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Neda Sadooghi Department of Physics Sharif University of Technology Tehran-Iran

Improved ring potential of QED at finite temperature and in the presence of weak and strong magnetic field. Neda Sadooghi Department of Physics Sharif University of Technology Tehran-Iran Prepared for PASCOS-08, Waterloo, ON, Canada June 2 – 6, 2008.

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Neda Sadooghi Department of Physics Sharif University of Technology Tehran-Iran

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  1. Improved ring potential of QED at finite temperature and in the presence of weak and strong magnetic field Neda Sadooghi Department of Physics Sharif University of Technology Tehran-Iran Prepared for PASCOS-08, Waterloo, ON, Canada June 2 – 6, 2008

  2. QED Effective Potential at Nonzero T and B

  3. QED Effective (Thermodynamic) Potential at Finite T and in a Background Magnetic Field Approximation beyondthe static limit k = 0 • Full QED effective potential consists of two parts • The one-loop effective potential • The ring potential

  4. QED One-Loop Effective Potential at Finite T and B • T independent part • T dependent part

  5. QED Ring Potential at Finite T and B • QED ring potential • Using a certain basis vectors defined by the eigenvalue equation of the VPT(Perez Rojas & Shabad ‘79)

  6. The free photon propagator in the Euclidean space • VPT at finite T and in a constant B field( Perez Rojas et al. ‘79) • Orthonormality properties of eigenvectors  Ring potential  Ring potential in the IR limit (n=0)

  7. Ring Potential of QED for Finite B and T • IR limit (n=0)

  8. The integrals ( Alexandre 2001)

  9. IR vs. Static Limit • Ring potential in the IR limit • In the static limitk 0 

  10. QED Ring Potential in Weak B Field Limit

  11. Weak B Field Limit • Characterized by: and • Evaluating in eB 0 limit • In the IR limit • In the static limit

  12. QED ring potential in the IR limit and weak magnetic field  In the high temperature expansion  In the limit • Comparing to the static limit, an additional term appears • Well-known terms in QCD at finite T HTL expansionBraaten+Pisarski (’90)

  13. QED Ring Potential in Strong B Field Limit

  14. QED in a Strong Magnetic Field at zero T • Characterized by Landau levels as in non-relativistic QM • For strong enough magnetic fields the levels are well separated and Lowest Landau Level (LLL) approximation is justified  In the LLLA, an effective QFT replaces the full QFT

  15. Properties at zero T: • Dynamical mass generation • Dynamical chiral symmetry breaking • Bound state formation • Dimensional reduction from D  D-2 • Two regimes of dynamical mass • Photon is massive in the 2nd regime:

  16. QED Ring Potential in Strong B Field Limit at nonzero T • Characterized by: • Evaluating in limit • QED ring potential in the IR limit with

  17. QED ring potential in the IR limit and strong magnetic field  In the high temperature limit  Comparing to the static limit • From QCD at finite T  Toimela (’83)

  18. Dynamical Chiral Symmetry Breaking in the LLL

  19. QED Gap Equation in the LLL • QED in the LLL Dynamical mass generation • The corresponding (mass) gap equation • Using • Gap equation  where

  20. One-loop Contribution: • Dynamical mass • Critical temperature Tc of DSB is determined by

  21. Ring Contribution • Dynamical mass • Critical temperature of DSB • Tc in the: • IR Limit • Static Limit  

  22. Critical Temperature of DSB in the IR Limit • Using • The critical temperature Tc in the IR limit • where is a fixed, T independent mass (IR cutoff) • and

  23. Critical Temperature of DSB in the Static Limit • Using • The critical temperature Tc in the static limit

  24. IR vs. Static Limit Question: How efficient is the ring contribution in the IR or static limits in decreasing the Tc of DSB arising from one-loop EP? • The general structure of Tc  To compare Tc in the IR and static limits, define • IR limit • Static limit

  25. Define the efficiency factor where and the Lambert W(z) function, staisfying • It is known that

  26. Numerical Results Choosing , and • Astrophysics of neutron stars • RHIC experiment (heavy ion collisions)

  27. Concluding Remarks

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