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Concluding Remarks

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Exploring the Early Universe with Gravitational Waves

Part of the book series: Springer Theses ((Springer Theses))

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Abstract

In this thesis, I have demonstrated that gravitational waves can be used as powerful probes of the early universe. I focussed on two separate topics, tensor perturbations from inflation within a quantum gravity formalism, and gravitational waves from preheating in the presence of a light scalar field.

Lack of comfort means we are on the threshold of new insights.

—Lawrence M. Krauss

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References

  1. BICEP2 Collaboration Collaboration, P.A.R. Ade et al., BICEP2 I: detection of B-mode polarization at degree angular scales, http://xxx.lanl.gov/abs/1403.3985

  2. J. Errard, The new generation CMB B-mode polarization experiment: POLARBEAR, http://xxx.lanl.gov/abs/1011.0763

  3. B. Crill, P. Ade, E. Battistelli, S. Benton, R. Bihary, et al., SPIDER: a balloon-borne large-scale CMB polarimeter, http://xxx.lanl.gov/abs/0807.1548

  4. B. Sathyaprakash, B. Schutz, Physics, astrophysics and cosmology with gravitational waves. Living Rev. Rel. 12 (2009) 2, http://xxx.lanl.gov/abs/0903.0338

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Correspondence to Laura Bianca Bethke .

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Bethke, L.B. (2015). Concluding Remarks. In: Exploring the Early Universe with Gravitational Waves. Springer Theses. Springer, Cham. https://doi.org/10.1007/978-3-319-17449-5_4

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