Stellar structure, magnetism and the variational principle
Andrej \v{C}ade\v{z}, Ale\v{s} Mohori\v{c}, Massimo Calvani

TL;DR
This paper develops a variational model for stellar structure that incorporates electromagnetic effects and angular momentum, providing new insights into the balance of forces in astrophysical objects.
Contribution
It reformulates the polytropic stellar model to include electromagnetic interactions and rotation within a variational framework, extending traditional models.
Findings
Electromagnetic effects can be integrated into stellar models via a surface integral approach.
Exact solutions are obtainable under simplifying assumptions.
The phase diagram reveals patterns indicating the complex interplay of matter, gravity, and electromagnetism.
Abstract
Matter interacts through two long range forces: gravity and electromagnetism. While all matter contributes to the gravitational potential, electromagnetic effects were traditionally expected to cancel in large systems because positive and negative charges balance. Yet astrophysical objects clearly show long range electromagnetic behavior, so the cancellation cannot be perfect. This paper develops a model for stationary aggregation of matter into a star that consistently includes angular momentum and electromagnetic effects. We reformulate the standard polytropic stellar model as a variational problem and extend it to include the kinetic energy of rigid rotation and the electromagnetic interaction energy between oppositely charged baryonic matter. The electromagnetic contribution to the action is taken to be the minimal energy required to generate the stellar magnetic dipole moment. This…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Cosmology and Gravitation Theories · Relativity and Gravitational Theory
