Published April 1, 2009
| Version v1
Journal article
CONSTRAINTS ON NONLUMINOUS MATTER FROM HIGHER ORDER PULSAR PERIOD DERIVATIVES
Description
Pulsar timing can detect the discreteness of the mass distribution in the Galaxy. The jerk imposed on millisecond pulsars by their nearest neighbors, and on the Sun by its nearest neighbor, may be detectable presently or within a decade. The method can detect planets in the outer solar system out to distances of several thousand AU, with the sensitivity rapidly increasing with time.
Availability note (English)
Available from http://dx.doi.org/10.1088/0004-637X/694/2/L95Additional details
Identifiers
Publishing Information
- Journal Title
- Astrophysical Journal (Online)
- Journal Volume
- 694
- Journal Issue
- 2
- Journal Page Range
- p. L95-L97
- ISSN
- 1538-4357
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41039710
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- GALAXIES; MASS DISTRIBUTION; NONLUMINOUS MATTER; PLANETS; PULSARS; SOLAR SYSTEM; SUN
- Descriptors DEC
- COSMIC RADIO SOURCES; DISTRIBUTION; MAIN SEQUENCE STARS; MATTER; SPATIAL DISTRIBUTION; STARS