Classical Love for Quantum Blackholes

Ram Brustein; Yotam Sherf

doi:10.1103/PhysRevD.105.024044

paper

Classical Love for Quantum Blackholes

arXiv:2104.06013 · doi:10.1103/PhysRevD.105.024044

Abstract

We present a method for comparing the classical and quantum calculations of the electric quadrupolar Love number $k_{2}$ and show that our previous derivation of the quantum Love number of a quantum blackhole matches exactly the classical calculation of $k_{2}$ when quantum expectation values are replaced by the corresponding classical quantities, as dictated by the Bohr correspondence principle. The standard derivation of $k_{2}$ for classical relativistic stars relies on fixing boundary conditions on the surface of the star for the Einstein equations in the presence of an external perturbing field. An alternative method for calculating $k_{2}$ uses properties of the spectrum of the non-relativistic fluid modes of the star. We adopt this alternative method and use it to derive an effective description of the interior modes in terms of a collection of driven harmonic oscillators characterized by different frequencies and amplitudes. We compare these two classical methods and find that most of the interior information can be integrated out, reducing the problem of calculating $k_{2}$ to fixing a single boundary condition for the perturbed Einstein equations on the surface of the deformed star. We then determine this single boundary condition in terms of the spectrum of the object and proceed to identify the relationship between classical quantities and quantum expectation values and to verify the agreement between the results of the effective classical calculation and the quantum calculation.

arXiv commentReplaced to agree with the published PRD version

Classical Love for Quantum Blackholes

Abstract

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