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gr-qc2023
Effects of magnetic field on the equation of state in curved spacetime of a neutron star
Golam Mortuza Hossain, Susobhan Mandal
Neutron stars are known to have strong magnetic fields reaching as high as Gauss, besides having strongly curved interior spacetime. So for computing an equation of state…
gr-qc2023
From Horndeski action to the Callan-Giddings-Harvey-Strominger model and beyond
Susobhan Mandal, Tausif Parvez, S. Shankaranarayanan
The knowledge of what entered black hole (BH) is completely lost as it evaporates. This contradicts the unitarity principle of quantum mechanics and is referred to as the informati…