line contributions, of the associated Goldstone diagrams, to the binding energy of nuclear matter. They use various modern nucleon-nucleon potentials of high precision. In all cases the three-hole-line contributions are sufficiently small suggesting that the expansion converges. Yet, the empirical saturation properties of nuclear matter are not reproduced for any potential. This means that very strong nuclear three-body forces are required in order to achieve satisfactory saturation properties of nuclear matter, and that such forces are essential for all considered potentials.
G. G. Adamian, N. V. Antonenko, L. A. Malov, and H. Lenske
Phys. Rev. C 96, 044310 (2017) - Published 9 October, 2017
J. Park et al.
Phys. Rev. C 96, 044311 (2017) - Published 9 October, 2017
Ting-Ting Sun (孙亭亭), Wan-Li Lu (吕万里), and Shi-Sheng Zhang (张时声)
Phys. Rev. C 96, 044312 (2017) - Published 9 October, 2017
M. Queiser et al.
Phys. Rev. C 96, 044313 (2017) - Published 10 October, 2017
J. Piekarewicz
Phys. Rev. C 96, 044314 (2017) - Published 12 October, 2017
G. L. Wilson, M. Takeyama, A. N. Andreyev, B. Andel, S. Antalic, W. N. Catford, L. Ghys, H. Haba, F. P. Heßberger, M. Huang, D. Kaji, Z. Kalaninova, K. Morimoto, K. Morita, M. Murakami, K. Nishio, R. Orlandi, A. G. Smith, K. Tanaka, Y. Wakabayashi, and S. Yamaki
Phys. Rev. C 96, 044315 (2017) - Published 13 October, 2017
T. Shizuma, T. Hayakawa, I. Daito, H. Ohgaki, S. Miyamoto, and F. Minato
Phys. Rev. C 96, 044316 (2017) - Published 13 October, 2017
D. Torresi et al.
Phys. Rev. C 96, 044317 (2017) - Published 18 October, 2017
Hiroyuki Morita and Yoshiko Kanada-En'yo
Phys. Rev. C 96, 044318 (2017) - Published 18 October, 2017
Vladimir Zelevinsky, Naftali Auerbach, and Bui Minh Loc
Phys. Rev. C 96, 044319 (2017) - Published 19 October, 2017
F. Didierjean et al.
Phys. Rev. C 96, 044320 (2017) - Published 20 October, 2017
R. M. E. B. Kandegedara, G. Bollen, M. Eibach, N. D. Gamage, K. Gulyuz, C. Izzo, M. Redshaw, R. Ringle, R. Sandler, and A. A. Valverde
Phys. Rev. C 96, 044321 (2017) - Published 20 October, 2017
V. dos S. Ferreira, F. Krmpotić, C. A. Barbero, and A. R. Samana
Phys. Rev. C 96, 044322 (2017) - Published 23 October, 2017
D. Lascar et al.
Phys. Rev. C 96, 044323 (2017) - Published 23 October, 2017
G. J. Farooq-Smith, A. R. Vernon, J. Billowes, C. L. Binnersley, M. L. Bissell, T. E. Cocolios, T. Day Goodacre, R. P. de Groote, K. T. Flanagan, S. Franchoo, R. F. Garcia Ruiz, W. Gins, K. M. Lynch, B. A. Marsh, G. Neyens, S. Rothe, H. H. Stroke, S. G. Wilkins, and X. F. Yang
Phys. Rev. C 96, 044324 (2017) - Published 23 October, 2017
N. A. Althubiti et al. (ISOLTRAP Collaboration)
Phys. Rev. C 96, 044325 (2017) - Published 27 October, 2017
A. Giannatiempo
Phys. Rev. C 96, 044326 (2017) - Published 25 October, 2017
Tomohiro Oishi, Markus Kortelainen, and Alessandro Pastore
Phys. Rev. C 96, 044327 (2017) - Published 26 October, 2017
S. Lalkovski, E. A. Stefanova, S. Kisyov, A. Korichi, D. Bazzacco, M. Bergström, A. Görgen, B. Herskind, H. Hübel, A. Jansen, T. L. Khoo, T. Kutsarova, A. Lopez-Martens, A. Minkova, Zs. Podolyák, G. Schönwasser, and O. Yordanov
Phys. Rev. C 96, 044328 (2017) - Published 26 October, 2017
A. B. Garnsworthy, M. Bowry, B. Olaizola, J. D. Holt, S. R. Stroberg, S. Cruz, S. Georges, G. Hackman, A. D. MacLean, J. Measures, H. P. Patel, C. J. Pearson, and C. E. Svensson
Phys. Rev. C 96, 044329 (2017) - Published 26 October, 2017
P. Becker, D. Davesne, J. Meyer, J. Navarro, and A. Pastore
Phys. Rev. C 96, 044330 (2017) - Published 26 October, 2017
Niu Wan, Chang Xu, Zhongzhou Ren, and Jie Liu
Phys. Rev. C 96, 044331 (2017) - Published 27 October, 2017
B. Elman, A. Gade, D. Weisshaar, D. Barofsky, D. Bazin, P. C. Bender, M. Bowry, M. Hjorth-Jensen, K. W. Kemper, S. Lipschutz, E. Lunderberg, N. Sachmpazidi, N. Terpstra, W. B. Walters, A. Westerberg, S. J. Williams, and K. Wimmer
