Published April 1, 2009 | Version v1
Journal article

CONSTRAINTS ON NONLUMINOUS MATTER FROM HIGHER ORDER PULSAR PERIOD DERIVATIVES

  • 1. Department of Physics, Ben-Gurion University, Beer-Sheva 84105 (Israel)

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/L95

Additional 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