16
Trispectrum estimator in equilateral type non- Gaussian models Shuntaro Mizuno (Portsmouth) COSMO/CosPA 2010@ The University of Tokyo 2010. 9. 27 – 10. 1 with Kazuya Koyama (Portsmouth) arXiv:1007.1462 [hep-th]

COSMO/CosPA 2010@ The University of Tokyo …...- multi-field DBI inflation 87 % correlation 33 % correlation More accurate than considering only the equilateral configuration •

  • Upload
    others

  • View
    0

  • Download
    0

Embed Size (px)

Citation preview

Page 1: COSMO/CosPA 2010@ The University of Tokyo …...- multi-field DBI inflation 87 % correlation 33 % correlation More accurate than considering only the equilateral configuration •

Trispectrum estimator in equilateral type non-Gaussian models

Shuntaro Mizuno (Portsmouth)

COSMO/CosPA 2010@ The University of Tokyo2010. 9. 27 – 10. 1

with Kazuya Koyama (Portsmouth)

arXiv:1007.1462 [hep-th]

Page 2: COSMO/CosPA 2010@ The University of Tokyo …...- multi-field DBI inflation 87 % correlation 33 % correlation More accurate than considering only the equilateral configuration •

Primordial Trispectrum

k3

k2

k1

k4

gives also important information !!

• Definition

Takahashi

Kobayashi

Izumi

Page 3: COSMO/CosPA 2010@ The University of Tokyo …...- multi-field DBI inflation 87 % correlation 33 % correlation More accurate than considering only the equilateral configuration •

Primordial Trispectrum in equilateral type model• single field DBIEx)• multi-field DBI

Arroja, SM, Koyama, Tanaka `09

SM, Arroja, Koyama `09

In-in formalism

Includes complicated functions like

practically, not so useful as a theoretical template !!

Page 4: COSMO/CosPA 2010@ The University of Tokyo …...- multi-field DBI inflation 87 % correlation 33 % correlation More accurate than considering only the equilateral configuration •

Bispectrum estimator• Estimator for general case model

calculation time

• Estimator for local type model

in general

with

separable form

calculation time HEALPix

theoryobservation

Komatsu, Spergel `01

Page 5: COSMO/CosPA 2010@ The University of Tokyo …...- multi-field DBI inflation 87 % correlation 33 % correlation More accurate than considering only the equilateral configuration •

Bispectrum estimator in equilateral type model• Separable equilateral shape function

matching the amplitudes at

DBI Separable form Difference

Babichi, Creminelli, Zaldarriaga `04

k3/k1 k3/k1 k3/k1

k2/k1k2/k1k2/k1This template fits the bispectrum in DBI inflation very well !!

Page 6: COSMO/CosPA 2010@ The University of Tokyo …...- multi-field DBI inflation 87 % correlation 33 % correlation More accurate than considering only the equilateral configuration •

Separable TrispectrumTrispectrum in DBI inflation is not separable, but

there is a quasi-separable and symmetric trispectrum.

• Quasi-separable trispectrum

separable by introducing the integral

・appears for k-inflation with

・not constrained by the bispectrum measurements

validity to use this shape as a template is nontrivial

Chen et al `09

Page 7: COSMO/CosPA 2010@ The University of Tokyo …...- multi-field DBI inflation 87 % correlation 33 % correlation More accurate than considering only the equilateral configuration •

Shape function• Shape function motivated by CMB trispectrum

configurations are specified by

• Physical region should satisfy

-Triangle conditions for and

-

reduced trispectrum

Page 8: COSMO/CosPA 2010@ The University of Tokyo …...- multi-field DBI inflation 87 % correlation 33 % correlation More accurate than considering only the equilateral configuration •

Shape correlator Regan, Shellard, Furgusson `10

• Overlap integral

-integration is over physical region

-weight function motivated by the estimator in space

• Shape correlator

We can check the validity of the estimator

Page 9: COSMO/CosPA 2010@ The University of Tokyo …...- multi-field DBI inflation 87 % correlation 33 % correlation More accurate than considering only the equilateral configuration •

Parametrisation of allowed regionFrom the scaling behaviour, we can separate out the overall scale q,

from the behaviour on a cross-sectional slice

only this part is important

• Intro. variables for triangle here, we set

asymmetry between and

ratio between and

Page 10: COSMO/CosPA 2010@ The University of Tokyo …...- multi-field DBI inflation 87 % correlation 33 % correlation More accurate than considering only the equilateral configuration •

Parametrisation of allowed region (cont.) • Intro. variables for triangle

ratio of the size of the two triangles not lose the generality to consider

asymmetry between and

given by

• necessary facts for the overlap integral

Page 11: COSMO/CosPA 2010@ The University of Tokyo …...- multi-field DBI inflation 87 % correlation 33 % correlation More accurate than considering only the equilateral configuration •

Results

Matching at a point underestimate the amplitudes by factor 2 ~ 4 !!

Cf. Bispectrum

Matching at a point

Page 12: COSMO/CosPA 2010@ The University of Tokyo …...- multi-field DBI inflation 87 % correlation 33 % correlation More accurate than considering only the equilateral configuration •

Conclusion and discussion• Estimator for equilateral type primordial non-Gaussianity

- Separable shape

- Shape correlation

• Predictions- special class of k-inflation

- single field DBI inflation

- multi-field DBI inflation

87 % correlation

33 % correlation

More accurate than considering only the equilateral configuration

• Detectability

• Application to other models?Ghost inflation, Lifshitz field, DBI Galileon, ….

Creminelli, Senatore, Zaldarriaga `07

Page 13: COSMO/CosPA 2010@ The University of Tokyo …...- multi-field DBI inflation 87 % correlation 33 % correlation More accurate than considering only the equilateral configuration •

Thank you very much !

Page 14: COSMO/CosPA 2010@ The University of Tokyo …...- multi-field DBI inflation 87 % correlation 33 % correlation More accurate than considering only the equilateral configuration •

Equilateral shape

This shape is obtained by a special class of k-inflation

shown to be natural from effective theory of inflation Senatore and Zaldarriaga `10

Page 15: COSMO/CosPA 2010@ The University of Tokyo …...- multi-field DBI inflation 87 % correlation 33 % correlation More accurate than considering only the equilateral configuration •

Shape function for single field DBI inflation

• Shape correlation

0.90 (configs. with ) 0.87 (full configs.)Sufficiently large overlap

Page 16: COSMO/CosPA 2010@ The University of Tokyo …...- multi-field DBI inflation 87 % correlation 33 % correlation More accurate than considering only the equilateral configuration •

Shape function for multi-field DBI inflation

• Shape correlation0.60 (configs. with ) 0.33 (full configs.)

SM, Arroja, Koyama `09Trispectrum can distinguish single DBI from multi DBI