Office: Hoyle H29
Office Tel: (01223) 766645
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I am interestd in probing the structure and evolution of the Universe with gravitational-waves. In particular, I have performed work on a technique to constrain cosmological parameters using only the gravitational-waves emitted by inspiraling double neutron-star systems. These systems are referred to as self-calibrating standard sirens, since they constitute a cosmological distance indicator which is calibrated only by our understanding of gravitation. I have also worked on constraining the properties and nature of a stochastic gravitational-wave background by using arrays of regularly observed millisecond pulsars. These pulsars act as very stable clocks such that any background of gravitational-waves may leave a measurable and correlated imprint in the arrival times of pulses.
S. R. Taylor, J. R. Gair, and L. Lentati, "Weighing The Evidence For A Gravitational-Wave Background In The First International Pulsar Timing Array Data Challenge", Phys. Rev. D 87, 044035 (2013), DOI:10.1103/PhysRevD.87.044035, arXiv:1210.6014
S. R. Taylor, and J. R. Gair, "Cosmology with the lights off: Standard sirens in the Einstein Telescope era", Phys. Rev. D 86, 023502 (2012), 1204.6739, DOI:10.1103/PhysRevD.86.023502, arXiv:1204.6739
S. R. Taylor, J. R. Gair, and L. Lentati, "Using Swarm Intelligence To Accelerate Pulsar Timing Analysis", (2012), arXiv:1210.3489
L. Lentati, P. Alexander, M. P. Hobson, S. Taylor, J. Gair, S. T. Balan, R. van Haasteren, "Hyper-efficient model-independent Bayesian method for the analysis of pulsar timing data", Phys. Rev. D 87, 104021 (2013), DOI:10.1103/PhysRevD.87.104021, arXiv:1210.3578