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Dark Matter Axions Pierre Sikivie 24 th Rencontres de Blois May 27 – June 1, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang

Dark Matter Axions

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Dark Matter Axions. Pierre Sikivie 24 th Rencontres de Blois May 27 – June 1, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang. Cold dark matter axions thermalize and form a Bose-Einstein condensate. An argument why the dark matter is axions. - PowerPoint PPT Presentation

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Page 1: Dark Matter Axions

Dark Matter Axions

Pierre Sikivie

24th Rencontres de Blois

May 27 – June 1, 2012

Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang

Page 2: Dark Matter Axions

An argument why the dark matter is axions

1. Cold dark matter axions thermalize and form a Bose-Einstein condensate.

2. The axion BEC rethermalizes sufficiently fast that axions about to fall onto a galactic halo almost all go to the lowest energy state for given total angular momentum.

3. As a result the axions produce - caustic rings of dark matter - in the galactic plane - with radii

Page 3: Dark Matter Axions

4. There is observational evidence for the existence of caustic rings of dark matter - in the galactic plane - with radii - with overall size consistent with tidal torque theory

5. The evidence for caustic rings is not explained by other forms of dark matter. Ordinary cold dark matter (WIMPs, sterile neutrinos, non-rethermalizing BEC, …) forms tent-like inner caustics.

Page 4: Dark Matter Axions

There are two cosmic axion populations: hot and cold.

When the axion mass turns on, at QCD time,

1T

1t

1 1 GeVT 9

11

1) 3 10 eV(ap t

t

71 2 10 sect

Page 5: Dark Matter Axions

Cold axion properties

• number density

• velocity dispersion

• phase space density

5 347 31

3 12

( )4 10( )

cm 10 GeV ( )af a t

n ta t

1

1

( )1

( )v( )

a

a t

m t a tt

83 3

6112

34

3

(2 )( ) 10

10 GeV( v)

a

a

fn t

m

N

ifdecoupled

Page 6: Dark Matter Axions

Cold axion properties

• number density

• velocity dispersion

• phase space density

5 347 31

3 12

( )4 10( )

cm 10 GeV ( )af a t

n ta t

1

1

( )1

( )v( )

a

a t

m t a tt

83 3

6112

34

3

(2 )( ) 10

10 GeV( v)

a

a

fn t

m

N

ifdecoupled

Page 7: Dark Matter Axions

Bose-Einstein Condensation

if identical bosonic particles

are highly condensed in phase space

and their total number is conserved

and they thermalize

then most of them go to the lowest energy

available state

Page 8: Dark Matter Axions

why do they do that?

by yielding their energy to the

non-condensed particles, the

total entropy is increased.

BECpreBEC

Page 9: Dark Matter Axions

Axion field dynamics

From self-interactions

From gravitational self-interactions

Page 10: Dark Matter Axions

In the “particle kinetic” regime

implies

When

Page 11: Dark Matter Axions

12

3

4

Page 12: Dark Matter Axions
Page 13: Dark Matter Axions

D. Semikoz & I. Tkachev, PRD 55 (1997) 489D.

Page 14: Dark Matter Axions

After , axions thermalize in the “condensed” regime

implies

for

and for self-gravity

Page 15: Dark Matter Axions

Toy model thermalizing in the condensed regime:

with

i.e.

Page 16: Dark Matter Axions

50 quanta among 5 states

316 251 system states

Start with

Number of particles

Total energy

Thermal averages

Page 17: Dark Matter Axions

Integrate

Calculate

Do the approach the on the predicted time scale?

Page 18: Dark Matter Axions
Page 19: Dark Matter Axions

Thermalization occurs due to gravitational interactions

at time 1t

-1with v)l m

1 ( )( ) / ( ) ( )g a tt H t t a t

2

2

Gm

q

q

PS + Q. Yang, PRL 103 (2009) 111301

Page 20: Dark Matter Axions

Gravitational interactions thermalize the axions and cause them to form a BEC when the photon temperature

After that 1v

m t

3 3( ) / ( ) ( )g t H t t a t

Page 21: Dark Matter Axions

Galactic halos have inner caustics as well as outer caustics.

If the initial velocity field is dominated by net overall rotation, the inner caustic is a ‘tricusp ring’.

If the initial velocity field is irrotational, the inner caustic has a ‘tent-like’ structure.

(Arvind Natarajan and PS, 2005).

Page 22: Dark Matter Axions

simulations by Arvind Natarajan

in case of net overall rotation

Page 23: Dark Matter Axions

The caustic ring cross-section

an elliptic umbilic catastrophe

D-4

Page 24: Dark Matter Axions

in case of irrotational flow

Page 25: Dark Matter Axions

On the basis of the self-similar infall model(Filmore and Goldreich, Bertschinger) with angular momentum (Tkachev, Wang + PS), the caustic rings were predicted to be

in the galactic plane

with radii

was expected for the Milky Way halo from the effect of angular momentum on the inner rotation curve.