Phys. Rev. C 96, 044332 (2017) - Published 27 October, 2017
W. Urban et al.
Phys. Rev. C 96, 044333 (2017) - Published 30 October, 2017
Adam Freese, Daniel Puentes, Shankar Adhikari, Rafael Badui, Lei Guo, and Brian Raue
Phys. Rev. C 96, 044601 (2017) - Published 2 October, 2017
Basudeb Sahu and Swagatika Bhoi
Phys. Rev. C 96, 044602 (2017) - Published 2 October, 2017
M. J. Ermamatov, R. Linares, J. Lubian, J. L. Ferreira, F. Cappuzzello, D. Carbone, M. Cavallaro, M. Cubero, P. N. de Faria, A. Foti, G. Santagati, and V. A. B. Zagatto
Phys. Rev. C 96, 044603 (2017) - Published 4 October, 2017
I. Gheorghe, H. Utsunomiya, S. Katayama, D. Filipescu, S. Belyshev, K. Stopani, V. Orlin, V. Varlamov, T. Shima, S. Amano, S. Miyamoto, Y.-W. Lui, T. Kawano, and S. Goriely
Phys. Rev. C 96, 044604 (2017) - Published 6 October, 2017
Gao-Chan Yong
Phys. Rev. C 96, 044605 (2017) - Published 9 October, 2017
V. Varlamov, B. Ishkhanov, and V. Orlin
Phys. Rev. C 96, 044606 (2017) - Published 9 October, 2017
Sabyasachi Paul, C. Sunil, Sanjoy Pal, V. Nanal, V. Suman, G. S. Sahoo, A. Shanbhag, S. P. Tripathy, T. Bandyopadhyay, M. Nandy, and A. K. Mohanty
Phys. Rev. C 96, 044607 (2017) - Published 10 October, 2017
T. N. Nag, R. Tripathi, S. Sodaye, K. Sudarshan, K. Ramachandran, B. K. Nayak, and P. K. Pujari
Phys. Rev. C 96, 044608 (2017) - Published 11 October, 2017
Ashok Tiwari, C. Zhang, D.-M. Mei, and P. Cushman
Phys. Rev. C 96, 044609 (2017) - Published 12 October, 2017
V. Avrigeanu and M. Avrigeanu
Phys. Rev. C 96, 044610 (2017) - Published 16 October, 2017
H. Paşca, Sh. A. Kalandarov, G. G. Adamian, and N. V. Antonenko
Phys. Rev. C 96, 044611 (2017) - Published 16 October, 2017
B. Paes, G. Santagati, R. Magana Vsevolodovna, F. Cappuzzello, D. Carbone, E. N. Cardozo, M. Cavallaro, H. García-Tecocoatzi, A. Gargano, J. L. Ferreira, S. M. Lenzi, R. Linares, E. Santopinto, A. Vitturi, and J. Lubian
Phys. Rev. C 96, 044612 (2017) - Published 18 October, 2017
K. P. Santhosh and C. Nithya
Phys. Rev. C 96, 044613 (2017) - Published 18 October, 2017
Abhishek Yadav, Pushpendra P. Singh, Mohd. Shuaib, Vijay R. Sharma, Indu Bala, Unnati, Sunita Gupta, D. P. Singh, M. K. Sharma, R. Kumar, S. Murlithar, R. P. Singh, B. P. Singh, and R. Prasad
Phys. Rev. C 96, 044614 (2017) - Published 18 October, 2017
L. Yang (杨磊), C. J. Lin (林承键), H. M. Jia (贾会明), D. X. Wang (王东玺), N. R. Ma (马南茹), L. J. Sun (孙立杰), F. Yang (杨峰), X. X. Xu (徐新星), Z. D. Wu (吴振东), H. Q. Zhang (张焕乔), and Z. H. Liu (刘祖华)
Phys. Rev. C 96, 044615 (2017) - Published 18 October, 2017
S. K. Pandit, A. Shrivastava, K. Mahata, V. V. Parkar, R. Palit, N. Keeley, P. C. Rout, A. Kumar, K. Ramachandran, S. Bhattacharyya, V. Nanal, C. S. Palshetkar, T. N. Nag, Shilpi Gupta, S. Biswas, S. Saha, J. Sethi, P. Singh, A. Chatterjee, and S. Kailas
