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The phi meson in nuclear matter                 - recent result from theory - The phi meson in nuclear matter                 - recent result from theory -

The phi meson in nuclear matter - recent result from theory - - PowerPoint Presentation

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The phi meson in nuclear matter - recent result from theory - - PPT Presentation

Talk at ECT Workshop New perspectives on Photons and Dileptons in Ultrarelativistic HeavyIon Collisions at RHIC and LHC 4 December 2015 P Gubler and K Ohtani Phys Rev D ID: 788602

nuclear matter rules sum matter nuclear sum rules results meson phys qcd spectral experiment function consistent mass density dim

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Slide1

The phi meson in nuclear matter - recent result from theory -

Talk at ECT* Workshop “New perspectives on Photons and Dileptons in Ultrarelativistic Heavy-Ion Collisions at RHIC and LHC” 4. December, 2015

P. Gubler and K. Ohtani, Phys. Rev. D 90, 094002 (2014). P. Gubler and W. Weise, Phys. Lett. B 751, 396 (2015).

Collaborators:

Keisuke

Ohtani

(

Tokyo Tech

)

Wolfram Weise (ECT*, TUM)

Slide2

Introduction

φ mesonmφ = 1019 MeV

Γφ = 4.3 MeVObject of study:

Interest:

Slide3

Previous developmentsThe E325 Experiment (KEK)

Slowly moving

φ mesons are produced in 12 GeV p+A reactions and are measured through di-leptons.

p

e

e

p

e

e

f

f

outside decay

inside decay

No effect

(

only vacuum)

Di-lepton spectrum reflects the modified

φ

-meson

Slide4

4

bg

<1.25 (Slow)

1.25<

bg

<1.75

1.75<

bg

(Fast)

Large Nucleus

Small Nucleus

Fitting Results

Slide5

Experimental Conclusions

Pole mass:

Pole width:

35 MeV negative mass shift at normal nuclear matter density

Increased width to 15 MeV at normal nuclear matter density

R. Muto et al, Phys. Rev. Lett.

98

, 042501 (2007).

Slide6

QCD sum rules

In this method the properties of the two point correlation function

is fully exploited:

is calculated

“perturbatively”,

using OPE

spectral function

of the operator

χ

After the

Borel

transformation:

M.A.

Shifman

, A.I.

Vainshtein

and V.I.

Zakharov

,

Nucl

. Phys. B147, 385 (1979); B147, 448 (1979).

q

2

Slide7

perturbative Wilson coefficients

non-perturbative condensates

More on the OPE in matter

Change in hot or dense matter!

Slide8

Structure of QCD sum rules for the phi meson

Dim. 0:

Dim. 2:

Dim. 4:

Dim. 6:

In Vacuum

Slide9

In Nuclear Matter

Structure of QCD sum rules for the phi meson

Dim. 0:

Dim. 2:

Dim. 4:

Dim. 6:

Slide10

The strangeness content of the nucleon: results from lattice QCD

Taken from M. Gong et al. (

χQCD Collaboration), arXiv:1304.1194 [hep-ph].

y ~ 0.04

Still large systematic uncertainties?

Slide11

Results of test-analysis (using MEM)

P. Gubler and K.

Ohtani, Phys. Rev. D 90, 094002 (2014). Peak position can be extracted, but not the width!

Slide12

Results for the φ

meson mass

P. Gubler and K. Ohtani, Phys. Rev. D 90, 094002 (2014).

Most important parameter, that

determines the behavior of the

φ

meson mass at finite density:

Strangeness content of the nucleon

Slide13

Compare Theory with Experiment

Experiment

Sum Rules + Experiment

Lattice QCD

Not consistent?

Slide14

However…

slope = σsN

Slide15

Experiment

Sum Rules + Experiment

Lattice QCD

Therefore…

?

Slide16

However…

Slide17

Experiment

Sum Rules + Experiment

Lattice QCD

Therefore…

??

Slide18

Issues of Borel sum rules

Details of the spectral function cannot be studied (e.g. width)Higher order OPE terms are always present (e.g. four-quark condensates at dimension 6)Use a model to compute the complete spectral function

Use moments to probe specific condensates

Slide19

Method

Vector meson dominance model:

Kaon

-loops introduce self-energy corrections to the

φ

-meson propagator

Slide20

Starting point:

Rewrite using hadronic degrees of freedom

Kaon

loops

Slide21

Vacuum spectrum

Data fromJ.P. Lees et al. (BABAR Collaboration), Phys. Rev. D

88, 032013 (2013).

