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Echoes from phantom wormholes

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arxiv 2007.09078 v2 pith:YSLTOVFY submitted 2020-07-17 gr-qc astro-ph.HEhep-th

classification gr-qcastro-ph.HEhep-th
keywords darkechoesenergyomegaphantomstatewormholesecho
verification ladder T0 review T1 audit T2 compute T3 formal

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abstract

We study the time evolution of the test scalar and electromagnetic fields perturbations in configurations of phantom wormholes surrounded by dark energy with state parameter $\omega< -1$. We observe obvious signals of echoes reflecting wormholes properties and disclose the physical reasons behind such phenomena. In particular, we find that the dark energy equation of state has a clear imprint in echoes in wave perturbations. When $\omega$ approaches the phantom divide $\omega=-1$ from below, the delay time of echoes becomes longer. The echo of gravitational wave is likely to be detected in the near future, the signature of the dark energy equation of state in the echo spectrum can serve as a local measurement of the dark energy.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Can we distinguish whether black holes have singularities or not through echoes and light rings?

    gr-qc 2025-05 conditional novelty 5.0 of 10

    In the Bardeen and Hayward black hole families, the singular type II branch can have two light rings and echo-like quasinormal signals, while regular black holes have one light ring.

  2. Phenomenology of Schwarzschild-like Black Holes with a Generalized Compton Wavelength

    gr-qc 2025-04 reject novelty 4.0 of 10

    A generalized Compton wavelength deformation of Schwarzschild spacetime yields EHT and solar system bounds on the deformation parameter epsilon, currently consistent with general relativity.

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