The false vacuum bubble : - formation and evolution -

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The false vacuum bubble : - formation and evolution - in collaboration with Bum-Hoon Lee, Chul H. Lee, Siyong Nam, and Chanyong Park Based on PRD74, 123520 (2006), PRD75, 103506 (2007), arXiv:0710.4599 [hep-th] Wonwoo Lee Sogang University HaengDang Symposium 2007 - Recent Studies in Astro-Particle Physics - Nov. 30.(Fri.) 2007

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HaengDang Symposium 2007 - Recent Studies in Astro-Particle Physics - Nov. 30.(Fri.) 2007. The false vacuum bubble : - formation and evolution -. Wonwoo Lee Sogang University. in collaboration with - PowerPoint PPT Presentation

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Page 1: The false vacuum bubble :       - formation and  evolution -

The false vacuum bubble :

- formation and evolution -

in collaboration withBum-Hoon Lee, Chul H. Lee, Siyong Nam, and Chanyong Park

Based on PRD74, 123520 (2006), PRD75, 103506 (2007), arXiv:0710.4599 [hep-th]

Wonwoo LeeSogang University

HaengDang Symposium 2007- Recent Studies in Astro-Particle Physics

- Nov. 30.(Fri.) 2007

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The plan of this talk1. Motivations, 2. False vacuum bubble nucleation due to a

nonminimally coupled scalar field 1) Numerical calculation 2) Thin-wall approximation

3. The dynamics of a false vacuum bubble : the junction equations

4. Summary and discussions

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1. Motivations -I

What is the origin of our universe?

1) Is our universe created from nothing?

2) Is our universe created from something?

3) Can the universe create itself?

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1. Motivations -II(1) What did the spacetime look like in the very early universe? - Wheeler’s spacetime foam structure - The cosmological constant as a dynamical variable Can we obtain the mechanism for the nucleation of a false vacuum bubble? Can a false vacuum bubble expand within the true vacuum background?

(2) The idea of the string theory landscape has a vast number of metastable vacua. Which mechanism worked to select our universe in this landscape?

Can we be in the vacuum with positive cosmological constant ?(through an alternative way to KKLT, for example)

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2. The Einstein theory of gravity with a nonminimally

coupled scalar fieldVacuum-to-vacuum phase transition rate

Action

Einstein equations

/ exp[ / ]V A B

4 21 1[ ( )]2 2 2RS gd x R U

12

R g R T

2 22

1 1[ ( ) ( )]1 2

T g U g

boundaryS

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curvature scalar

Potential

Rotationally invariant Euclidean metric : O(4)-symmetry

The Euclidean field equations

boundary conditions

2 2( ) ( 2 ) ( 2 )8 2 oU b b U

b

2 2 2 2 2 2 2 2( )[ sin ( sin )]ds d d d d

2

2

1]3)(4[

U

R

3 ''' ' EdURd

22 2

2

1' 1 ( ' )3(1 ) 2

U

0|,)( 0(max)

lim

dd

T

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Our main idea

(during the phase transition)

3 ' 'ER

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1) Numerical calculation(Case 1) from de Sitter to de Sitter

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(Case 2) from flat to de Sitter

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(Case 3) from anti-de Sitter to de Sitter

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(Case 4) from anti-de Sitter to flat

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(Case 5) from anti-de Sitter to anti-de Sitter

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False-to-true True-to-falseDe Sitter – de

Sitter O O

Flat – de Sitter O OAnti-de Sitter –

de Sitter O OAnti-de Sitter –

flat O OAnti-de Sitter – Anti-de Sitter O O

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2)Thin-wall approximation

B is the difference

In this approximation

Outside the wall

b TE EB S S

in wall outB B B B

( ) ( ) 0out E T E TB S S

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In the wall

where

inside the wall

dUUS F

TTo )]()([2

412 4(1 2ln )b bC

22 2 3/ 2

22

2

( )(1 ) {[1 ] 1}3(1 )12 [ ( )]( )

FF

Fin F T

F

U

BU

),(2 232

CSB owall

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(a) false vacuum bubble nucleation

if

6816

3)2(4

4)82( 242

22 CSbbUUbSbH oo

oo

23

83

83

281

29

222222ooooo SUbUbUSE

38256

3264

2364 CSbbCSbD oo

22 H H ED

E

o

4

2

2

1

22

2221

oo

op

/3 oo S )](/3[21 TF UU 2

2 [3/ ( )]F TU U

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The coefficient B

(b) true vacuum bubble nucleation

1

)41(31)41(1

31112

2/3

22

2222/32

2

2

bU

UbU

UB T

T

F

F

6816

3)2(4

4)82( 1242

22

1 CSbbUUbSbH oo

oo

38256

3264 1

23614

1 CSbbCSbD oo

23

83

83

281

29

222222ooooo SUbUbUSE

)

4ln21(12

41

bbC

EEDHH 1

2112

1

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The coefficient B

if (by S. Parke)

where

o

4

2

2

1

22

2221

oo

op

13

11)41(3

11)41(122/322/3

22

222

2

2F

F

T

T

UUb

UUbB

2/14

2

2

1

2

1

2

4

2

2/14

2

2

1

2

1

22211

2

2221

212

ooo

oooo

p

B

B

342 2/27 oo SB

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Two types related to this formalism

(1) Boundary surface

(2) Surface layer In this case it is related to the discontinuity of the extrinsic curvature of the surface. We consider thin-wall partitions bulk spacetime into two distinct manifolds

and with boundaries and , respectively. To obtain the single glued manifold

we demand that the boundaries are identified as follows:

0ijS

0ijS

3. The dynamics of a false vacuum bubble : the junction

equations

M

M MMM

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We consider the action

where

In this framework, junction condition becomes

or

where , a effective negative tension of the wall

There are parameter regions including that both and are positive in all ranges of

4 21 1[ ( )]2 2 2RS gd x R U

twSKxdh )1( 23

),(3

UxdhStw,8 G gg det

rHrHr21)1( 222

)(21 _

22

rHrHr

Hr

r2

2_ 2

,1)( 2rAinH rGMrAoutH 21)( 2

r

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After squaring twice, the equation turns out to be

where the effective potential is

with

PPQTT

rVeff 2)(

2

0)(21 2

rVr eff

222

2

22422222

222222222

222222222

42222222

222222222

22222222

])1(1[

,4)1(4)1]()1(1[

])1(1[4)1](41)1[(

}21]

41)1][()1(1{[2

}]41)1{[(

,}21]

41)1][()1(1{[

)1(])1(1[2])1(1[

PrMG

rGM

GMrAA

rAA

rAAAQ

rAA

rGMT

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(1) M = 0

DS – DS

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DS – FLAT

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DS – ADS

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(2) M > 0

DS – SDS

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DS – S

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DS – SADS

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ER

4. Summary and Discussions• The false vacuum bubble can be nucleated within the true vacuum background with a nonminimally coupled scalar field• expect the phenomenon be possible in many other theories of gravity with similar terms. • A false vacuum bubble with minimal coupling, without singularity in their past, can expand within the true vacuum background with nonminimal coupling.• An expanding false vacuum bubble is not inside the horizon of a black hole from outside observer’s point of view. • Can it be a model for the accelerating expanding universe?

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Thank you for

your attention!