Gravitational Radiation from Colliding Black Holes

S. W. Hawking
Phys. Rev. Lett. 26, 1344 – Published 24 May 1971
An article within the collection: The Work of Stephen Hawking in Physical Review
PDFExport Citation

Abstract

It is shown that there is an upper bound to the energy of the gravitational radiation emitted when one collapsed object captures another. In the case of two objects with equal masses m and zero intrinsic angular momenta, this upper bound is (22)m.

  • Received 11 March 1971

DOI:https://doi.org/10.1103/PhysRevLett.26.1344

©1971 American Physical Society

Collections

This article appears in the following collection:

The Work of Stephen Hawking in Physical Review

To mark the passing of Stephen Hawking, we gathered together his 55 papers in Physical Review D and Physical Review Letters. They probe the edges of space and time, from "Black holes and thermodynamics” to "Wave function of the Universe."

Authors & Affiliations

S. W. Hawking

  • Institute of Theoretical Astronomy, University of Cambridge, Cambridge, England

References (Subscription Required)

Click to Expand
Issue

Vol. 26, Iss. 21 — 24 May 1971

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review Letters

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×