8–13 Jun 2025
America/Winnipeg timezone
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A New Look at Quark Stars

10 Jun 2025, 15:30
15m
Oral (Non-Student) / Orale (non-étudiant(e)) Theoretical Physics / Physique théorique (DTP-DPT) (DTP) T2-10 Classical gravity and general relativity | Gravité classique et relativité générale (DPT)

Speaker

Robert Mann

Description

Quark stars — a gravitationally bound quark-gluon plasma — have been
hypothesized to be the last gravitationally stable state of matter preceding collapse into a black hole. Originally such stars were thought to necessarily contain a significant component of strange quarks, but recent work has shown that up-down quark matter can be more stable than ordinary nuclei at sufficiently large baryon number beyond the periodic table. I shall describe how such up-down quark stars open up new possibilities for astrophysical searches for such objects as well as new tests of general relativity.

Keyword-1 Astrophysics
Keyword-2 Quark
Keyword-3 Gravitation

Author

Robert Mann

Presentation materials

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