Published July 1982
| Version v1
Journal article
Gravitational radiation of the binary pulsar PSR 1913 + 16
Description
It is shown that in accordance with the relativistic tensor theory of the gravitational field in flat space-time the power of the gravitational radiation from the binary pulsar PSR 1913 + 16 exceeds the prediction of the general theory of relativity by 3.5%. This small correction is due to the contribution of the scalar gravitational radiation. It is noted that in the case of spherically symmetric pulsations of bodies the scalar gravitational radiation becomes decisive
Additional details
Publishing Information
- Journal Title
- Astrophysics (Engl. Transl.)
- Journal Volume
- 18
- Journal Issue
- 1
- Series
- Astrophysics (Engl. Transl.).
- Journal Page Range
- 58-61
- ISSN
- 0004-6396
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 14797659
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BINARY STARS; GENERAL RELATIVITY THEORY; GRAVITATIONAL RADIATION; GRAVITATIONAL WAVES; PULSARS; TENSORS
- Descriptors DEC
- COSMIC RADIO SOURCES; FIELD THEORIES; RADIATIONS; STARS
Optional Information
- Notes
- Translated from Astrofizika; 18: 93-99(Jan 1982). Cover-to-cover translation of Astrofizika (USSR).