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Screening mechanism and dark coupling Kazuya Koyama Institute of Cosmology and Gravitation University of Portsmouth

Screening mechanism and dark couplingmaccio/ringberg/Talks/Koyama.pdfVainshtein mechanism originally discussed in massive gravity rediscovered in DGP brane world model linear theory

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Page 1: Screening mechanism and dark couplingmaccio/ringberg/Talks/Koyama.pdfVainshtein mechanism originally discussed in massive gravity rediscovered in DGP brane world model linear theory

Screening mechanism and dark

coupling

Kazuya Koyama

Institute of Cosmology and Gravitation

University of Portsmouth

Page 2: Screening mechanism and dark couplingmaccio/ringberg/Talks/Koyama.pdfVainshtein mechanism originally discussed in massive gravity rediscovered in DGP brane world model linear theory

General relativity

Why do we believe general relativity?

Observational point of view

GR is tested to very high accuracy by solar system

experiments and pulsar timing measurements

Theoretical point of view

GR is the unique metric theory in 4D that gives second order

differential equations

C. Will gr-qc/0510072

Page 3: Screening mechanism and dark couplingmaccio/ringberg/Talks/Koyama.pdfVainshtein mechanism originally discussed in massive gravity rediscovered in DGP brane world model linear theory
Page 4: Screening mechanism and dark couplingmaccio/ringberg/Talks/Koyama.pdfVainshtein mechanism originally discussed in massive gravity rediscovered in DGP brane world model linear theory

Brans-Dicke theory

Action

f(R) gravity:

quasi-static approximations (neglecting time derivatives)

24 ( )BDS d x R V

2 2 2 2(1 2 ) ( ) (1 2 )ds dt a t dx 0

2

2 2

(3 2 ) 8

14

2

BD G

G

0BD

2 2

0 plV H M

Page 5: Screening mechanism and dark couplingmaccio/ringberg/Talks/Koyama.pdfVainshtein mechanism originally discussed in massive gravity rediscovered in DGP brane world model linear theory

Constraints on BD parameter

Solutions

PPN parameter

This constraint excludes any detectable modifications in cosmology

1

2

BD

BD

51 (2.1 2.3) 10 40,000BD

2

2

1

(3 2 ) 8

4 2 4 24 ,

3 2 3 2

2

1

BD

BD BDeff

BD BD

BD

BD

G

G G G

Page 6: Screening mechanism and dark couplingmaccio/ringberg/Talks/Koyama.pdfVainshtein mechanism originally discussed in massive gravity rediscovered in DGP brane world model linear theory

How we suppress fifth force (1)

Break equivalent principle

Einstein frame

Remove coupling to baryons (Interacting dark energy)

Jordan frame

the coupling compensates the fifth force acting on baryons

(however, interpretation of observations is non-trivial)

2 /4 1

( ) [ ]2

plM

E mS d x g R V L e g

1

3 2 BD

2 /4 1

( ) [ ] [ ]2

plM

E DM baryonS d x g R V L e g L g

24 ( ) [ ] [ ( ) ]BD

DM baryonS d x R V L g L f g

Wetterich ,

Amendora

Baldi’s talk

Deruelle, Sasaki 1012.5386

Page 7: Screening mechanism and dark couplingmaccio/ringberg/Talks/Koyama.pdfVainshtein mechanism originally discussed in massive gravity rediscovered in DGP brane world model linear theory

How to suppress the fifth force (2)

GR is recovered if (i) the mass is large or

(ii) the kinetic term is large

These limits should be realised in environmentally (density)

dependent way to avoid the recovery of GR on all scales

24 ( )

( ) [ ]BDmS d x R V L g

BD

''V

Page 8: Screening mechanism and dark couplingmaccio/ringberg/Talks/Koyama.pdfVainshtein mechanism originally discussed in massive gravity rediscovered in DGP brane world model linear theory

Chameleon/symmetron/dilaton

Einstein frame

24 21

( ) [ ( ) ]2

E mS d x g R V L A g

( ), ( ) ( ) ( ( ) 1)eff effV V V A

Talks by Brax, Davis, Khoury, Li, Hu,..