(Vacuum)

How

is this spectrum modified in nuclear matter?

Is the (modified) spectral function consistent with QCD sum rules?

Slide22

What happens in nuclear matter?

Forward KN (or KN) scattering amplitude

If working at linear order in density, the free scattering amplitudes can be used

Slide23

More on the free KN and KN scattering amplitudes

For KN: Approximate by a real constant (↔ repulsion) T. Waas, N. Kaiser and W. Weise, Phys. Lett. B

379, 34 (1996). For KN: Use the latest fit based on SU(3) chiral effective field theory, coupled channels and recent experimental results (

↔ attraction)

Y. Ikeda, T.

Hyodo

and W. Weise,

Nucl

. Phys. A

881

, 98 (2012).

K

-

p scattering length obtained from

kaonic

hydrogen (SIDDHARTA Collaboration)

Slide24

Results (Spectral Density)

Takes into account further KN-interactions with intermediate hyperons, such as:

Asymmetric modification of the spectrum.

Not necessarily

parametrizable

by a simple

Breit

-Wigner peak!

Important message for future E16 experiment at J-PARC

Slide25

Moment analysis of obtained spectral functions

Starting point: Borel-type QCD sum rules

Large M limitFinite-energy sum rules

Slide26

Consistency check

(Vacuum) Are the zeroth and first momentum sum rules consistent with our phenomenological spectral density?Zeroth MomentFirst Moment

Consistent!

Slide27

Consistency check

(Nuclear matter) Are the zeroth and first momentum sum rules consistent with our phenomenological spectral density?Zeroth MomentFirst Moment

Consistent!

Slide28

Dependence on continuum onset?

Ansatz used so far:However, experiments give us a different picture:

Slide29

New trial: ramp function

Mimics the experimental behavior of the 2K + n

π

states

Will this new

ansatz

significantly change the behavior of our results?

Slide30

New trial: ramp function

→ modified sum rules

Slide31

Results of ramp-function analysis

(Vacuum) → Consistent, if W’ is not too small

Slide32

Results of ramp-function analysis

(Nuclear matter) → Also consistent, if W’ is not too small

Slide33

Ratios of moments

Vacuum: Nuclear Matter: (S-Wave) (S- and P-Wave)

Interesting to measure in actual experiments?

Slide34

Second moment sum rule

Factorization hypothesis Strongly violated?

Slide35

Summary and Conclusions

The φ-meson mass shift in nuclear matter constrains the strangeness content of the nucleon:increasing φ-meson mass in nuclear matter??The E325 experiment at KEK measured a negative mass shift of -35 MeV at normal nuclear matter density

a σsN-value of > 100 MeV??Most lattice calculations give a small σsN

-value

decreasing

φ

-meson mass in nuclear matter??

One recent lattice calculates obtains a large

σ

sN

-value (

σ

sN

= 105 MeV)

Slide36

Summary and Conclusions

We have computed the φ meson spectral density in vacuum and nuclear matter based on an effective vector dominance model and the latest experimental constraints Accurate description of the spectral function in vacuumNon-symmetric behavior of peak in nuclear matter

We have carried out a moment analysis of the obtained spectral functionsSpectral functions are consistent with lowest two momentum sum rules

Moments provide direct links between QCD condensates and experimentally measurable quantities

Slide37

Outlook

Further improve the sum rule computationComplete OPE up to operators of mass dimension 6Accurate evaluation of four-quark condensates (on the lattice?)

Consider finite momentumUse both QCD sum rules and effective theory

Make predictions for the E16 experiment at J-PARC

Slide38

Backup slides

Slide39

In-nucleus decay fractions for E325 kinematics

Taken from: R.S. Hayano and T. Hatsuda, Rev. Mod. Phys. 82, 2949 (2010).

Slide40

Other experimental results

There are some more experimental results on the φ-meson width in nuclear matter, based on the measurement of the transparency ratio T:

T. Ishikawa et al, Phys. Lett. B

608

, 215 (2005).

Measured at SPring-8 (LEPS)

A.

Polyanskiy

et al, Phys. Lett. B

695

, 74 (2011).

Measured at COSY-ANKE

Slide41

Results of test-analysis (using MEM)

P. Gubler and K. Ohtani, Phys. Rev. D 

90, 094002 (2014).

Slide42

Results of ramp-function analysis

(Nuclear matter) → Also consistent, if W’ is not too small