The Cosmic Gravitational Wave Background in a Cyclic Universe
The Cosmic Gravitational-Wave Background in a Cyclic Universe Latham A. Boyle1, Paul J. Steinhardt1, and Neil Turok2 1Department of Physics, Princeton University, Princeton, New Jersey 08544 2Department of Applied Mathematics and Theoretical Physics, Centre for Mathematical Sciences, University of Cambridge, Wilberforce Road, Cambridge CB3 OWA, United Kingdom (Dated: July 2003) Inflation predicts a primordial gravitational wave spectrum that is slightly “red,” i.e. nearly scale-invariant with slowly increasing power at longer wavelengths. In this paper, we compute both the amplitude and spectral form of the primordial tensor spectrum predicted by cyclic/ekpyrotic models. The spectrum is exponentially suppressed compared to inflation on long wavelengths, and the strongest constraint emerges from the requirement that the energy density in gravitational waves should not exceed around 10 per cent of the energy density at the time of nucleosynthesis. The recently-proposed cyclic model[1, 2] differs radi- V(φ) cally from standard inflationary cosmology [3, 4], while retaining the inflationary predictions of homogeneity, 4 5 φ 6 flatness, and nearly scale-invariant density perturbations. end It has been suggested that the cosmic gravitational wave 3 1 φ background provides the best experimental means for dis- tinguishing the two models. Inflation predicts a nearly 2 scale-invariant (slightly red) spectrum of primordial ten- sor perturbations, whereas the cyclic model predicts a blue spectrum.[1] The difference arises because inflation involves an early phase of hyper-rapid cosmic accelera- tion, whereas the cyclic model does not. In this paper, we compute the gravitational wave spec- trum for cyclic models to obtain both the normalization and spectral shape as a function of model parameters, im- V proving upon earlier heuristic estimates.
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