Consequences of the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>σ</mml:mi> </mml:math> -cut potential for the properties of neutron stars within the framework of the relativistic mean-field model based on chiral effective field theoryAarsha Nandana, B. K. Sharma, Yashmitha Kumaran et al.|Physical review. C|2025Cited by 0