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 theory
Aarsha Nandana(Amrita Vishwa Vidyapeetham), B. K. Sharma, Yashmitha Kumaran(Eastern Mediterranean University), Tauhid Bin Iqbal(Babasaheb Bhimrao Ambedkar University), G. Sriram Bhashyam(Amrita Vishwa Vidyapeetham)
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