A Theoretical Study of the Magnetically Deformed Inner Crust Matter of Magnetars
Arpita Ghosh, Somenath Chakrabarty
TL;DR
This paper presents a theoretical analysis of the physical properties of magnetically deformed crustal matter in magnetars using a relativistic Thomas-Fermi model to understand atomic and matter deformation under strong magnetic fields.
Contribution
It introduces a relativistic Thomas-Fermi model in cylindrical coordinates to study magnetically deformed crust matter in magnetars, providing new insights into their physical properties.
Findings
Properties of magnetically deformed atoms analyzed
Relativistic TF model applied to neutron star crust
Insights into matter deformation under strong magnetic fields
Abstract
We have studied various physical properties of magnetically deformed atoms and the associated matter, replacing the atoms by the deformed Wigner-Seitz (WS) cells at the crustal region of strongly magnetized neutron stars (magnetars). A relativistic version of Thomas-Fermi (TF) model in presence of strong magnetic field in cylindrical coordinates is used to study the properties of such matter.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.