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odification of nucleon spectral unction in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka kyo Institute of Technology Keisuke Ohtani

Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

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Page 1: Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

Modification of nucleon spectral function in the nuclear medium from QCD sum rules

Collaborators: Philipp Gubler(ECT*), Makoto Oka

Tokyo Institute of Technology   Keisuke Ohtani

Page 2: Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

Outline

•Nucleon QCD sum rule in vacuum

•Summary

•QCD sum rules

•Nucleon QCD sum rule in nuclear matter

•Introduction

Page 3: Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

Introduction

・ Hadron properties in the nuclear medium

N

N

N

N

N N

N

N

NN

N

Probe hadron

Nuclear matter

The properties of the hadron are modified in the medium.

Partial restoration of the chiral symmetry

Interaction with the nucleons in the nuclear matter

We focus on the nucleon ground state and its negative parity excited state.

Page 4: Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

IntroductionMass spectrum of the nucleons

p, n

N(1440)

N(1535)

N(1650)

Positive parity Negative parity

Page 5: Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

IntroductionMass spectrum of the nucleons

p, n

N(1440)

N(1535)

N(1650)

Positive parity

• It is predicted that Chiral symmetry breaking cause these difference.

Negative parity

• The mass difference between nucleon ground state and N(1535) is about 600 MeV.

Page 6: Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

IntroductionMass spectrum of the nucleons

p, n

N(1440)

N(1535)

N(1650)

Positive parity

• It is predicted that Chiral symmetry breaking cause these difference.

Negative parity

• The mass difference between nucleon ground state and N(1535) is about 600 MeV.

To investigate these properties from QCD, non perturbative method is needed.

When chiral symmetry is restored, the mass spectrum will change.

Analysis of QCD sum rule in nuclear matter

• The mass difference between nucleon ground state and N(1535) is about 600 MeV.

?In the nuclear matter

Page 7: Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

is calculated by the operator product expansion (OPE)

Non perturbative contributions are expressed by some Condensates.

QCD sum rulesHadronic spectral function

, ・・・

An order parameter of chiral symmetry

Application of the analyses in the nuclear matter.

Page 8: Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

QCD sum rulesVacuum Nuclear matter

N

N

N

N

N N

N

N

NN

N

Probe hadron

In nuclear matterIn vacuum

Probe hadron: Ground state of nuclear matter

Page 9: Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

Nuclear matter

N

N

N

N

N N

N

N

NN

N

In nuclear matterIn vacuum

Probe hadron

Modification:

Chiral condensate :

New condensate:

Probe hadron

: Ground state of nuclear matter

QCD sum rulesVacuum

Page 10: Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

QCD sum rules

τ 、 s: parameterOPE side

Gaussian sum rule

Vacuum Nuclear matter

is calculated by OPETransformation

We extract the information on the spectral function with maximum entropy method (MEM).

Page 11: Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

contains the term

Nucleon QCD sum rule in vacuumThe behavior of the OPE data in the vacuum

The difference between positive parity and negative parity is mainly caused by chiral condensate term.

Positive parity OPENegative parity OPE

term

Parity: + Parity: -

Mass spectrum of the nucleons

Page 12: Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

930MeV

Positive parity Negative parity

1550 MeV

In both positive and negative parity, the peaks are found.In the negative parity state, the peak correspond to the N(1535) or (and) N(1650).

Nucleon QCD sum rule in vacuum

Page 13: Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

The behavior of the OPE data in the nuclear matter

Vacuum Nuclear matter

N

N

N

N

N N

N

N

NN

N

Probe nucleon

In nuclear matterIn vacuum

Probe hadron

: Ground state of nuclear matter

Nucleon QCD sum rule in nuclear matter

Page 14: Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

Positive parity OPE Negative parity OPE

term

term

ρN: nuclear matter density

The behavior of the OPE data in the nuclear matter

Vacuum Nuclear matter

Parity: + Parity: -

Mass spectrum of the nucleonsVacuum

Nucleon QCD sum rule in nuclear matter

Page 15: Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

contain the terms

Positive parity: OPE data decreases.

Negative parity: OPE data slightly increases.

ρ = 0.25ρNPositive parity OPE Negative parity OPE

term

term

ρN: nuclear matter density

The behavior of the OPE data in the nuclear matter

Parity: + Parity: -

?Mass spectrum of the nucleons

contains the term

Nucleon QCD sum rule in nuclear matter

Page 16: Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

Positive parity OPE Negative parity OPE

term

term

ρN: nuclear matter density

The behavior of the OPE data in the nuclear matter

Parity: + Parity: -

?Mass spectrum of the nucleonsρ = 0.5ρN

contain the terms

contains the term

Positive parity: OPE data decreases.

