Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012...

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Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang

Transcript of Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012...

Page 1: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

Axion BEC Dark Matter

Pierre Sikivie

Vistas in Axion Physics

Seattle, April 22-26, 2012

Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang

Page 2: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

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: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

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: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

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: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

Axion production by vacuum realignment

2 2 21 1 1 1

1

1

2

1

2( ) ( ) ( ) ( )a a at t t t

tn m a f

GeVT GeVT

V

a

V

a

1

0

3 7

60 1( ) ( )a aa a

R

Rt tm mn

initialmisalignmentangle

Page 6: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

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: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

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 8: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

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 9: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

why do they do that?

by yielding their energy to the

non-condensed particles, the

total entropy is increased.

BECpreBEC

Page 10: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

the axions thermalize and form a BEC after a time

the axion fluid obeys classical field equations

the axion fluid does not obey classical field equations

Page 11: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

the axion BEC rethermalizes

the axion fluid obeys classical field equations

the axion fluid does not obey classical field equations

Page 12: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

Axion field dynamics

From self-interactions

From gravitational self-interactions

Page 13: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

In the “particle kinetic” regime

implies

When

Page 14: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

12

3

4

Page 15: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.
Page 16: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

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

Page 17: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

After , axions thermalize in the “condensed” regime

implies

for

and for self-gravity

Page 18: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

Toy model thermalizing in the condensed regime:

with

i.e.

Page 19: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

50 quanta among 5 states

316 251 system states

Start with

Number of particles

Total energy

Thermal averages

Page 20: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

Integrate

Calculate

Do the approach the on the predicted time scale?

Page 21: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.
Page 22: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

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 23: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

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 24: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

In the linear regime, within the horizon, the axion BEC remains in the same state

axion BEC density perturbations obey

Jeans’ length

42

0 2 4( , ) 2 ( , ) 4 ( , ) 0

4t tk

k t H k t G k tm a

1 1

1 -5 292 42 144

J10 eV 10 g/cc

16 1.02 10 cmG mm

Page 25: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

In the linear regime within the horizon, axion BEC and CDM are indistinguishable on all scales of observational interest,

but

axion BEC differs from CDM when it rethermalizes

in the non-linear regime &

upon entering the horizon

Page 26: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

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 27: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

simulations by Arvind Natarajan

in case of net overall rotation

Page 28: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

The caustic ring cross-section

an elliptic umbilic catastrophe

D-4

Page 29: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

in case of irrotational flow

Page 30: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

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 31: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

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

Page 32: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

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 33: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

Inner Galactic rotation curveInner Galactic rotation curve

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

Page 34: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

Outer Galactic rotation curve

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

Page 35: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

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 36: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

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

Page 37: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

10 arcmin = 2.2 kpc

29.2 kpc15.410.3

Page 38: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

The caustic ring halo model assumes

• net overall rotation

• axial symmetry

• self-similarity

L. Duffy & PSPRD78 (2008)063508

Page 39: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

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 40: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

Tidal torque theory

neighboringprotogalaxy

Stromberg 1934; Hoyle 1947; Peebles 1969, 1971

Page 41: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

Tidal torque theorywith ordinary CDM

neighboringprotogalaxy

the velocity field remains irrotational

v 0 ����������������������������

Page 42: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

For collisionless particles

If initially,

then for ever after.

v v, ) , ) v( , ) v( , )

, )

dr t r t r t r t

dt t

r t

0v =

0v =

Page 43: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

in case of irrotational flow

Page 44: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

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 45: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

For axion BEC

is minimized for given

when .

2

1 2

Ni

i

LE

I

1

N

ii

L L

1 2 3 ... NL L L L

Page 46: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

in case of net overall rotation

Page 47: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

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 48: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

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 49: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

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 50: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

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 51: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

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 52: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

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 53: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

Conclusion:

The dark matter looks like axions

Page 54: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

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 55: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

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 56: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

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

photons cool

baryon to photon ratio

effective numberof neutrinos

Page 57: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.
Page 58: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.
Page 59: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.
Page 60: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

Effective number of neutrinos

WMAP 7 year:

J. Hamann et al. (SDSS):

Atacama Cosmology Telescope:

Page 61: Axion BEC Dark Matter Pierre Sikivie Vistas in Axion Physics Seattle, April 22-26, 2012 Collaborators: Ozgur Erken, Heywood Tam, Qiaoli Yang.

we will see …