Abstract
We report a new microscopic equation of state (EoS) of pure neutron matter (PNM) at zero temperature using the recent realistic two-body interaction derived in the framework of chiral perturbation theory (ChPT). The EoS is derived using the Brueckner–Bethe–Goldstone quantum many-body theory in the Brueckner–Hartree–Fock approach. We have calculated the EoS of PNM at low and high densities using LO, NLO, N\(^{2}\)LO, N\(^{3}\)LO, N\(^{4}\)LO potentials at three different values of the momentum-space cut-off \(\Lambda \) = 450, 500 and 550 MeV. It is found that the EoS is not much affected by the cut-off variations at low densities. Also the binding energy of PNM has been computed within the framework of the Brueckner–Hartree–Fock (BHF) approach plus two-body density-dependent Skyrme potential which is equivalent to three-body forces. The effect of the two-body density-dependent Skyrme potential is to produce a stiffer EoS. This is actually needed to improve the saturation point of symmetric nuclear matter obtained using the two-body NN interaction. The results of several microscopic approaches are compared. It is found that the EoS is sensitive to the momentum-space cut-off \(\Lambda \). Also the partial wave contributions to potential energy at the empirical saturation density \(\rho = 0.16\) fm\(^{-3}\) for different potentials are listed from \(^{1}S_{0}\) to \(^{3}F_{3}\) states. It is found that all contributions are nearly cut-off independent except the ones from \(^{3}P_{1}\), \(^{3}P_{2}, ^{3}\!H_{4}\) and \(^{3}F_{4}\) states, which are increasing with the cut-off \(\Lambda \). Actually, the size of these contributions is strongly dependent on the central and tensor components in the NN potential. The larger cut-off \(\Lambda \) corresponds to harder interactions and gives more repulsive contribution to the NN potential at short distance. It leads to smaller binding energy.
Similar content being viewed by others
References
P Demorest, T Pennucci, S Ransom, M Roberts and J Hessels, Nature 467, 1081 (2010)
J Antoniadis et al, Science 340, 6131 (2013)
R Oechslin, H T Janka and A Marek, Astron. Astrophys. 467, 395 (2007)
R Oechslin and H T Janka, Phys. Rev. Lett. 99, 121102 (2007)
Y I Shin, C H Schunck, A Schirotzek and W Ketterle, Nature 689, 451 (2008)
M J H Ku, A T Sommer, L W Cheuk and M W Zwierlein, Science 563, 335 (2012)
Y LeCun, Y Begio and G E Hinton, Nature 521, 436 (2015)
D Kasen, B Metzger, J Barnes, E Quataert and E Ramirez-Ruiz, Nature 551, 80 (2017)
LIGO Scientific, Virgo: B P Abbott et al, Phys. Rev. Lett. 121, 161101 (2018)
E Annala, T Gorda, A Kurkela and A Vuorinen, Phys. Rev. Lett. 120, 172703 (2018)
I Bombaci and D Logoteta, Astron. Astrophys. 609, A128 (2018)
Y Fujimoto, K Fukushima and K Murase, Phys. Rev. D 101, 054016 (2020)
J M Lattimer and M Prakash, Astrophys. J. 550, 426 (2001)
J M Lattimer and M Prakash, Science 304, 536 (2004)
J M Lattimer and M Prakash, Phys. Rep. 442, 109 (2007)
F J Fattoyev, W G Newton, J Xu and B-A Li, Phys. Rev. C 86, 025804 (2012)
T Krüger, I Tews, B Friman, K Hebeler and A Schwenk, Phys. Lett. B 726, 412 (2013)
T Krüger, I Tews, K Hebeler and A Schwenk, Phys. Rev. C 88, 025802 (2013)
J M Dong, U Lombardo and W Zuo, Phys. Rev. C 87, 062801(R) (2013)
I Tews, T Krueger, K Hebeler and A Schwenk, Phys. Rev. Lett. 110, 032504 (2013)
I Tews, T Krüger, A Gezerlis, K Hebeler and A Schwenk, Proceedings of the International Conference on Nuclear Theory in the Supercomputing Era 2013 (Iowa State University, May 13–17, 2013)
H Heiselberg and M Hjorth-Jensen, Phys. Rep. 328, 237 (2000)