Local tests forbid the modification above a few Mpc Khoury’s talk

Page 9: Screening mechanism and dark couplingmaccio/ringberg/Talks/Koyama.pdfVainshtein mechanism originally discussed in massive gravity rediscovered in DGP brane world model linear theory

How to suppress the fifth force (3)

Vainshtein mechanism

originally discussed in massive gravity

rediscovered in DGP brane world model

linear theory

even if gravity is weak, the scalar can be non-linear

2

2 2

3 8

14

2

G

G

2

2 2 2 23 8i j

c i jr Ga 1 1

0cr m H

0BD

Talks by Hu, Hui

Page 10: Screening mechanism and dark couplingmaccio/ringberg/Talks/Koyama.pdfVainshtein mechanism originally discussed in massive gravity rediscovered in DGP brane world model linear theory

Vainshtein mechanism

Spherically symmetric solution for the scalar

3 3

2

2( ), ( ) 1 1

3

g V

V

rd r rr r

dr r r r

12 38

, 29

c g

V g

r rr r GM

2

2

,2 2

2 2

g g

c

g g

c

r r r

r r

r r r

r r

4D BD

2,

2 3

4

2 3

g

g

r

r

r

r

4D Einstein

gr Vrcr

2.95km 0.1 kpc 3000Mpc for the Sun

Page 11: Screening mechanism and dark couplingmaccio/ringberg/Talks/Koyama.pdfVainshtein mechanism originally discussed in massive gravity rediscovered in DGP brane world model linear theory

Solar system constraints

The fractional change in the gravitational potential

The anomalous perihelion precession

The vainshtein radius is shorter for a smaller object

Lunar laser ranging: the Erath-moon distance

2r rr r r

54.1 10 kmE Mr

1/23

11

2

32.4 10 ,

4 8

pl E ME M V

c

M rr r

r M

60 1 1

010c plr M H Dvali et.al 0212069

Burrgae & Seery 1005.1927

Local tests are beginning to exclude the acceleration from new physics

Page 13: Screening mechanism and dark couplingmaccio/ringberg/Talks/Koyama.pdfVainshtein mechanism originally discussed in massive gravity rediscovered in DGP brane world model linear theory

Observational implications (1) equivalence violation

(1) Equivalence violation

interacting dark energy model (Einstein frame)

modified gravity models (Jordon frame)

BD IDE

A combination of weak lensing and RSD

can break the degeneracy

(i.e. Eg parameter)

2 2( ) 4 ( , ) m mk Ga a k

2 24 ( , ) m mk Ga a k

( , ) 1

2(2 )( , )

3 2

BD

BD

a k

a k

BD

IDE ( )

Reyes’s talk

Page 14: Screening mechanism and dark couplingmaccio/ringberg/Talks/Koyama.pdfVainshtein mechanism originally discussed in massive gravity rediscovered in DGP brane world model linear theory

Tidal disruption of satellite galaxies

Observational implications (1) equivalence violation

An enhanced force acting on

DM redistribute stars from the

leading stream to the trailing

stream

10% enhancement of DM force

would be excluded

Kesden, Kamionkowski

astro-ph/0608095

Page 15: Screening mechanism and dark couplingmaccio/ringberg/Talks/Koyama.pdfVainshtein mechanism originally discussed in massive gravity rediscovered in DGP brane world model linear theory

Observational implication (2) Environmental screening

(2) Environmental dependent screening

dark matter halos

screening depends on environment and halo mass

Schmidt 1003.0409, Zhao, Li Koyama 1011.1257

Li, Zhao, Koyama 1111.2602

[0 :1/ 3]M

difference between

lensing and dynamical

mass cf. f(R) gravity

Zhao’s talk

Page 16: Screening mechanism and dark couplingmaccio/ringberg/Talks/Koyama.pdfVainshtein mechanism originally discussed in massive gravity rediscovered in DGP brane world model linear theory

Apparent violation of equivalent principle

The rotation curve of HI gas is enhanced compare with stars

The stellar disk is displaced from the HI gas disk

If we can use dwarf galaxies in voids that have shallower

potentials than the Milky way, we can go beyond local tests

HI gas:

unscreened

Stellar disk:

screened

Hui, Nicolis, Stubbs 0905.2966

Jain & VanderPlas 1106.0065

Observational implication (2) Environmental screening

Page 17: Screening mechanism and dark couplingmaccio/ringberg/Talks/Koyama.pdfVainshtein mechanism originally discussed in massive gravity rediscovered in DGP brane world model linear theory

