Bose-Einstein Condensation of Dark Matter Axions · • axion BEC and CDM are indistinguishable in...
Transcript of Bose-Einstein Condensation of Dark Matter Axions · • axion BEC and CDM are indistinguishable in...
Bose-Einstein Condensationof Dark Matter Axions
Pierre Sikivie
Texas Cosmology Network MeetingAustin, October 29-30, 2009
The Dark Matter is Axions
based on arXiv: 0901.1106with Qiaoli Yang
I’ll argue:
How so?
• axions differ from ordinary CDM because they form a BEC, and the axion BEC continues to rethermalize, tracking the lowest energy state.
• axion BEC appears to solve two puzzles with CDM 1) evidence for caustic rings of dark matter implies that the dark matter falls onto galactic halos with ``net overall rotation", implying whereas CDM predicts ,
2) unexpected alignments among CMBR multipoles .
0v! # r r
0v =! r r
Outline• Review of axion properties
• Cold dark matter axions form a rethermalizing Bose-Einstein condensate
• Axion BEC differs from ordinary CDM
• Compare CDM and axion BEC density perturbations withobservations in three arenas
1. upon entering the horizon 2. in the linear regime within the horizon 3. in the non-linear regime
CDMaxionBEC
f f
a
a
!!
610 GeVeVa
af
m
6
= 0.97 in KSVZ model 0.36 in DFSZ model
g!
5fa f f
a
L i g f ff
!" =
a
a
L g E Bf
!! !
" #
$ = %
ur ur
The remaining axion window
laboratory searches
510
1510
1010 (GeV)af
(eV)am1
510
! 1010
!
stellar evolution
cosmology
There are two axionpopulations: hot and cold.
When the axion mass turns on, at QCD time,
1T
1t
11 GeVT
7
12 10 sect
! "
9
1
1
1) 3 10 eV(ap t
t
! = "
Axion production by vacuum realignment
GeVT ! 1 GeVT ! 1
V
a
V
a
initialmisalignmentangle
2 2 2
1 1 1 1
1
1
2
1
2( ) ( ) ( ) ( )a a at t t t
tn m f !"
1
0
3 7
60 1( ) ( )
a aa a
at t
am mn!
"# $ % & '
( )
Cold axion properties
• number density
• velocity dispersion
• phase space density
5347
31
3 12
( )4 10( )
cm 10 GeV ( )
af a tn t
a t
! "# ! " $ %$ %
& ' & '
1
1
( )1
( )v( )
a
a t
m t a tt!
83
361
1234
3
(2 )( ) 10
10 GeV( v)
a
a
fn t
m!
!
"
# $ % &
' (
N
ifdecoupled
The cold axions thermalize andtherefore form a BEC
2
2
0 4 5
6
cm10 eV
m m
f!
"#105
#
1 $ % = 1.5 &10 ' (
64 ) *
a
a a
a
2
4
2...a
m
f!
1 +
4! = ... + L
0( ) v( ) ( )n t t H t! " << but …
At high phase space density
D. Semikozand I. Tkachev,1995, 1997
2
scatt 0vn ! "# N
relax 0vn ! "# N
scattering rate
thermalization rate
61( 10 ) N
relax 1 1(t H t! ( ) )
A critical aspect of axion BECphenomenology is whether the BECcontinues to thermalize after it has formed.
Axion BEC means that almost all axions goto one state.
However, only if the BEC continuallyrethermalizes does the axion state trackthe lowest energy state.
After the thermalization ratedue to self-interactions is
at time
3 1( )( ) / ( ) ( ) a tt H t t a t!" "
# $ $
Self-interactions are insufficient to rethermalize axion BEC after t1even if they cause axion BEC at t1.
1t
1t
2
H
n m!
!
! "#
# / $(1)
However, the thermalization ratedue to gravitational interactions
at time1t
-1with v)l m!= (
1 ( )( ) / ( ) ( )g a tt H t t a t !" # #
2
3
12
2 2
10 GeV
g
gf
H
G n m l
!8
" # / 4 $10 % &
' (
)
)
Gravitational interactions thermalize theaxions and cause them to form a BECwhen the photon temperature
After that
12
12eV10 GeV
fT!
" #100 $ %
& '
1v
m t!
3 3( ) / ( ) ( )g t H t t a t!
" #
axion BEC
Except for a tiny fraction, all axions are in thesame state
2( ) [ ] ( ) ( )D x g x m xDµ µ! "µ µ ! µ! "# # # = $ $ % & $ =
†( ) [ ( ) ( ) ]x a x a x! ! ! ! !" #= $ % %+
0
†1| (
!) | 0N
N
N
a> = >
( 0)! =
N is the number ofaxions
in a homogeneousand isotropicspace-time.