Negative parity: OPE data slightly increases.

Nucleon QCD sum rule in nuclear matter

Page 17: Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

Positive parity OPE Negative parity OPE

term

term

ρN: nuclear matter density

The behavior of the OPE data in the nuclear matter

Parity: + Parity: -

?Mass spectrum of the nucleonsρ = 0.75ρN

contain the terms

contains the term

Positive parity: OPE data decreases.

Negative parity: OPE data slightly increases.

Nucleon QCD sum rule in nuclear matter

Page 18: Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

Positive parity OPE Negative parity OPE

term

term

ρN: nuclear matter density

The behavior of the OPE data in the nuclear matter

Parity: + Parity: -

?Mass spectrum of the nucleonsρ = 1.0ρN

contain the terms

contains the term

Positive parity: OPE data decreases.

Negative parity: OPE data slightly increases.

Nucleon QCD sum rule in nuclear matter

Page 19: Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

Positive parity OPE dataNegative parity OPE data

term

term

: n=n0

: ρ=0.75ρ0

: ρ=0.5ρ0

: ρ=0.25ρ0

: Vacuum

Positive parity Negative parity

ρN : nuclear matter density

Vacuum

Nucleon QCD sum rule in nuclear matter

Page 20: Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

ρ = 0.25ρN Positive parity OPE dataNegative parity OPE data

term

term

: n=n0

: ρ=0.75ρ0

: ρ=0.5ρ0

: ρ=0.25ρN

: Vacuum

ρN : nuclear matter density

Positive parity Negative parity

Nucleon QCD sum rule in nuclear matter

Page 21: Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

ρ = 0.5ρN Positive parity OPE dataNegative parity OPE data

term

term

: n=n0

: ρ=0.75ρ0

: ρ=0.5ρN

: ρ=0.25ρN

: Vacuum

ρN : nuclear matter density

Positive parity Negative parity

Nucleon QCD sum rule in nuclear matter

Page 22: Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

ρ = 0.75ρN Positive parity OPE dataNegative parity OPE data

term

term

: n=n0

: ρ=0.75ρN

: ρ=0.5ρN

: ρ=0.25ρN

: VacuumPositive parity Negative parity

ρN : nuclear matter density

: ρ=1.0ρ0

Positive parity Negative parity

Nucleon QCD sum rule in nuclear matter

Page 23: Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

ρ = 1.0ρN Positive parity OPE dataNegative parity OPE data

term

term

: n=n0

: ρ=0.75ρN

: ρ=0.5ρN

: ρ=0.25ρN

: VacuumPositive parity Negative parity

ρN : nuclear matter density

: ρ=1.0ρN

Positive parity Negative parity

The values of the energies are obtained.

Nucleon QCD sum rule in nuclear matter

Page 24: Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

Vacuum Nuclear matter

N N

N

N

N

N

N N

N

Probe nucleon

Propagator: Propagator:

N

NN

N

Pole of positive energy state:

Effective mass:

Pole of negative energy state:

Nucleon QCD sum rule in nuclear matter

Page 25: Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

         Investigation of effective masses and vector self energies

210 q

210 q

u

By fitting the phenomenological side and OPE side, we can investigate the self energies.

+ (contribution of negative parity states)

are calculated by OPE are expressed by the propagators in physical energy region

Nucleon QCD sum rule in nuclear matter

Page 26: Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

ρN: nuclear matter density

Nucleon QCD sum rule in nuclear matter

Vacuum ρ=0.25 ρN ρ=0.5 ρN ρ=0.75 ρN ρ=1.0 ρN

810

120

151040

660

270

1460

80

490

430

1430

110

290

640

1410

130

1550

930

0

0

Page 27: Modification of nucleon spectral function in the nuclear medium from QCD sum rules Collaborators: Philipp Gubler(ECT*), Makoto Oka Tokyo Institute of Technology

•We analyze the nucleon spectral function by using QCD sum rules with MEM

Summary

• The information of not only the ground state but also the negative parity excited state is extracted

• We find that the difference between the positive and negative parity spectral function is mainly caused by the chiral condensate.

•We apply this method to the analyses in nuclear medium and investigate the effective masses and the vector self-energies.

•As the density increases, the effective masses decrease and the vector self-energies increase.