Cauchy horizon stability in self-similar collapse: Scalar radiation

Thomas Waters; Brien Nolan

Cauchy horizon stability in self-similar collapse: Scalar radiation

Thomas Waters, Brien Nolan

School of Mathematics & Physics

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Abstract

The stability of the Cauchy horizon in spherically symmetric self-similar collapse is studied by determining the flux of scalar radiation impinging on the horizon. This flux is found to be finite.

Original language	English
Journal	Physical Review D
Volume	66
Publication status	Published - 2002

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Cauchy horizon stability in self-similar collapse - scalar radiation

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title = "Cauchy horizon stability in self-similar collapse: Scalar radiation",

abstract = "The stability of the Cauchy horizon in spherically symmetric self-similar collapse is studied by determining the flux of scalar radiation impinging on the horizon. This flux is found to be finite.",

author = "Thomas Waters and Brien Nolan",

year = "2002",

language = "English",

volume = "66",

journal = "Physical Review D",

issn = "2470-0010",

publisher = "American Physical Society",

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T1 - Cauchy horizon stability in self-similar collapse: Scalar radiation

AU - Waters, Thomas

AU - Nolan, Brien

PY - 2002

Y1 - 2002

N2 - The stability of the Cauchy horizon in spherically symmetric self-similar collapse is studied by determining the flux of scalar radiation impinging on the horizon. This flux is found to be finite.

AB - The stability of the Cauchy horizon in spherically symmetric self-similar collapse is studied by determining the flux of scalar radiation impinging on the horizon. This flux is found to be finite.

M3 - Article

SN - 2470-0010

VL - 66

JO - Physical Review D

JF - Physical Review D

ER -

Cauchy horizon stability in self-similar collapse: Scalar radiation

Abstract

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