Using Gravitational-Wave Observations to Constrain the Parameters of Bag Model

Physics

Scientific paper

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Scientific paper

We consider possibilities for obtaining information about the equation of state for quark matter by using future direct observational data on gravitational waves. We study the nonradial oscillations of the fluid modes of pure quark stars. If we observe the f modes from quark stars, by using the simultaneously obtained radiation radius we can constrain the bag constant B with reasonable accuracy, independently of the s quark mass.

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