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Equation of State and Transport Coefficients of Relativistic Nuclear Matter Azwinndini Muronga 1,2 1 Centre for Theoretical Physics & Astrophysics Department of Physics, University of Cape Town 2 UCT-CERN Research Centre Department of Physics, University of Cape Town SQM2007

Equation of State and Transport Coefficients of Relativistic Nuclear Matter Azwinndini Muronga 1,2 1 Centre for Theoretical Physics & Astrophysics Department

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Page 1: Equation of State and Transport Coefficients of Relativistic Nuclear Matter Azwinndini Muronga 1,2 1 Centre for Theoretical Physics & Astrophysics Department

Equation of State and Transport Coefficients of Relativistic Nuclear Matter

Azwinndini Muronga1,2

1Centre for Theoretical Physics & AstrophysicsDepartment of Physics, University of Cape Town

2UCT-CERN Research CentreDepartment of Physics, University of Cape Town

SQM2007

24-29 June 2007, Levoča, Slovakia

Page 2: Equation of State and Transport Coefficients of Relativistic Nuclear Matter Azwinndini Muronga 1,2 1 Centre for Theoretical Physics & Astrophysics Department

Transport properties of relativistic nuclear matter

Viscosities, diffusivities, conductivities.

Determine relaxation to equilibrium in heavy ion collisions – strangeness equilibration (by flavor diffusion), spin and color diffusion

In astrophysical situations such as in neutron stars – cooling and burning of neutron star into a strange quark star

In cosmological applications such as the early universe – electroweak baryogenesis

QED and QCD plasmas

Baym et. al., Gavin, Prakash et. al., Davesne, Heiselberg, Muroya et. al., Muronga, Arnold et. al.,….

Page 3: Equation of State and Transport Coefficients of Relativistic Nuclear Matter Azwinndini Muronga 1,2 1 Centre for Theoretical Physics & Astrophysics Department
Page 4: Equation of State and Transport Coefficients of Relativistic Nuclear Matter Azwinndini Muronga 1,2 1 Centre for Theoretical Physics & Astrophysics Department

Origin of the news:

Page 5: Equation of State and Transport Coefficients of Relativistic Nuclear Matter Azwinndini Muronga 1,2 1 Centre for Theoretical Physics & Astrophysics Department
Page 6: Equation of State and Transport Coefficients of Relativistic Nuclear Matter Azwinndini Muronga 1,2 1 Centre for Theoretical Physics & Astrophysics Department

14-field theory of relativistic dissipative fluid dynamics

Primary variables

Conservation of net charge, energy-momentum and balance of fluxes

qquqqqsuS

CCuqBCuuACP

uFqFuuqFuFuuuFF

uqpuuT

nuN

q

qq

10212

0

012

12121

2

15

12)3(

3

4

633

2)(

02

5

1

4

0

0

0

11211

0

1

2

qqS

CCF

qBCFu

ACFuu

T

Tu

N

q

See A. Muronga, nuc-th/0611090 for details

Page 7: Equation of State and Transport Coefficients of Relativistic Nuclear Matter Azwinndini Muronga 1,2 1 Centre for Theoretical Physics & Astrophysics Department

Relaxation equations for dissipative fluxes

Relaxation equations for the dissipative fluxes

Transport and relaxation times/lengths

q

aT

TTqq

q

q

qqq

q

2

CCCB

TCA q

20

21

22 2

5 , ,16

1100

210

2 , , ,

2 , ,

qqqq

q

TT

T

Page 8: Equation of State and Transport Coefficients of Relativistic Nuclear Matter Azwinndini Muronga 1,2 1 Centre for Theoretical Physics & Astrophysics Department

Transport Coefficients and Relaxation Times/Lengths

Relativistic transport equation

Phase-space integrals

),(),( processes

)( pxIpxFpk

kaa

in out in out

outinnj

n

ijji

ka

jFjjjF

PPppMpdS

pxI

)()()()(

)(2),...,(1

)(),( )4(42

11

4)(

31

0

10

2

Fermions 1

Boltzmann 0

Bosons 1

)(1)(

gA

jFAj

pe

AjF1

)( 00

See A. Muronga, nuc-th/0611091 for details

Page 9: Equation of State and Transport Coefficients of Relativistic Nuclear Matter Azwinndini Muronga 1,2 1 Centre for Theoretical Physics & Astrophysics Department

Transport Coefficients and Relaxation Times/Lengths

For any scalar function of distribution function and any tensor function of momenta

After linearization within relativistic Grad moment method

in out in out

outinnj

n

ijji

jFjjjF

pFdwPPppMpdS

dwppF

)()()()(

)()()(2),...,(1

)(

)()(

')4(42

11

4

)()( 4

100

4

in out

jjFppppWwdC

CuuCCCCuuuuC q 3

1 ,

3

1 ,

cCF

ppxcpxbxapx

jjjFjF

)()()(),(

)()(1)()( 00

Page 10: Equation of State and Transport Coefficients of Relativistic Nuclear Matter Azwinndini Muronga 1,2 1 Centre for Theoretical Physics & Astrophysics Department

Relaxation Coefficients

Page 11: Equation of State and Transport Coefficients of Relativistic Nuclear Matter Azwinndini Muronga 1,2 1 Centre for Theoretical Physics & Astrophysics Department

• Transport coefficients are as important as the equation of state.

• They should be calculated self consistently together with the equation of state.

• The relaxation times/lengths should be compared with the characteristic time/length scales of the system under consideration.

• Strangeness equilibration could be easily understood via strangeness (flavor) diffusion coefficient.

• Looking forward to talks by W. Broniowski and by L. Turko at this meeting.

Looking beyond an idealistic picture