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Circular Polarization of Gravitational Waves in String Cosmology

MIAMI, 200 7 .12.14. Circular Polarization of Gravitational Waves in String Cosmology. Jiro Soda. Kyoto University. work with Masaki Satoh & Sugumi Kanno arXiv:0706.3585. Polarization of Gravitational Waves. Action for GW.

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Circular Polarization of Gravitational Waves in String Cosmology

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  1. MIAMI, 2007.12.14 Circular Polarization of Gravitational Waves in String Cosmology Jiro Soda Kyoto University work with Masaki Satoh & Sugumi Kanno arXiv:0706.3585

  2. Polarization of Gravitational Waves Action for GW GW propagating in the z direction can be written in the TT gauge as Any linear combination of these polarization can be a basis of GW.

  3. Circular polarization of GW Right-handed circular polarization Left-handed circular polarization Without a parity violating process, the circular polarization of primordial GW does not exist.

  4. Motivation of our work In the effective action of superstring theory, gravitational Chern-Simons term, which violates the parity invariance, often appears. Hence, it may produce Circular polarization of primordial GW Known result S.Alexander & J.Martin, Phys.Rev.D71, 063526 (2005) Slow roll inflation does not produce circular polarization Our observation Gauss-Bonnet term also appears in superstring theory We should study the primordial GW in the context of Gauss-Bonnet-Chern-Simons gravity.

  5. Summary of our result Inflaton drives the slow-roll inflation This term is not relevant to background dynamics, but could produce the circular polarization of gravitational waves This term induces the super-inflation, and the instability of gravitational waves These effects produce 100 % circular polarization of GW. Moreover, the amplitude is also enhanced by the factor . Hence, the effect is detectable by DECIGO/BBO or even by LISA.

  6. Outline of my talk • Inflation in Gauss-Bonnet-Chern-Simons Gravity • A mechanism to produce circular polarization • Two field inflation & detectability • Conclusion

  7. Inflation in Gauss-Bonnet -Chern-Simons Gravity

  8. Cosmological background space-time Homogeneous and isotropic universe Friedman equation Scalar field equation For concreteness, we take a simple model The equations can be cast into the autonomous system There exists a region where super-inflation occurs.

  9. Numerical Result Super-inflation regime Slow roll regime GB term drives the super-inflation. It indicates the violation of weak energy condition.

  10. Analytic solution in Super-inflation regime In the super-inflationary regime, the system can be well described by Gauss-Bonnet dominant equations It is not difficult to obtain an analytic solution decreasing expanding What can we expect for the gravitational waves in this background?

  11. A mechanism to produce circular polarization

  12. Gravitational waves in GB-CS gravity Tensor perturbation Polarization state polarization tensor Circular polarization With the transformation , we get GB CS Right-handed and left-handed waves obey different equations!

  13. GW in Super inflationary regime In super-inflationary regime and on the scales Thus, we have Both GB and CS contribute here

  14. Instability induces Polarization quantization vacuum fluctuations E.O.M. on sub-horizon scales Left-handed circular polarization mode is simply oscillating, Right-handed circular polarization mode is exponentially growing.

  15. Schematic picture of evolution right-handed instability freeze Bunch-Davis vacuum

  16. Degree of Polarization The instability continues during The growth factor gives Hence, we have the degree of circular polarization The string theory could produce 100 percent circularly polarized GW! Note that the amplitude is also enhanced by the instability.

  17. Everything seems to go well. However, we have to consider the scalar curvature perturbations for which we also expect the very blue power spectrum Fortunately, it is possible to circumvent this difficulty.

  18. Two field inflation & detectability

  19. Primordial GW (Maggiore 2000) Pulsar timing BBN bound CMB bound LIGO II LISA DECIGO/BBO Inflation origin There is almost no constraint in this frequency range!

  20. Two-field inflation field drives the first inflation where CMB spectrum is relevant field drives the second inflation where GB and CS are important At the onset of the second inflation, GB term induces the super-inflation The amplitude of GW is enhanced there and the circular polarization is created. In principle, it is possible to observe the circular polarization of GW by LISA, if the onset of the second inflation lies in the appropriate period.

  21. A concrete realization

  22. Detectability We thus have the following schematic picture. Assuming 10 years observational time Seto 2006 at For LIGO and LCGT, we have Taruya&Seto 2007 It should be stressed that our model is completely consistent with current observations.

  23. Conclusion

  24. Observe the circular polarization of primordial gravitational waves! That might be a signature of the superstring theory! It must be easier than that we have thought before. Because the amplitude is enhanced by several orders! It strongly supports the superstring theory. At least, it indicates the existence of gravitational Chen-Simons term.

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