1,2,3...n

maxj 0.18

rot max40kpc v j

220km/s 0.18n

na

Page 26: Dark Matter Axions

Effect of a caustic ring of dark matter upon the galactic rotation curve

Page 27: Dark Matter Axions

Composite rotation curve(W. Kinney and PS, astro-ph/9906049)

• combining data on

32 well measured

extended external

rotation curves

• scaled to our own galaxy

Page 28: Dark Matter Axions

Inner Galactic rotation curveInner Galactic rotation curve

from Massachusetts-Stony Brook North Galactic Pane CO Survey (Clemens, 1985)

Page 29: Dark Matter Axions

Outer Galactic rotation curve

R.P. Olling and M.R. Merrifield, MNRAS 311 (2000) 361

Page 30: Dark Matter Axions

Monoceros Ring of stars

H. Newberg et al. 2002; B. Yanny et al., 2003; R.A. Ibata et al., 2003; H.J. Rocha-Pinto et al, 2003; J.D. Crane et al., 2003; N.F. Martin et al., 2005

in the Galactic planeat galactocentric distance appears circular, actually seen forscale height of order 1 kpcvelocity dispersion of order 20 km/s

may be caused by the n = 2 caustic ring of dark matter (A. Natarajan and P.S. ’07)

20 kpcr 0 0100 270l

Page 31: Dark Matter Axions

Rotation curve of Andromeda Galaxyfrom L. Chemin, C. Carignan & T. Foster, arXiv: 0909.3846

Page 32: Dark Matter Axions

10 arcmin = 2.2 kpc

29.2 kpc15.410.3

Page 33: Dark Matter Axions

The caustic ring halo model assumes

• net overall rotation

• axial symmetry

• self-similarity

L. Duffy & PSPRD78 (2008)063508

Page 34: Dark Matter Axions

The specific angular momentum distribution on the turnaround sphere

a

2

m xˆ( , ) ˆ ˆˆ( )( )

nR t

n tt

z nj

2 2

3 9( )R t t

0.25 0.35

Is it plausible in the context of tidal torque theory?

Page 35: Dark Matter Axions

Tidal torque theory

neighboringprotogalaxy

Stromberg 1934; Hoyle 1947; Peebles 1969, 1971

Page 36: Dark Matter Axions

Tidal torque theorywith ordinary CDM

neighboringprotogalaxy

the velocity field remains irrotational

v 0 ����������������������������

Page 37: Dark Matter Axions

in case of irrotational flow

Page 38: Dark Matter Axions

Tidal torque theorywith axion BEC

v 0 ����������������������������

net overall rotation is obtained because, in the lowest energy state,all axions fall with the same angular momentum

Page 39: Dark Matter Axions

in case of net overall rotation

Page 40: Dark Matter Axions

The specific angular momentum distribution on the turnaround sphere

a

2

m xˆ( , ) ˆ ˆˆ( )( )

nR t

n tt

z nj

2 2

3 9( )R t t

0.25 0.35

Is it plausible in the context of tidal torque theory?

Page 41: Dark Matter Axions

Tidal torque theorywith axion BEC

v 0 ����������������������������

net overall rotation is obtained because, in the lowest energy state,all axions fall with the same angular momentum

Page 42: Dark Matter Axions

Magnitude of angular momentum

fits perfectly ( )0.25 0.35

0.05G. Efstathiou et al. 1979, 1987

max 0.18j

from caustic rings

1

2

5

2

max| | 16 8

5 3 10 3

L E

G M

j

Page 43: Dark Matter Axions

The specific angular momentum distribution on the turnaround sphere

a

2

m xˆ( , ) ˆ ˆˆ( )( )

nR t

n tt

z nj

2 2

3 9( )R t t

0.25 0.35

Is it plausible in the context of tidal torque theory?

Page 44: Dark Matter Axions

Self-Similarity

a comoving volume

3

( )

( ) ( , ) ( ( , )V t

t d r r t r r t

( )r a t x ( ) , ) ( )r a t x t x

( )

( , )( , )

t

r tr t

( ) , ) ( ) ( )r a t x t a t x

4 30( ) ( ) ( ) ( ) ( ( ))x

V

t t a t d x x x x

Page 45: Dark Matter Axions

Self-Similarity (yes!)

time-independent axis of rotation

2

3ˆ ˆ( ) ( )t z a t z t

5

3ˆ( )L t z t

1 4 523 9 3( )

ˆ( , )R t

n t t tt

0.33provided

Page 46: Dark Matter Axions

Conclusion:

The dark matter looks like axions

Page 47: Dark Matter Axions

Baryons and photons may enter into thermal contact with the axions by gravitational interactions as well

a

a

p

p

O. Erken, PS, H.Tam and Q. Yang, PRL 108 (2012) 061304

p may be any species of particle

Page 48: Dark Matter Axions

Relativistic axion modes and photons reach thermal contact with the cold axions if the cold axion correlation

length reaches horizon size by the time of equality

Page 49: Dark Matter Axions

If photons, baryons and axions all reach the same temperature before decoupling

photons cool

baryon to photon ratio

effective numberof neutrinos

Page 50: Dark Matter Axions
Page 51: Dark Matter Axions
Page 52: Dark Matter Axions
Page 53: Dark Matter Axions

Effective number of neutrinos

WMAP 7 year:

J. Hamann et al. (SDSS):

Atacama Cosmology Telescope:

Page 54: Dark Matter Axions

we will see …