Creating a screening map

It is essential to find places where GR is not recovered

Small galaxies in underdense regions

SDSS galaxies within 200 Mpc

GR is recovered

Cabre, Vikram, Zhao, Jain, KK

1204.6046

5

0| | 10Rf

6

0| | 10Rf

Page 18: Screening mechanism and dark couplingmaccio/ringberg/Talks/Koyama.pdfVainshtein mechanism originally discussed in massive gravity rediscovered in DGP brane world model linear theory

Observational implication (3) Vainshtein mechanism

(3) Vainshtein mechanism

dark matter halos

Screening depends on environment and mass very weakly

Schmidt 1003.0409

Page 19: Screening mechanism and dark couplingmaccio/ringberg/Talks/Koyama.pdfVainshtein mechanism originally discussed in massive gravity rediscovered in DGP brane world model linear theory

Morphology dependence

The non-linear term vanishes for 1D plane wave

screening is weak in filaments

Apparent equivalent principle violation

stars can feel an external field

generated by large scale structure but a

black hole does not due to no hair

theorem

central BH lag behind stars

2

2 i j

i j

BH

Observational implication (3) Vainshtein mechanism

Hui, Nicolis 1201.1508

Hui’s talk

Page 20: Screening mechanism and dark couplingmaccio/ringberg/Talks/Koyama.pdfVainshtein mechanism originally discussed in massive gravity rediscovered in DGP brane world model linear theory

Non-superposition

Two body problem (cf. Earth-moon)

Observational implication (3) Vainshtein mechanism

Hiramatsu, Hu, KK, Schmidt

Page 21: Screening mechanism and dark couplingmaccio/ringberg/Talks/Koyama.pdfVainshtein mechanism originally discussed in massive gravity rediscovered in DGP brane world model linear theory

Near a small body B (moon)

the interference term cancels the second derivative of the field

from the large body (Earth) 2 2

2 2 2| | | |

A

A

P

Observational implication (3) Vainshtein mechanism

2 2 ( / )A A BO M M

Earth

Moon

Page 22: Screening mechanism and dark couplingmaccio/ringberg/Talks/Koyama.pdfVainshtein mechanism originally discussed in massive gravity rediscovered in DGP brane world model linear theory

Effects on the first derivative (force) is small

There is a 5-10% effect on the

fifth force from the interference term

Observational implication (3) Vainshtein mechanism

1

| |

| | | |

A

A

P

Earth

Moon

Page 23: Screening mechanism and dark couplingmaccio/ringberg/Talks/Koyama.pdfVainshtein mechanism originally discussed in massive gravity rediscovered in DGP brane world model linear theory

Challenge for simulations

Screening mechanism

governed by a non-linear Poisson equation

no superposition rule

it is not possible to separate long and short range forces

need to solve the non-linear Poisson equation on a mesh

MLAPM

ECOSMOG

(based on

RAMSES)

ECOSMOG-Vainshtein simulations are underway Li, Zhao, Koyama

2 24 ( ) '( ) [ , ]GA V N

Li, Zhao 0906.3880, Li, Barrow 1005.4231

Zhao, Li, Koyama 1011.1257

Li, Zhao, Teyssier, Koyama 1110.1379

Jennings et.al. 1205.2698, Li et.al. 12064317

Brax et.al. 1206.3568

Oyaizu et.al, Schmidt et.al.

Schimidt 0905.0858, 0910.0235 Chan & Scoccimarro 0906.4548

Page 24: Screening mechanism and dark couplingmaccio/ringberg/Talks/Koyama.pdfVainshtein mechanism originally discussed in massive gravity rediscovered in DGP brane world model linear theory

Conclusion

Modification of GR

generally introduce the fifth force, which should be screened

1) break equivalence principle and remove coupling to baryons

Einstein frame - interacting dark energy models

2) Environmentally (density) dependent screening

Chameleon/Symmetron/dilaton models

3) Vainshtein mechanism

massive gravity, Galileon models, braneworld models

Non-linearity of the Poisson equation for the fifth force leads to rich phenomenology