Literature DB >> 17501038

Gravitational-wave stochastic background from cosmic strings.

Xavier Siemens1, Vuk Mandic, Jolien Creighton.   

Abstract

We consider the stochastic background of gravitational waves produced by a network of cosmic strings and assess their accessibility to current and planned gravitational wave detectors, as well as to big bang nucleosynthesis (BBN), cosmic microwave background (CMB), and pulsar timing constraints. We find that current data from interferometric gravitational wave detectors, such as Laser Interferometer Gravitational Wave Observatory (LIGO), are sensitive to areas of parameter space of cosmic string models complementary to those accessible to pulsar, BBN, and CMB bounds. Future more sensitive LIGO runs and interferometers such as Advanced LIGO and Laser Interferometer Space Antenna (LISA) will be able to explore substantial parts of the parameter space.

Entities:  

Year:  2007        PMID： 17501038     DOI： 10.1103/PhysRevLett.98.111101

Source DB:  PubMed          Journal:  Phys Rev Lett        ISSN： 0031-9007            Impact factor:   9.161


  1 in total

1.  An upper limit on the stochastic gravitational-wave background of cosmological origin.

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Journal:  Nature       Date:  2009-08-20       Impact factor: 49.962
  1 in total

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