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On the degeneracy between w 0 and w a Yungui Gong Huazhong Univ of Science and Tech 华华华华华华 华华华 e 7 th Aegean Summer School, Paros, Greece, 2013.9.27

On the degeneracy between w 0 and w a

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On the degeneracy between w 0 and w a. Yungui Gong Huazhong Univ of Science and Tech 华中科技大学 龚云贵. The 7 th Aegean Summer School, Paros, Greece, 2013.9.27. Contents. Motivations: General Property of Scalar Field dynamics Dark energy parametrizations The degeneracy between w 0 and w a - PowerPoint PPT Presentation

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Page 1: On the degeneracy between w 0  and w a

On the degeneracy between w0 and wa

Yungui Gong

Huazhong Univ of Science and Tech

华中科技大学龚云贵

The 7th Aegean Summer School, Paros, Greece, 2013.9.27

Page 2: On the degeneracy between w 0  and w a

Contents

Motivations: General Property of Scalar Field dynamics

Dark energy parametrizations

The degeneracy between w0 and wa

The consequence of the derived degeneracy

Page 3: On the degeneracy between w 0  and w a

Motivations

General Property of scalar field dynamics scalar field as dark energy: Tracking

solutions

Tracker fields (Steinhardt etal, PRD 1999)

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Tracking Solutions

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Tracking Solution: General Property

Almost independent of initial conditions Relation

Common Dynamics for scalar fields

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Efstathiou Parametrization Dark energy parametrization: capture the main dynamics of scalar field

MNRAS 383, 879 (1999)

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CPL Parametrization

Approximation

E. Linderastro-ph/0210217

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The degeneracy in CPL model

w0 and wa is degenerated

What is the degeneracy? related with ?

Page 9: On the degeneracy between w 0  and w a

Dark Energy Parametrizations (Partial Lists)

Dark energy parametrization: capture the main dynamics of scalar field

Efstathiou 1999, MNRAS 310, 842

CPL, Chevallier & Polarski 2001, IJMPD 10, 213; Linder 2003, PRL 90, 091301

JBP, Jassal, Bagla & Padmanabhan, MNRAS 356, L11

Wetterich 2004, PLB 594, 17

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Scalar Field approximation

Cosmological equations

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Scalar Field Dynamics

Take the (Slow-roll) approximation

For Thawing scalar field

Scherrer & Sen 2008, PRD 77, 083515

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approximation

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Thawing scalar fields

Approximate w(z)

dotted curve

short dash curve

long dash curve

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The degeneracy between and

Relation

0th order approximation

Scherrer and Sen 2008, PRD 78, 067303

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SSLCPL model

Taylor Expansion

Gong etal., Int. J. Mod. Phys. 22 (2013) 1350035, 1301.1224

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The accuracy of the approximation

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SSWCPL model

Take approximation

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The accuracy of the approximation

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The degeneracy

Self-consistency

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Flat SSLCPL Results

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Flat SSWCPL Results

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Flat CPL Results

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Comparisons

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Conclusions

The dynamics of scalar fields has some common features

The exists an approximate relation between w and

For thawing models, the dynamics can be approximated by CPL parametrization with degenerated relation between w0 and wa

The reduced degeneracy helps improve the constraint on w(z)

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THANK YOU!