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GENERAL HOLOMORPHIC PURE SUPERGRAVITY AND ITS COSMOLOGY Takahiro Terada Univ. of Tokyo, Japan Sergei V. Ketov and TT, JHEP07(2013)127, arXiv:1304.4319 [hep-th] 19th International Summer Institute on Phenomenology of Elementary Particles and Cosmology GENERALIZATION OF SUPERGRAVITY SUPERSYMMETRIZATION OF MODIFIED GRAVITY

General holomorphic pure supergravity and its cosmology

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Generalization of Supergravity. General holomorphic pure supergravity and its cosmology. 19th International Summer Institute on Phenomenology of Elementary Particles and Cosmology. Takahiro Terada Univ. of Tokyo, Japan Sergei V. Ketov and TT, JHEP07(2013)127, - PowerPoint PPT Presentation

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Page 1: General holomorphic pure supergravity and its cosmology

GENERAL HOLOMORPHIC PURE SUPERGRAVITY AND

ITS COSMOLOGY

Takahiro Terada

Univ. of Tokyo, Japan

Sergei V. Ketov and TT,

JHEP07(2013)127,

arXiv:1304.4319 [hep-th]

19th International Summer Institute on Phenomenology of Elementary Particles and Cosmology

GENERALIZATION OF

SUPERGRAVITY

SUPERSYMMETRIZATION OF MODIFIED GRAVITY

Page 2: General holomorphic pure supergravity and its cosmology

Ordinary Matter; 4.90% Dark Matter; 26.80%

Dark Energy; 68.30%

Energy Density of The Universe

Ordinary Matter Dark Matter Dark Energy

𝐺𝜇𝜈=8𝜋 𝐺𝑇 𝜇𝜈

Many reasons to do that!!• pure theoretical interests• stringy/quantum corrections• potential applications to pheno• application to inflation• to embed modified gravity into

fundamental theory, etc.

Planck collaboration, arXiv:1303.5082

Page 3: General holomorphic pure supergravity and its cosmology

• A. Einstein, 1915

gravity• A. De Felice and S. Tsujikawa, Living Rev. Rel. 13

(2010) 3 and references therein.

gravity• Our work

• D. Z. Freedman, P. van Nieuwenhuizen and S. Ferrara,

Phys. Rev. D 13 (1976) 3214;• S. Deser and B. Zumino, Phys. Lett. B 62 (1976) 335.

supergravity• S.J. Gates, Jr. and S.V. Ketov, Phys. Lett. B674 (2009) 59

supergravity• Our work

Simple

General

Supersymmetrization

Bosonic sector

NEW NEW

Positioning of the work

Page 4: General holomorphic pure supergravity and its cosmology

ℒ= ∫ d2Θ 2ℰ 𝐹 (ℛ ,𝒲 )+H .c .where is a holomorphic function.

+H.c.

New action for supergravity

Page 5: General holomorphic pure supergravity and its cosmology

gravity and Inflation

𝑓 (𝑅 ,𝐶 )=𝑅− 𝑅2

6𝑀2 +𝑏𝑅𝐶𝜇𝜈𝜌𝜎𝐶𝜇𝜈𝜌𝜎

Starobinsky model + correction term () as a simple non-trivial example:

𝑉=34 𝑀

2 (1−𝑒− √2 /3𝜎+𝑏𝐶𝜇𝜈𝜌𝜎𝐶𝜇𝜈𝜌𝜎𝑒√2 /3𝜎 )2

where is the inflaton mass and is a coupling constant.

𝑆=− 12 ∫ 𝑑4𝑥 √−𝑔 𝑓 (𝑅 ,𝐶)

f(R) gravity Scalar-tensor gravity

f(R,C) gravity scalar-tensor gravity with Weyl tensor

equivalent

equivalent

Page 6: General holomorphic pure supergravity and its cosmology

~𝑏=0.05~𝑏=0.01

~𝑏=0.002~𝑏=0

02~𝑏=−0.01

~𝑏=−0.05

𝑉=34 𝑀

2 (1−𝑒− √2 /3𝜎+~𝑏𝑒√2 /3𝜎 )2

~𝑏≡𝑏𝐶𝜇𝜈𝜌𝜎𝐶𝜇𝜈𝜌𝜎

Page 7: General holomorphic pure supergravity and its cosmology

GENERAL HOLOMORPHIC PURE SUPERGRAVITY AND

ITS COSMOLOGY

Takahiro Terada

Univ. of Tokyo, Japan

Sergei V. Ketov and TT,

JHEP07(2013)127,

arXiv:1304.4319 [hep-th]

19th International Summer Institute on Phenomenology of Elementary Particles and Cosmology

ℒ= ∫ d2Θ 2ℰ 𝐹 (ℛ ,𝒲 )+H .c .SUMMARY• There are many reasons to study modified supergravity.

• We proposed a new type of action for modified gravity and supergravity.

• It’s interesting to compare the results with future CMB data.