World Scientific
Skip main navigation

Cookies Notification

We use cookies on this site to enhance your user experience. By continuing to browse the site, you consent to the use of our cookies. Learn More
×

System Upgrade on Tue, May 28th, 2024 at 2am (EDT)

Existing users will be able to log into the site and access content. However, E-commerce and registration of new users may not be available for up to 12 hours.
For online purchase, please visit us again. Contact us at customercare@wspc.com for any enquiries.
SPECIAL ISSUE – VII Black Holes Workshop; Guest Editors: Carlos A. R. Herdeiro, Vitor Cardoso, José P. S. Lemos and Filipe C. MenaNo Access

Schwarzschild radial perturbations in Eddington–Finkelstein and Painlevé–Gullstrand coordinates

    https://doi.org/10.1142/S0218271815420067Cited by:7 (Source: Crossref)

    In a previous paper, we have considered the Regge–Wheeler equation for fields of spin s = 0, 1 or 2 on the Schwarzschild spacetime in coordinates that are regular at the horizon. In particular, we have constructed in Eddington–Finkelstein (EF) coordinates exact solutions in terms of series that are regular at the horizon and converge on the entire open domain from the central singularity to infinity. Here, we extend this earlier work in two different directions. First, we consider in EF coordinates a massive scalar field that can serve as a dark matter candidate. Second, we extend the treatment of the massless case to Painlevé–Gullstrand (PG) coordinates, which are associated with radially infalling observers.

    PACS: 04.70.Bw, 03.65.Pm, 04.30.Nk, 11.80.Et
    You currently do not have access to the full text article.

    Recommend the journal to your library today!