Static Tidal Perturbations of Relativistic Stars: Corrected Center Expansion and Love Numbers-I
Emel Altas, Ercan Kilicarslan, Onur Oktay, Bayram Tekin
TLDR
This paper corrects a subleading coefficient in the Frobenius expansion for relativistic star tidal perturbations and extends the formalism to Schwarzschild-de Sitter backgrounds.
Key contributions
- Corrected a subleading coefficient in the Frobenius expansion for relativistic star tidal perturbations.
- Derived the static even-parity master equation for Schwarzschild-de Sitter backgrounds.
- Showed how the general interior even-parity system reduces to the standard quadrupolar equation.
- Confirmed the corrected coefficient doesn't change the Love number k2 within numerical accuracy.
Why it matters
This work refines the theoretical framework for understanding tidal perturbations of relativistic stars, crucial for gravitational wave astronomy. By correcting a long-standing coefficient and extending the model to more complex spacetimes, it enhances the accuracy and applicability of Love number calculations.
Original Abstract
We revisit static tidal perturbations of relativistic stars with emphasis on two technical issues in the standard quadrupolar formulation. First, we derive the regular-center Frobenius expansion of the interior even-parity master function and obtain a corrected subleading coefficient, which differs from the expression commonly used in the literature. Second, we derive the static even-parity master equation on a Schwarzschild-de Sitter background, extending the usual asymptotically flat problem to a two-horizon geometry. To place these results on a common footing, we also show how the general interior even-parity system in Regge-Wheeler gauge reduces to the standard quadrupolar equation used in Love-number calculations. Numerical integrations for polytropic equations of state show that the corrected center coefficient affects only subleading initial data and leaves the extracted Love number $k_2$ unchanged within numerical accuracy. Taken together, these results fix the regular-center input to the standard quadrupolar problem and extend the static even-parity formalism to Schwarzschild-de Sitter backgrounds.
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