Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and...

28
Correlations of Mass Distributions Correlations of Mass Distributions between between Dark Matter and Visible Matter Dark Matter and Visible Matter Yuriy Mishchenko and Chueng- Yuriy Mishchenko and Chueng- Ryong Ji Ryong Ji NC State University NC State University Raleigh, NC Raleigh, NC KIAS-APCTP-DMRC Workshop on “The Dark Side of the Universe” May 24, 2005

Transcript of Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and...

Page 1: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.

Correlations of Mass DistributionsCorrelations of Mass Distributionsbetween between

Dark Matter and Visible MatterDark Matter and Visible Matter

Yuriy Mishchenko and Chueng-Ryong JiYuriy Mishchenko and Chueng-Ryong JiNC State University NC State University

Raleigh, NCRaleigh, NC

KIAS-APCTP-DMRC Workshop on “The Dark Side of the Universe” May 24, 2005

Page 2: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.

MotivationMotivation • Universal Rotation Curves in Spiral Galaxies and

Strong Gravitational Lensing in Galaxy Clusters

provide convincing evidences of Dark Matter.• High Resolution Mass Map of CL0024+1654 is

now available from the deep imaging with the Hubble Space Telescope.

• Two dramatically different systems seem to exhibit a consistency in correlations of mass distributions between Dark Matter and Visible Matter.

Y.Mishchenko and C.Ji, PRD68, 063503 (2003)

Page 3: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.

OutlineOutline

• Gravitational Lensing

-Galaxy Clusters CL0024+1654

-Mass Map by Tyson et al.

-Simple but general theromodynamic analysis • Universal Rotation Curves

-Spiral Galaxies with different luminosities

-Consistency with the thermodynamic analysis• Discussions and Conclusions

Page 4: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.

Gravitational Lensing EffectGravitational Lensing Effect

• gravitational lensing is phenomenon of light deflection in gravitational field

• allows to restore 2D projected mass distribution

Einstein Cross Q2237+0305 Einstein Cross Q2237+0305

Page 5: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.

CL0024+1654CL0024+1654

Page 6: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.

Dark vs. Visible in Galaxy ClustersDark vs. Visible in Galaxy Clusters

from J. Tyson, G. Kochanski, I. Dell’Antonio, astro-ph/9801193

Page 7: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.

02.057.0

1007900

)335(

)1(

)1()(

2

1

22

2

pchMK

kpchrr

ry

y

yKy

corecore

Power Law ModelPower Law Model

02.057.0

1007900

)335(

)1(

)1()(

2

1

22

2

pchMK

kpchrr

ry

y

yKy

corecore

02.057.0

1007900

)335(

)1(

)1()(

2

1

22

2

pchMK

kpchrr

ry

y

yKy

corecore

02.057.0

1007900

)335(

)1(

)1()(

2

1

22

2

pchMK

kpchrr

ry

y

yKy

corecore

02.057.0

1007900

)335(

)1(

)1()(

2

1

22

2

pchMK

kpchrr

ry

y

yKy

corecore

Page 8: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.

J. Tyson, G. Kochanski, I. Dell’Antonio, astro-ph/9801193

Page 9: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.

Dark vs. Visible in Galaxy ClustersDark vs. Visible in Galaxy Clusters

• presented analysis of Hubble telescope images of strong gravitational lensing in galaxy cluster CL0024+1654

• presented detailed mass map and radial “averaged” profiles for total and visible matter

• primary conclusion was about inconsistency with Cold Dark Matter simulations (soft core)

J. Tyson, G. Kochanski, I. Dell’Antonio, 1998:J. Tyson, G. Kochanski, I. Dell’Antonio, 1998:

Page 10: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.

Correlation between Dark Matter and Visible Matter

Page 11: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.

• projected density radial profiles presented on log-log scale for the total and visible matter distribution

• if profiles were re-plotted on log-linear scale, one would observe exponential decay

anomalous flat region at about 100kpc in the visible mass profile

Flat Region around 100 kpc

Page 12: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.
Page 13: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.

Thermodynamic PrincipleThermodynamic Principle

)ln(lnlnln

lnln

lnln

:)(

1

:

)( )()(

dvdv

d

v

d

v

dd

vv

ii

i

rri

aa

a

a

potentialnalgravitatior

kT

icomponentofmassmolecular

ear ii

i

Log-Log Linear Correlation

Page 14: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.

4.41.2 4.41.2

4.41.2

4.41.2

Page 15: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.

Dark Matter in Spiral GalaxiesDark Matter in Spiral Galaxies

Rotation Curve represents gas/stars circular orbit velocity as function of distance from the galaxy’s center

spiral galaxy NGC2403

Page 16: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.

Dark vs. Visible in Spiral GalaxiesDark vs. Visible in Spiral Galaxies

• presented analysis of a sample of spiral galaxies’ Rotation Curves classified by galaxy luminosities and normalized to vopt and ropt .

