Survey of Issues Misak Sargsian Florida International University.

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Survey of Issues Misak Sargsian Florida International University

Transcript of Survey of Issues Misak Sargsian Florida International University.

Page 1: Survey of Issues Misak Sargsian Florida International University.

Survey of IssuesMisak Sargsian

Florida International University

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Structure of the NucleonStructure of the Nucleon

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Nuclear MatterNuclear Matter

Electromagnetic Interaction

Strong Interaction

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Quark Degrees of Freedom

Neutron Stars

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Pandharipande, Heiselberg, 2000

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Microscopic Structure of NN Interactionand properties of Dense Nuclear Matter

Degenerate neutron and electron Fermi Gas

Oppenheimer-Volkoff model, 1939

Observational

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Microscopic Structure of NN , NNN, ... Interactions

NN interaction

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In the Lab

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How to get nucleons close together

Probing at large relative momenta

In the Lab

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Day,Frankfurt, MS, Strikman, PRC 1993

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Egiyan, et al PRC 2004

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Egiyan, et al PRL 2006

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What we Learned from A(e,e’)X Reactions

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neutron

proton

6p and 6n

rate

calculate the expected proton rate

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92% of the time two-nucleon high density fluctuations

are ptoron and neutron

4% of the time proton-proton or neutron-neutron

Piasetzky, Sargsian, Strikman, Frankfurt, WatsonPRL 2006

Important Implication for the structure of the neutron stars

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3N Intercation

Relativistic Effects

Effectively Repulsive ?

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In the Lab

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Chemical Potential and Quantum Field

Classical Thermodynamics for Open Systems

Added energy due to Ni matter introduced to the system

Diffusive Equilibrium

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Particles in the Cold Dense Matter

Everything may change when kinetic energy

of NN system exceeds 300 MeV

The system becomes effectively open

Particles which leave the star do not contribute in

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Kaon Condensation

Interaction is attractivekaon energy decreases with density

Strangeness Enhancement

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In the Lab

The role of in High Density Fluctuations

Role of the Strangeness in High Density Fluctuations

Hyperon N interaction

Chiral Restoration

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Chiral Restoration and Hidden Color

In the world where chiral symmetry is broken

Deuteron (t=0,s=1) two nucleons two-separately color neutral objects

In the world where chiral symmetry is unbroken

Signature of Chiral Simmetry Restoration

with an increase of internal momenum in the deuteron

Survey Experiments

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with an increase of internal momenum in the deuteron

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Quark Matter

Estimates done within Bag Model

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In the Lab

Probing superfast quarks

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Hard Disintegration

N

N

d

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Modification of quark distributions

in nucllei (EMC effect)

α,pt

d

e

e’

x,

Q2

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