A Precision Test for an Extra Spatial Dimension Using Black Hole--Pulsar Binaries

@article{Simonetti2010APT,
  title={A Precision Test for an Extra Spatial Dimension Using Black Hole--Pulsar Binaries},
  author={J. Simonetti and M. Kavic and D. Minic and Umair Surani and Vipin Vejayan},
  journal={arXiv: High Energy Astrophysical Phenomena},
  year={2010}
}
We discuss the observable effects of enhanced black-hole mass loss in a black hole--neutron star (BH--NS) binary, due to the presence of a warped extra spatial dimension of curvature radius $L$ in the braneworld scenario. For some masses and orbital parameters in the expected ranges the binary components would outspiral, the opposite of the behavior due to energy loss from gravitational radiation alone. If the NS is a pulsar, observations of the rate of change of the orbital period with a… Expand

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