N K Glendenning, Phys. Rep. 342, 393 (2001)
M Baldo, I Bombaci and G F Burgio, Astron. Astrophys. 328, 274 (1997)
R Schiavilla, V R Pandharipande and R B Wiringa, Nucl. Phys. A 449, 219 (1986)
J Carlson, R R Pandharipande and R B Wiringa, Nucl. Phys. A 401, 59 (1983)
R Machleidt and D R Entem, Phys. Rep. 503, 1 (2011)
E Marji, A Canul, Q Macpherson, R Winzer, Ch Zeoli, D R Entem and R Machleidt, Phys. Rev. C 88, 054002 (2013)
F Sammarruca, R Machleidt and N Kaiser, Phys. Rev. C 92, 054327 (2015)
D R Entem, R Machleidt and Y Nosyk, Phys. Rev. C 96, 024004 (2017)
F Sammarruca, L E Marcucci, L Coraggio, J W Holt, N Itaco and R Macheidt, arXiv:1807.06640v1
M Hoferichter, J Ruiz, de Elvira, B Kubis and U-G Meissner, Phys. Rev. Lett. 115, 192301 (2015); Phys. Rep. 625, 1 (2016)
J P Jeukenne, A Lejeune and C Mahaux, Phys. Rev. C 10, 1391 (1974)
H Q Song, M Baldo, G Giansiracusa and U Lombardo, Phys. Rev. Lett. 81, 1584 (1998)
Kh Gad, Eur. Phys. J. A 22, 405 (2004)
K Gad, Nucl. Phys. A 747, 655 (2005)
K Gad, J. Phys. G 32, 799 (2006)
K Gad and K S A Hassaneen, Nucl. Phys. A 793, 67 (2007)
K Hassaneen and K Gad, J. Phys. Soc. Jpn. 77, 084201 (2008)
P Gögelein, E N E Van Dalen, K Gad, K S A Hassaneen and H Müther, Phys. Rev. C 79, 024308 (2009)
H Mansour, K Gad and K S A Hassaneen, Prog. Theor. Phys. 123, 687 (2010)
K Gad, Ann. Phys. 326, 2474 (2011)
K Gad, Ann. Phys. 327, 2403 (2012)
F Coester, S Cohen, B D Day and C M Vincent, Phys. Rev. C 1, 769 (1970)
S Gandolfi, A Gezerlis and J Carlson, Annu. Rev. Nucl. Part. Sci. 65, 303 (2015)
T H R Skyrme, Nucl. Phys. 9, 615 (1959]
D Vautherin and D M Brink, Phys. Rev. C 5, 62 (1972)
P Bonche and D Vautherin, Nucl. Phys. A 372, 496 (1981)
J R Stone and P-G Reinhard, Prog. Part. Nucl. Phys. 56, 587 (2007)
I Dutt and N K Dhiman, Chin. Phys. Lett. 27, 112401 (2010)
E Chabanat, P Bonche, P Haensel, J Meyer and R Schaeffer, Nucl. Phys. A 627, 710 (1997); Nucl. Phys. A 635, 231 (1998)
E N E van Dalen, P Gögelein and H Müther, Phys. Rev. C 80, 044312 (2009)
P Grygorov, E N V van Dalen, J Margueron and H Müther, Phys. Rev. C 82, 014315 (2010)
E N E van Dalen and H Müther, Phys. Rev. C 90, 034312 (2014)
P Grange, J Cugnon and A Lejeune, Nucl. Phys. A 473, 365 (1987)
G Q Li, R Machleidt and R Brockmann, Phys. Rev. C 45, 2782 (1992)
S Gandolfi, J Carlson, S Reddy, A W Steiner and R B Wiringa, Eur. Phys. J. A 50, 10 (2014)
A Akmal, V R Pandharipande and D G Ravenhall, Phys. Rev. C 58, 1804 (1998)
R Millerson and F Sammarruca, arXiv:1906.02905v1
S Binder, J Langhammer, A Calci and R Roth, Phys. Lett. B 736, 119 (2014)
K Gad, Eur. Phys. J. A 51, 98 (2015)
P Wang and W Zuo, Chin. Phys. C 33, 1 (2009)
P Danielewicz, R Lacey and W G Lynch, Science 298, 1592 (2002)
M Prakash, T L Ainsworth and J M Lattimer, Phys. Rev. Lett. 61, 2518 (1988)
M Baldo, G F Burgio, H-J Schulze and G Taranto, Phys. Rev. C 89, 048801 (2014)
K Gad, Phys. At. Nucl. 81, 429 (2018)
K Gad, Indian J. Phys. 95, 1499 (2021)
Acknowledgements
The author is grateful to Deanship of Scientific Research at Islamic University of Madinah for funding this work through the research Project No. (23/40) of the 10th (Takamul) programs of academic year 1440-1441 AH. The author would like to thank Professor R Machleidt for providing potential code.
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Gad, K. Properties of pure neutron matter at low and high densities. Pramana - J Phys 95, 108 (2021). https://doi.org/10.1007/s12043-021-02144-7
Received:
Revised:
Accepted:
Published:
DOI: https://doi.org/10.1007/s12043-021-02144-7