• found that majority of normalized RC in given luminosity group follow universal profiles (Universal Rotation Curves).

• described URC in terms of simple mass model: dark spherical halo + exponential thin stellar disk.

)5.185.23( M

M. Persic, P. Salucci, F. Stel, 1996:M. Persic, P. Salucci, F. Stel, 1996:

Page 17: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.

Universal Rotation Curve of Spiral Galaxy

5.185.23,10

)(5.1

)log(44.072.0

)]6.1()6.1()6.1()6.1([28.1)(

)1)(1()(

)()()(

5/)9.21(

*

5

1

*

*

1100222

22

2222

222

ML

L

L

L

L

L

xKxIxKxIxvxv

x

xv

r

rxv

rvrvrv

M

optv

optopt

d

vdURC

Page 18: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.

Universal Rotation Curves in Spiral GalaxiesUniversal Rotation Curves in Spiral Galaxies

• In Persic, Salucci, Stel visible mass contribution is known but approximated with an analytical fit,

• Dark halo contribution is parameterized,

• Final Rotation Curve is described with

2,)78.0(

97.1)(43.122

22.12

x

x

xxv

v

2,/8615.0)(2 xxxvv

22

222 )1)(1()(

x

xxvd

)()()( 222 xvxvxv dvURC

Page 19: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.

Luminosity Dependence of URCs Luminosity Dependence of URCs

Page 20: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.

Correlation of Mass DensityCorrelation of Mass Density

• URC can be fit in the region 0 r/ropt 2 with exponential dark hallo for all luminosities

• For larger r and are linearly correlated)log( v )log( d

)/exp()( optd rrar

Exponential Thin Disk )/2.3exp( optv rr

It corresponds to T~105 K consistent with the temperatureof the interstellar gas.

Page 21: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.

Dark vs. Visible in Spiral GalaxiesDark vs. Visible in Spiral Galaxies

Page 22: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.

Dark vs. Visible in Spiral GalaxiesDark vs. Visible in Spiral Galaxies

M visible: 3.2 dark: a

-18.5 2.52-2.55 3.2 1.28 2.50

-21.5 1.85-2.03 3.2 0.97 3.31

-23.5 1.56-1.76 3.2 0.78 4.11

best fit values of a for different luminosities M

)/2.3exp()( optv rrr

2.45.2

)/exp()( optd rrar

4.41.2 …remember obtained for CL0024+1654,

Log-Log-Linear Correlation in Spiral GalaxiesLog-Log-Linear Correlation in Spiral Galaxies

Page 23: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.

Dark vs. Visible MatterDark vs. Visible Matter

We observed Log-Log-Linear correlation with essentially the same correlation coefficient in different spiral galaxies and a galaxy cluster.

This is a remarkable coincidence…

How do we interprete?How do we interprete?

Page 24: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.

Interpretation of ResultsInterpretation of Results

• Local Thermodynamic Equilibrium since it is unlikely

that the molar mass ratio varies in a precise correlation

with the temperature ratio to make kappa constant both

for the galaxy clusters and the spiral galaxies.

• Visible matter primarily consists of H, H2 and He.

d

v

d

v

d

v

d

v

d

v

QCDdark

HeHHH

MeVfewaM

MeVMMMMeVM

100

3730,2,9402

QCDdark

HeHHH

MeVfewaM

MeVMMMMeVM

100

3730,2,9402

Massive neutrinos and/or axions < 25MeVWIMP ~ 10GeV-1TeVSUSY lightest particles(e.g. neutralino)>30GeV

Page 25: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.

Discussions and ConclusionsDiscussions and Conclusions

• Correlations of mass distributions between dark matter and visible matter in two dramatically different systems, galaxy cluster and spiral galaxies, are remarkably consistent with each other.

• Based on an almost isothermal Boltzmann distribution, we find K = 2.1~4.4 which indicate the typical mass scale of dark matter particles around the order of 100 MeV.• Since this is right around the QCD mass scale, any relation between the dark matter and QCD vacuum condensates?

Page 26: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.

Things to do:Things to do:• Experimental – improve “statistics”

– large survey of dark vs. visible matter in galaxy clusters…

• Theoretical – investigate different possibilities– role of gravity in thermalization processes…

– better understanding of galaxy cluster dynamics…

– better understanding of spiral galaxy dynamics…

Page 27: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.

-20

-10

0

10

20 0

2

4

6

8

0

10

20

30

40

-20

-10

0

10

20

C.Ji, Gungwon Kang and Jungjai Lee, work in progress…

Page 28: Correlations of Mass Distributions between Dark Matter and Visible Matter Yuriy Mishchenko and Chueng-Ryong Ji NC State University Raleigh, NC KIAS-APCTP-DMRC.