# Maximum Mass Of Differentially Rotating Strange Quark Stars

## TL;DR

This paper presents relativistic simulations showing that differential rotation can significantly increase the maximum mass of strange quark stars, with potential implications for astrophysical observations of massive compact objects.

## Contribution

First fully relativistic numerical calculations of differentially rotating strange quark stars using the MIT Bag model, exploring their maximum mass limits across various rotation degrees.

## Key findings

- Maximum mass increases with differential rotation and solution type.
- Maximum mass can be over four times the non-rotating value.
- Differential rotation allows strange stars to reach masses much larger than nuclear matter stars.

## Abstract

We present the first fully relativistic numerical calculations of differentially rotating Strange Quark Stars models for broad ranges of the maximum density and of the degree of differential rotation. Our simulations are performed with the very accurate and stable multi-domain spectral code FlatStar and use the MIT Bag model for describing strange quark matter. Our calculations based on a thorough exploration of the solution space show that the maximum mass of strange stars depends on both the degree of differential rotation and a type of solution, similarly to neutron stars described by a polytropic equations of state. The highest increase of the maximum mass (compared to the value for a non-rotating star) is obtained for models with a low degree of differential rotation. This highest mass is over four times larger than that of the equivalent non rotating configuration. Comparing our results with calculations done for realistic models of neutron stars, we conclude that with the help of differential rotation, strange stars can sustain masses much larger than stars made from nuclear matter for low degree of differential rotation which reinforces the hope of demonstrating, or of ruling out, the existence of strange matter through the observation by gravitational waves, by gamma rays or by neutrinos of the massive material object born from the merger of a compact binary system or during some supernova events.