Phys. Rev. C 96, 044616 (2017) - Published 19 October, 2017
Junhua Luo, Li Jiang, and Suyuan Li
Phys. Rev. C 96, 044617 (2017) - Published 23 October, 2017
Yin Xia, Jun Xu, Bao-An Li, and Wen-Qing Shen
Phys. Rev. C 96, 044618 (2017) - Published 23 October, 2017
B. Nedaee-Shakarab, M. Saadati-Niari, and F. Zolfagharpour
Phys. Rev. C 96, 044619 (2017) - Published 24 October, 2017
Zhimin Wang, Huaiyong Bai, Luyu Zhang, Haoyu Jiang, Yi Lu, Jinxiang Chen, Guohui Zhang, Yu. M. Gledenov, M. V. Sedysheva, and G. Khuukhenkhuu
Phys. Rev. C 96, 044620 (2017) - Published 24 October, 2017
Zhimin Wang, Huaiyong Bai, Luyu Zhang, Haoyu Jiang, Yi Lu, Jinxiang Chen, Guohui Zhang, Yu. M. Gledenov, M. V. Sedysheva, and G. Khuukhenkhuu
Phys. Rev. C 96, 044621 (2017) - Published 24 October, 2017
S. Q. Guo, Y. Gao, J. Q. Li, and H. F. Zhang
Phys. Rev. C 96, 044622 (2017) - Published 26 October, 2017
Krishichayan, M. Bhike, W. Tornow, A. P. Tonchev, and T. Kawano
Phys. Rev. C 96, 044623 (2017) - Published 26 October, 2017
Deepak Kumar and Moumita Maiti
Phys. Rev. C 96, 044624 (2017) - Published 30 October, 2017
Nachiketa Sarkar and Premomoy Ghosh
Phys. Rev. C 96, 044901 (2017) - Published 6 October, 2017
Akihiko Monnai and Jean-Yves Ollitrault
Phys. Rev. C 96, 044902 (2017) - Published 11 October, 2017
Scott Pratt
Phys. Rev. C 96, 044903 (2017) - Published 12 October, 2017
As the hot and dense matter created in relativistic heavy-ion collisions expands and cools, theory must accurately treat its thermodynamic properties as well as its transport behavior. Because gradient terms probe the local environment within the evolving system, they are important in modeling the growth of thermal fluctuations, especially near a critical point, where knowledge of the size and spread of correlations is crucial. This paper demonstrates how gradient terms can be incorporated into the hydrodynamic equations of motion and how those modifications can be consistently applied to all thermodynamic quantities.
L. Adamczyk et al. (STAR Collaboration)
Phys. Rev. C 96, 044904 (2017) - Published 13 October, 2017
The beam-energy scan at RHIC aims to discover whether a critical point exists in the phase diagram of QCD. This paper reports on the most comprehensive measurement of single-particle spectra for a multitude of hadrons from the first run, taken with the STAR experiment. From these the authors infer the kinetic and chemical freeze-out temperatures and the baryon chemical potential as functions of beam energy and centrality. The results provide an opportunity for the beam-energy scan program at RHIC to enlarge the () region of the phase diagram to search for the QCD critical point.