0 3
2( )
im tA
a t
e!
" =
0 0 0 0
2
0 0 0 0
|
( )]
| [N T
g m
N Nµ! µ ! ! µ
"µ! "
# #
# #
< $ % $ + $ % $
+ &% $ $ & $ $
> = % %
%
In Minkowski space-time
Let
then
Let
then
0 ( ) ( )imtx e x
!" = #
21
2t
im
! " ## = $for non -relativisticmotion
( , )1( , ) ( , )
2
i x tx t B x t
mN
e!
" =rr r
2
00 ( , ) ( , ) ( , )( )T x t x t m B x t!" =r r r
hence
2
0vj j jT B !" = # $% #
1v( , ) = ( , )x t x t
m!"
rr r r
2
2
1 1
4v v ( )j jjk k k jkT
m! ! " !
!! + # # $ %=
stresses related to the Heisenberg uncertaintyprinciple tend to homogenize the axion BEC
We have
and
with
( v) 0t! !" #+ $ =
ur ur
( )v v vt q! + "# = $#ur ur ur ur ur
2
2
1
2mq
!
!
"= #
To recover CDM, let m go to infinity
In the linear regime,within the horizon,
axion BEC density perturbations obey
Jeans’ length
42
0 2 4( , ) 2 ( , ) 4 ( , ) 0
4t t
kk t H k t G k t
m a! ! " # !
$ %& + & ' ' =( )
* +
r r r
( )
1 11 -5 292 4
2 144J
10 eV 10 g/cc16 1.02 10 cmG m
m! "
"
#$ % $ %= & ' ( ' (
) * ) *=l
In the linear regime within thehorizon, axion BEC and CDM areindistinguishable on all scalesof observational interest,
but
axion BEC differs from CDMin the non-linear regime &upon entering the horizon
CMBmultipoles
arealigned
quadrupole:
octupole: M. Tegmark, A. de Oliveira-CostaA. Hamilton, 2003
C. CopiD. HutererD. SchwarzG. Starkman, 2006
Upon entering the horizon
CDM density perturbations evolve linearly
the density perturbations in the axion BEC evolve non-linearly because the axionBEC rethermalizes upon entering the horizon.
axion BEC provides a possible mechanism for the alignment of CMBR multipoles through the ISW effect.
x
x.
DM particles in phase space
DM forms caustics in the non-linear regime
x
xx
.x
! !
Phase space structure ofspherically symmetric halos
(from Binney and Tremaine’s book)
Phase space structure ofspherically symmetric halos
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).
simulations by Arvind Natarajan
The caustic ring cross-section
an elliptic umbilic catastrophe
D-4
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).
On the basis of the self-similar infall model(Filmore and Goldreich, Bertschinger) with angularmomentum (Tkachev, Wang + PS), the causticrings were predicted to be
in the galactic plane with radii
was expected for the Milky Wayhalo from the effect of angular momentumon the inner rotation curve.
( )1,2,3...n =
maxj 0.18!
rot max40kpc v j
220km/s 0.18n
na
! "! "= # $# $
% &% &
Effect of a caustic ring of dark matter uponthe galactic rotation curve
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
Inner Galactic rotation curveInner Galactic rotation curve
from Massachusetts-Stony Brook North Galactic Pane CO Survey (Clemens, 1985)
Outer Galactic rotation curve
R.P. Olling and M.R. Merrifield, MNRAS 311 (2000) 361
Monoceros Ring of starsH. 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 distanceappears circular, actually seen forscale height of order 1 kpcvelocity dispersion of order 20 km/s
may be caused by the n = 2 caustic ring ofdark matter (A. Natarajan and P.S. ’07)
20 kpcr 0 0100 270l < <
from L. Duffy and PS, Phys. Rev. D78 (2008) 063508
Tidal torque theory with CDM
The velocity field remains irrotational
v 0! =ur r
neighboringprotogalaxy
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
! ( = ( + "#
!
= $#%(
r r rr r r r r r
r r
0v =! " r r
0v =! " r r
Tidal torque theory with axion BEC
Net overall rotation is produced because, in thelowest energy state, all axions fall with the sameangular momentum
v 0!" #ur r
For axion BEC
is minimized for given
when .
2
1 2
N
i
i
LE
I=
= !
1
N
i
i
L L
=
= !
1 2 3...
NL L L L= = = =
is allowed through theappearance of vortices; see discussionby Tanja Rindler-Daller and Paul Shapiroat this meeting.
v 0!" #ur r
Summary
• axion BEC and CDM are indistinguishable in the linear regime inside the horizon on all scales of observational interest.
• axion BEC may provide a mechanism for net overall rotation in galactic halos.
• axion BEC may provide a mechanism for the
alignment of CMBR multipoles.