1. Nucleon PDF inside Compressed Nuclear Matter Jacek Rozynek NCBJ Warsaw ‘‘Is it possible to maintain my volume constant when the pressure increases?” - an nucleon when entering the compressed medium. J. Phys. G: Nucl. Part. Phys. 42 (2015) 045109. Nuclear Entalpies, 1311.3591; Pressure Corrections to the Equation of State in the Nuclear Mean Field, 1205.0431, Acta Phys. Pol. B Proc. Suppl. Vol. 5 No 2 (2012) 375 Valparaiso QNP2015

2. Introduction The aim is to check two approximations of The nuclear Relativistic Mean Field Model 1. constant nucleon mass 2. no nucleon volumes i compressed NM Possible applications in HI colisions and inside neutron stars. Valparaiso QNP2015

3. Finite volume effect in compressed medium Nucleon inside saturated NM Compressed inside Neutron Star or in H I collision Nucleon pressure

4. Two Scenarios for NN repulsion with qq attraction Constant Volume = Constant Enthalpy Constant Mass = Increasing Enthalpy 1/R Valparaiso QNP2015 ΩAΩA ΩNΩN ΩNΩN

5. Two Scenarios affecting nuclear compressibility K A -1 Constant Volume = Constant Enthalpy Constant Mass = Increasing Enthalpy 1/R Valparaiso QNP2015

6. Definitions Enthalpy is a measure of the total energy of a thermodynamic system. It includes the system's internal energy and thermodynamic potential (a state function), as well as its volume Ω and pressure p H (the energy required to "make room for it" by displacing its environment, which is an extensive quantity). H A = E A + p H Ω A Nuclear Enthalpy (1) H N = M pr + p H Ω N Nucleon Enthalpy (2) Specific Enthalpies (3) h A (      p H  h N (  ) = H N /M pr = 1+ p H /(  cp M pr  Valparaiso QNP2015

7. Enthalpy vs Hugenholz - van Hove relation with chemical potential (1a) Valparaiso QNP2015 Also valid for constant nucleon volumes !!

8. Nuclear convolution model f N (y) Light cone variables in the rest frame x=k + /p N + y=p N + /P A

9. RMF and Momentum Sum Rule Frankfurt, Strikman Phys. Reports 160 (1988) (4) Valparaiso QNP2015 (Jaffe)

10. Finally with a good normalization of S N we have: and Momentum Sum Rule Flux Factor Fermi Energy Enthalpy/A B - =B 0 -B 3 B-B- q=0 kk No NN pairs baryon current P 0 A =E A =A  A Valparaiso QNP2015

11. Bag Model in Compress Medium p H =0 (7) Valparaiso QNP2015

12. Nucleon compressibilty and two scenarios Constant Nucleon Mass Constant Nuclear Radius Semi-experimental Value sum rules K N -1 =>M E x 2 (Morsch, Julich, PRL 1995) From 7Gev/c (α,p) scattering in P 11 region in SATURN

13. K -1 =235MeVfm -3 Nuclear compressibility for different constant nucleon radii in compressed NM Nucleon Mass for different nucleon radii in compressed NM Our version of Hugenholz-Van Hove relation for finite nucleons in NM Valparaiso QNP2015

14. Nucleon radius in compressed NM for a constant nucleon mass Bag constant in function of nuclear pressure Valparaiso QNP2015

15. RMF Equation of State for const Enthalpy scenario B (8) (9) Valparaiso QNP2015

16. Equation of state - different models Valparaiso QNP2015

17. Results Valparaiso QNP2015 SASA SBSB

18. Two possible scenario of phase transition A - constant nucleon radius, B - constant nucleon mass Energy alignment  cr  (  cr ) =  cp M(  cr ) R[fm]=0.8 -> 0.69 3rd International Conference on New Fronties in`Physics Valparaiso QNP2015

19. A model for parton distribution σ =1/(2R) k + = xp + Kinematical conditions for Monte Carlo technique Primodial quark transverse momentum distribution Line cone variables in the nucleon rest frame COMPRESSED Nuclear Case p + rest = H N (R)

23. Nuclear Models - equilibrium JR G.Wilk PLB 473 (2000) Only 1% of nuclear pions Phys. Rev. C71 (2005) Shifting pion mass f N (y)

24. Toy Model (Edin and Ingelman) (Neglecting transverse quark momenta) In our case d h m h => R*H N (R) is const. But the x=k + /H N (R(ρ)) depends on nucleon density where

25. Finite Nucleon Volumes - Conclusions A. Constant nucleon mass requires increasing enthalpy STIFFER EOS Shift in Bjorken X B. Constant nucleon volume gives the constant enthalpy with decreasing nucleon mass, lower compressibility SOFTER EOS A&B. In both cases the same width of parton distribution because R*H N (R) const. Valparaiso QNP2015

26. The toy model for phase transition Valparaiso QNP2015

27. PRC 74 our model Valparaiso QNP2015