charm physics dn interactions in nuclear matter

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1 Charm physics DN interactions in nuclear matter Clara Estela Jiménez Tejero National Nuclear Summer School 2007, Tallahassee, Florida Advisors: I. Vidaña, A. Ramos T. Mizutani, A. Ramos, hep- ph/0607257 J.Hofmann and M.F.M.Lutz, Nucl. Phys. A763, 90 (2005)

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Charm physics DN interactions in nuclear matter. Clara Estela Jiménez Tejero. National Nuclear Summer School 2007, Tallahassee, Florida. Advisors: I. Vidaña, A. Ramos. T. Mizutani, A. Ramos, hep-ph/0607257. J.Hofmann and M.F.M.Lutz, Nucl. Phys. A763, 90 (2005). Index. - PowerPoint PPT Presentation

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Page 1: Charm physics DN interactions in nuclear matter

1

Charm physics

DN interactions in nuclear matter

Clara Estela Jiménez Tejero

National Nuclear Summer School 2007, Tallahassee, Florida

Advisors:I. Vidaña, A. Ramos

T. Mizutani, A. Ramos, hep-ph/0607257

J.Hofmann and M.F.M.Lutz, Nucl. Phys. A763, 90 (2005)

Page 2: Charm physics DN interactions in nuclear matter

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Index

I. Discovery of charm

II. Motivation

III. Coupled Channel Approach model for solving DN interactions -Results in free space

IV. Conclusion and future perspectives

V. Panda experiment at GSI (if I have time)

Page 3: Charm physics DN interactions in nuclear matter

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Charmonium discovery

October, 1974Simultaneous discovery:

• Ting et al. at BNL AGS• Richter et al. at SLAC SPEAR

p + Be→ e+e- + X at AGS

e+e- annihilation

1976 Nobel prize in physics

Very narrow peaks -> very long lifetimes (10-20s): thousand of times longer than expected!

In both experiments a

peak was found at 3.1 GeV

New kind of property forth type of quark!

Page 4: Charm physics DN interactions in nuclear matter

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Example of decay’ → J/ + + + - Followed by J/ → e+e-

Decay of J/psi lowest level in lighter particles -> 90% decay to lighter quark particles (pions, kaons)-> Rarely decays to an electron and a positron (or muon and antimuon)

photonspions

electronsmuons

Page 5: Charm physics DN interactions in nuclear matter

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Techniques in 80´s made possible to see charm particles directly by their trails, but how?

You just need to collide, for example, a photon with a proton …

PHOTON PROTON

Creation of charmed particles

Charm quarks combine with lighter quarks (u, d, s) to form either barions or mesons

PHOTON

xavi
Page 6: Charm physics DN interactions in nuclear matter

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Production of charmed particles in the bubble chamber (SLAC) in 1980

2 mm

Page 7: Charm physics DN interactions in nuclear matter

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Can be produced in pairs (D+,D-)

• in heavy ion experiments:

• or antiproton anhilation experiments (PANDA at FAIR) on protons and nuclei:

… production of charm particles at

present

Page 8: Charm physics DN interactions in nuclear matter

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Motivation Why is important to understand the interaction of charmed mesons in a hadronic medium?

If the mass of the D (and Dbar) mesons gets reduced appreciably in the medium (cold or hot), this would provide a conventional hadronic physics explanation to explain J/ supression (attributed to be a signal for the formation of a Quark-Gluon Plasma)

Hints that a D Dbar meson-pair could feel attraction: an open charm enhancement has been observed in nucleus-nucleus collisions by the NA50 Collaboration

D and Dbar in the medium

Page 9: Charm physics DN interactions in nuclear matter

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KN and DN are “similar” systems:Apparent similarity in their coupled channel nature by their association with the Lambda resonances: Presence of the c(2593) (udc)

(plays a similar role as the (1405) (uds) in KN dynamics)

D and Dbar mesons:

Similar to Kbar K:

Why do we believe in the “couple channel approach” model that we use?

Other methods like QCDSR and NMFA become innapropiate when the 2-body interaction:Strongdominated by intermediate bound states or resonances and/orstrongly coupled to other channels

Page 10: Charm physics DN interactions in nuclear matter

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D mesons in symmetric nuclear matter:DN couple-channel equations approach

• First step: (1)-> Solving Bethe-Salpeter

equation in free space

• Second step: (2)-> Solving Bethe-

Salpeter equation in nuclear medium.

-> T is the transition operator matrix.-> The propagator G, diagonal matrix in which every element is the product of single-particle propagator for a meson and a barion.-> The potential V, whose elements are Weinberg-Tomozawa type meson-baryon interactions.

