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Final Remarks

  • Pantelis PnigourasEmail author
Chapter
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Part of the Springer Theses book series (Springer Theses)

Abstract

Summary, conclusions, and final remarks.

References

  1. Doneva, D. D., Kokkotas, K. D., & Pnigouras, P. (2015). Gravitational wave afterglow in binary neutron star mergers. Physical Review D, 92, 104040.  https://doi.org/10.1103/PhysRevD.92.104040, arXiv:1510.00673.
  2. Kastaun, W., Willburger, B., & Kokkotas, K. D. (2010). Saturation amplitude of the f-mode instability. Physical Review D, 82, 104036.  https://doi.org/10.1103/PhysRevD.82.104036, arXiv:1006.3885.
  3. Passamonti, A., & Glampedakis, K. (2012). Non-linear viscous damping and gravitational wave detectability of the f-mode instability in neutron stars. Monthly Notices of the Royal Astronomical Society, 422, 3327–3338.  https://doi.org/10.1111/j.1365-2966.2012.20849.x, arXiv:1112.3931.ADSCrossRefGoogle Scholar
  4. Passamonti, A., Gaertig, E., Kokkotas, K. D., & Doneva, D. (2013). Evolution of the f-mode instability in neutron stars and gravitational wave detectability. Physical Review D, 87, 084010.  https://doi.org/10.1103/PhysRevD.87.084010, arXiv:1209.5308.

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© Springer Nature Switzerland AG 2018

Authors and Affiliations

  1. 1.Mathematical Sciences and STAG Research CentreUniversity of SouthamptonSouthamptonUK

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