10
Analytic reheating Joseph Elliston University of Sussex In collaboration with Stefano Orani and David Mulryne arXiv: 1402.4800

Analytic reheatingbenasque.org/2014cosmology/talks_contr/145_Elliston.pdf · Analytic reheating Joseph Elliston! University of Sussex In collaboration with Stefano Orani and David

  • Upload
    others

  • View
    2

  • Download
    0

Embed Size (px)

Citation preview

Page 1: Analytic reheatingbenasque.org/2014cosmology/talks_contr/145_Elliston.pdf · Analytic reheating Joseph Elliston! University of Sussex In collaboration with Stefano Orani and David

Analytic reheating

Joseph Elliston!University of Sussex

In collaboration with Stefano Orani and David Mulryne

arXiv: 1402.4800

Page 2: Analytic reheatingbenasque.org/2014cosmology/talks_contr/145_Elliston.pdf · Analytic reheating Joseph Elliston! University of Sussex In collaboration with Stefano Orani and David

Reheating matters…

0 50 100 150−2

0

2

4

6

8

10

12

N

fNL

Page 3: Analytic reheatingbenasque.org/2014cosmology/talks_contr/145_Elliston.pdf · Analytic reheating Joseph Elliston! University of Sussex In collaboration with Stefano Orani and David

Our result encapsulates:

Two-field slow-roll inflation Curvaton-type

Inhomogeneous End of Inflation! Modulated Reheating!

Page 4: Analytic reheatingbenasque.org/2014cosmology/talks_contr/145_Elliston.pdf · Analytic reheating Joseph Elliston! University of Sussex In collaboration with Stefano Orani and David

Two-field slow-roll inflation Curvaton-type

Inhomogeneous End of Inflation! Modulated Reheating!

Page 5: Analytic reheatingbenasque.org/2014cosmology/talks_contr/145_Elliston.pdf · Analytic reheating Joseph Elliston! University of Sussex In collaboration with Stefano Orani and David

Inhomogeneous End of Inflation!

Isocurvature fieldAdiabatic!field

Video Available on Youtube

Page 6: Analytic reheatingbenasque.org/2014cosmology/talks_contr/145_Elliston.pdf · Analytic reheating Joseph Elliston! University of Sussex In collaboration with Stefano Orani and David

Modulated Reheating !

MatterRadiation

H = �(�)

Decay width

Equivalence between Inhomogeneous End of Inflation and Modulated Reheating: see arXiv: 1307.7095

Video Available on Youtube

Page 7: Analytic reheatingbenasque.org/2014cosmology/talks_contr/145_Elliston.pdf · Analytic reheating Joseph Elliston! University of Sussex In collaboration with Stefano Orani and David

Analytic calculations…

Phase A is just repeating Vernizzi and Wands (2006)…

Page 8: Analytic reheatingbenasque.org/2014cosmology/talks_contr/145_Elliston.pdf · Analytic reheating Joseph Elliston! University of Sussex In collaboration with Stefano Orani and David

Analytic calculations…

Allows arbitrary hypersurfaces

(uniform density limit)

Page 9: Analytic reheatingbenasque.org/2014cosmology/talks_contr/145_Elliston.pdf · Analytic reheating Joseph Elliston! University of Sussex In collaboration with Stefano Orani and David

Principle result

Modulation effects !=1 if standard curvaton

Horizon Crossing Approximation piece!

(constant)

“Oscillation parameter”!degenerate with r

Page 10: Analytic reheatingbenasque.org/2014cosmology/talks_contr/145_Elliston.pdf · Analytic reheating Joseph Elliston! University of Sussex In collaboration with Stefano Orani and David

Conclusions

• Reheating can alter the predictions of inflation!

• We have a general but simple formula for perturbative reheating with two-components!

• Combines the Curvaton, Inhomogeneous End of Inflation and Modulated Reheating models.!

• Our work is a test bed for investigating the analytic criterion for phase transitions.

arXiv: 1402.4800