(1)

(2)

xavi
Page 11: Charm physics DN interactions in nuclear matter

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In-medium effects

Pauli blocking on intermediate nucleons: consequence of Pauli principle, prevents the scattering to intermediate nucleon states below Fermi momentum, pf.

Dressing of mesons and baryons: Non perturbative strong interaction at low energies -> particles of intermediate loops interact through strong force with the nucleons of the Fermi sea, and their properties are modified with respect to those in free space.

In medium effects are contained in the propagator

D

Medium: isosymmetric nuclear matter (nucleons, Np=Nn)

Page 12: Charm physics DN interactions in nuclear matter

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njnmkmkikmjmkmkikkjkikijij

njnmjmkmkikkjkikijij

mjmkmkjkikijij

kjkikijij

TGVGVGVVGVGVVGVVT

TGVVGVGVVGVVT

TGVVGVVT

TGVVT

ln

ln )(

)(

Self-consistent coupled channels method: Bethe-Salpeter equation

T = ( I - V·G )-1 ·VT = V+V·GT

V?

G?

Page 13: Charm physics DN interactions in nuclear matter

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)3245(´),3085(),3071(),2960(

),2835(),2810(),2589(:)0,0,1(´

cscc

cc

DKK

DNSIC

)3415(´),3160(),3071(),3005(

),2960(),2810(),2589(),2425(:)0,1,1(´

cscc

ccc

DK

KDNSIC

The sectors of our interest:In S-wave and JP=(1/2)-, two different

channels

First channel with seven states:

Second channel with eight states:

Page 14: Charm physics DN interactions in nuclear matter

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q1 q2

p1 p2

V Light vector meson exchange

Page 15: Charm physics DN interactions in nuclear matter

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Pseudoscalar meson fields

vector meson fields

barion fields

Page 16: Charm physics DN interactions in nuclear matter

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t-channel exchange of vector mesons:

universal vector coupling constant

chiral symmetry in the light sector imposed

W.T interaction

-> With these approximations and projecting in s-wave:

Page 17: Charm physics DN interactions in nuclear matter

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I=0 I=1

Coefficients C=0, S=0

Li · Lj = [kinetic term]·Ci,j

Page 18: Charm physics DN interactions in nuclear matter

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… solving T matrix in the free space …

Page 19: Charm physics DN interactions in nuclear matter

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))()((

1

)(

1

)(

1

)2()(

22200

004

4

imkQkQ

ikEkikEkE

MkdisG

i

iii

ii

all 4-momenta are given in the lab frame

Ei and Mi is the energy and mass of the baryon mi the mass of the meson

Propagator in free space

q1=(q10,q1)q2=(q20,q2)

p1=(p10,p1) p2=(p20,p2)

s = (Q0)2 – (Q)2 Energy of mass frame

Page 20: Charm physics DN interactions in nuclear matter

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Free space DN amplitudes

I=0 I=1

c(2595) c

Page 21: Charm physics DN interactions in nuclear matter

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T matrix in the nuclear matter …

Page 22: Charm physics DN interactions in nuclear matter

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G in nuclear matter

T = V+V·GT

V

GG in free space

Ci,j

T = ( I - V·G )-1 ·V

D N Intermediate states DN

Summary

(Li · Lj = [kinetic term]·Ci,j)

Page 23: Charm physics DN interactions in nuclear matter

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Conclusions …

-> DN interaction in coupled channels from a model (inspired on the work of Hofmann and Lutz)

-> In free space, we generate the c(2595) dynamically in I=0. The same interaction generates a I=1 wide resonance which we denote as c(2770)

… and Future

-> We will implement the medium effects on the DN amplitudes (Pauli blocking, self-consistent dressing of D meson, dressing of ) self-consistently.

Ds also develops a self-energy

-> Solve C=1 S=1 DsN problem in the medium and incorporate Ds self-energy in our coupled-channel problem (DN strongly coupled to DsY)

[M.F.M.Lutz, and C.L.Korpa, Phys. Lett. B 633,43 (2006)]

Page 24: Charm physics DN interactions in nuclear matter

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thanks for your

patience …

… so early

in the

morning

Question time

Page 25: Charm physics DN interactions in nuclear matter

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Panda menu- Charmonium spectrospcopy- Gluonic excitations (hibrids, glueballs)- Open and hidden charm in nuclei- -ray spectroscopy of hypernuclei

http://www-panda.gsi.de/auto/_home.htm

Page 26: Charm physics DN interactions in nuclear matter

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Characteristics HESR 10^11stored antiprotons1.5 -14.5 GeVL= 2 x 1032cm-2s-1δp/p ≥ 10-5σx≥ 50 μm