Dark Branches of Immortal Stars at the Galactic Center

Fuente: arXiv
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Main Authors: John, Isabelle, Leane, Rebecca K., Linden, Tim
Format: Preprint
Published: 2024
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author John, Isabelle
Leane, Rebecca K.
Linden, Tim
author_facet John, Isabelle
Leane, Rebecca K.
Linden, Tim
contents We show that stars in the inner parsec of the Milky Way can be significantly affected by dark matter annihilation, producing population-level effects that are visible in a Hertzsprung-Russell (HR) diagram. We establish the dark HR diagram, where stars lie on a new stable $\textit{dark main sequence}$ with similar luminosities, but lower temperatures, than the standard main sequence. The dark matter density in these stars continuously replenishes, granting these stars immortality and solving multiple stellar anomalies. Upcoming telescopes could detect the dark main sequence, offering a new dark matter discovery avenue.
format Preprint
id arxiv_https___arxiv_org_abs_2405_12267
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Dark Branches of Immortal Stars at the Galactic Center
John, Isabelle
Leane, Rebecca K.
Linden, Tim
High Energy Astrophysical Phenomena
Solar and Stellar Astrophysics
High Energy Physics - Phenomenology
We show that stars in the inner parsec of the Milky Way can be significantly affected by dark matter annihilation, producing population-level effects that are visible in a Hertzsprung-Russell (HR) diagram. We establish the dark HR diagram, where stars lie on a new stable $\textit{dark main sequence}$ with similar luminosities, but lower temperatures, than the standard main sequence. The dark matter density in these stars continuously replenishes, granting these stars immortality and solving multiple stellar anomalies. Upcoming telescopes could detect the dark main sequence, offering a new dark matter discovery avenue.
title Dark Branches of Immortal Stars at the Galactic Center
topic High Energy Astrophysical Phenomena
Solar and Stellar Astrophysics
High Energy Physics - Phenomenology
url https://arxiv.org/abs/2405.12267