Francesco Scardina, Santosh K. Das, Vincenzo Minissale, Salvatore Plumari, and Vincenzo Greco
Phys. Rev. C 96, 044905 (2017) - Published 17 October, 2017
Yufu Lin, Lizhu Chen, and Zhiming Li
Phys. Rev. C 96, 044906 (2017) - Published 17 October, 2017
Chun-Jian Zhang and Jun Xu
Phys. Rev. C 96, 044907 (2017) - Published 18 October, 2017
P. Garg and D. K. Mishra
Phys. Rev. C 96, 044908 (2017) - Published 20 October, 2017
Zack Wolff and Denes Molnar
Phys. Rev. C 96, 044909 (2017) - Published 23 October, 2017
Mubarak Alqahtani, Mohammad Nopoush, Radoslaw Ryblewski, and Michael Strickland
Phys. Rev. C 96, 044910 (2017) - Published 23 October, 2017
L. E. Finch and S. J. Murray
Phys. Rev. C 96, 044911 (2017) - Published 23 October, 2017
Weiyao Ke, J. Scott Moreland, Jonah E. Bernhard, and Steffen A. Bass
Phys. Rev. C 96, 044912 (2017) - Published 25 October, 2017
E. Kurban and M. C. Güçlü
Phys. Rev. C 96, 044913 (2017) - Published 25 October, 2017
Yao Zhang, Jingbo Zhang, Tong Chen, Desheng Liu, and Yun Chao
Phys. Rev. C 96, 044914 (2017) - Published 25 October, 2017
Martin Cleven, Volodymyr K. Magas, and Angels Ramos
Phys. Rev. C 96, 045201 (2017) - Published 10 October, 2017
Volodymyr Vovchenko, Anton Motornenko, Paolo Alba, Mark I. Gorenstein, Leonid M. Satarov, and Horst Stoecker
Phys. Rev. C 96, 045202 (2017) - Published 10 October, 2017
Li-Hua Song and Lin-Wan Yan
Phys. Rev. C 96, 045203 (2017) - Published 12 October, 2017
Tsubasa Hoshino, Shota Ohnishi, Wataru Horiuchi, Tetsuo Hyodo, and Wolfram Weise
Phys. Rev. C 96, 045204 (2017) - Published 16 October, 2017
Juan M. Torres-Rincon and Joerg Aichelin
Phys. Rev. C 96, 045205 (2017) - Published 20 October, 2017
Yu Ninomiya, Wolfgang Bentz, and Ian C. Cloët
Phys. Rev. C 96, 045206 (2017) - Published 24 October, 2017
Joanna E. Sobczyk
Phys. Rev. C 96, 045501 (2017) - Published 26 October, 2017
M. R. Dunlop et al.
Phys. Rev. C 96, 045502 (2017) - Published 30 October, 2017
J. J. He, A. Parikh, Y. Xu, Y. H. Zhang, X. H. Zhou, and H. S. Xu
Phys. Rev. C 96, 045801 (2017) - Published 2 October, 2017
M. E. Mosquera and O. Civitarese
Phys. Rev. C 96, 045802 (2017) - Published 6 October, 2017
Débora P. Menezes and Constança Providência
Phys. Rev. C 96, 045803 (2017) - Published 9 October, 2017
X. Fang, W. P. Tan, M. Beard, R. J. deBoer, G. Gilardy, H. Jung, Q. Liu, S. Lyons, D. Robertson, K. Setoodehnia, C. Seymour, E. Stech, B. Vande Kolk, M. Wiescher, R. T. deSouza, S. Hudan, V. Singh, X. D. Tang, and E. Uberseder
Phys. Rev. C 96, 045804 (2017) - Published 9 October, 2017
N. Özkan, R. T. Güray, C. Yalçın, W. P. Tan, A. Aprahamian, M. Beard, R. J. deBoer, S. Almaraz-Calderon, S. Falahat, J. Görres, Q. Li, A. Sauerwein, K. Sonnabend, M. Wiescher, Zs. Fülöp, Gy. Gyürky, E. Somorjai, and J. Greene
Phys. Rev. C 96, 045805 (2017) - Published 10 October, 2017
Miguel Marques, Micaela Oertel, Matthias Hempel, and Jérôme Novak
Phys. Rev. C 96, 045806 (2017) - Published 10 October, 2017
A. Grassi, G. Mangano, L. E. Marcucci, and O. Pisanti
Phys. Rev. C 96, 045807 (2017) - Published 12 October, 2017
Peter Mohr
Phys. Rev. C 96, 045808 (2017) - Published 13 October, 2017
D. E. Alvarez-Castillo and D. B. Blaschke
Phys. Rev. C 96, 045809 (2017) - Published 18 October, 2017
G. Quintero Angulo, A. Pérez Martínez, and H. Pérez Rojas
Phys. Rev. C 96, 045810 (2017) - Published 19 October, 2017
A. M. Mukhamedzhanov and G. V. Rogachev
Phys. Rev. C 96, 045811 (2017) - Published 19 October, 2017
S. A. Kuvin, J. Belarge, L. T. Baby, J. Baker, I. Wiedenhöver, P. Höflich, A. Volya, J. C. Blackmon, C. M. Deibel, H. E. Gardiner, J. Lai, L. E. Linhardt, K. T. Macon, B. C. Rasco, N. Quails, K. Colbert, D. L. Gay, and N. Keeley
Phys. Rev. C 96, 045812 (2017) - Published 27 October, 2017
J. Park et al.
Phys. Rev. C 96, 049901 (2017) - Published 19 October, 2017
S. Goudarzi and H. R. Moshfegh
Phys. Rev. C 96, 049902 (2017) - Published 26 October, 2017