Constraining parity violation in gravity with measurements of neutron-star moments of inertia
- Department of Physics, Princeton University, Princeton, New Jersey 08544 (United States)
- Department of Astronomy, University of Arizona, Tucson, Arizona 85721 (United States)
- Institute for Theory and Computation (ITC), Harvard Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts 02138 (United States)
Neutron stars are sensitive laboratories for testing general relativity, especially when considering deviations where velocities are relativistic and gravitational fields are strong. One such deviation is described by dynamical, Chern-Simons modified gravity, where the Einstein-Hilbert action is modified through the addition of the gravitational parity-violating Pontryagin density coupled to a field. This four-dimensional effective theory arises naturally both in perturbative and nonperturbative string theory, loop quantum gravity, and generic effective field theory expansions. We calculate here Chern-Simons modifications to the properties and gravitational fields of slowly spinning neutron stars. We find that the Chern-Simons correction affects only the gravitomagnetic sector of the metric to leading order, thus introducing modifications to the moment-of-inertia but not to the mass-radius relation. We show that an observational determination of the moment-of-inertia to an accuracy of 10%, as is expected from near-future observations of the double pulsar, will place a constraint on the Chern-Simons coupling constant of {xi}{sup 1/4} < or approx. 5 km, which is at least three-orders of magnitude stronger than the previous strongest bound.
- OSTI ID:
- 21409408
- Journal Information:
- Physical Review. D, Particles Fields, Vol. 81, Issue 6; Other Information: DOI: 10.1103/PhysRevD.81.064020; (c) 2010 The American Physical Society; ISSN 0556-2821
- Country of Publication:
- United States
- Language:
- English
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79 ASTROPHYSICS
COSMOLOGY AND ASTRONOMY
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GENERAL RELATIVITY THEORY
GRAVITATIONAL FIELDS
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METRICS
MOMENT OF INERTIA
NEUTRON STARS
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PARTICLE PROPERTIES
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