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Scalar D mesons in nuclear matter Taesoo Song, Woosung Park, Kie Sang Jeong and Su Houng Lee (Yonsei Univ.)

Scalar D mesons in nuclear matter

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Scalar D mesons in nuclear matter. Taesoo Song, Woosung Park, Kie Sang Jeong and Su Houng Lee (Yonsei Univ.). Procedure. Motivation 2. QCD sum rule in vacuum & in nuclear matter 3. Application to Scalar D mesons 4. Conclusions. 1. Motivation. - PowerPoint PPT Presentation

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Page 1: Scalar D mesons in nuclear matter

Scalar D mesons in nuclear matter

Taesoo Song, Woosung Park,

Kie Sang Jeong and Su Houng Lee

(Yonsei Univ.)

Page 2: Scalar D mesons in nuclear matter

Procedure

1. Motivation

2. QCD sum rule in vacuum & in nuclear matter

3. Application to Scalar D mesons

4. Conclusions

Page 3: Scalar D mesons in nuclear matter

1. Motivation

• Charm-strange scalar meson Ds0+(2317) was

discovered in 2003• Its mass is too lower than the expected values in

quark models and other theoretical predictions.• It has been interpreted as the isosinglet state

(conventional scalar meson), a four-quark state, a mixed state of both, a DK molecule, …

• Later charm scalar meson D0*(2400) with broad width was discovered in 2004

• Its mass is similar to or larger than that of D+

s0(2317), even though Ds(0-) is 100 MeV higher than D(0-).

Page 4: Scalar D mesons in nuclear matter

2. QCD sum rule

1. OPE (operator product expansion)

2. Phenomenological side

3. Dispersion relation

4. Borel transformation

Page 5: Scalar D mesons in nuclear matter

2. 1. OPE (operator product expansion)

effect) range (long

ndimension ith operator wr Nonsingula :

effect) range(short t Coefficien Wilson :

)0(

)(

)0()()0()(lim0

n

n

nnn

x

O

xC

OxCBxA

Page 6: Scalar D mesons in nuclear matter

As an example,

sduq

xccqxqxcxSc

qxSxqxSxSTrxedi

qcxcxqTxedi

jxjTxedi

q

ccqxiq

xiq

xiq

,,

:)()0()0()(::)()()0(

:)0()()(::)()(:

)0()0(),()(

)0(),(

)3()2()1()0(

4

4

4

where,

:

iscurrent scalar charm offunction on polarizati The

may be ignored

Page 7: Scalar D mesons in nuclear matter

Perturbative quark propagator in a weak gluonic background field(The gluons are supposed to emerge from the ground state)

Page 8: Scalar D mesons in nuclear matter

:)()( xSxSTr cq : ~ gConsiderin (0)

Perturbative part I : dimension 0

Gluon condensates<G2> : dimension 4

and more condensateswith higher dimensionor more strong couplings

Page 9: Scalar D mesons in nuclear matter

:)(......:!

)(

)...(...!

1)(

)...(...)2(!

)(

0)(

11

011

011

qqSDDqn

i

DDxxn

x

FDDxxnn

xxA

xAx

cn

nn

n

nxn

n

nxn

n

and

GaugeSchwinger Fock in

(1)

Page 10: Scalar D mesons in nuclear matter

y graphicall is )1(

Quark condensate <qq> : dimension 3

Quark-gluon mixed condensates<qGq> : dimension 5

and more condensateswith higher dimensionor more strong couplings

Page 11: Scalar D mesons in nuclear matter

OPE up to dimension 5 in vacuum

, where C0 (q2) is perturbative part

Page 12: Scalar D mesons in nuclear matter

OPE up to dimension 5 in nuclear matter

where

at meson scalar gconsiderin and

, matter, theof framerest in the

),()()(

),0,(

)0,1(

200

200

0

qqqq

qq

v

oe

Page 13: Scalar D mesons in nuclear matter

List of employed condensate parameters

Page 14: Scalar D mesons in nuclear matter

2.2. Phenomenological side

.

, function step of definition theand

, operatorson translatiusing and

,

operatorscurrent obetween twoperator identity Inserting

iqEE

jo

iqEE

joq

iw

edw

ix

joexjo

dpI

oxjjoxojxjoxxedi

ojxjToxediq

qq

q

qq

q

iwx

pxip

p

ppp

xiq

xiq

0

2

0

2

0

3

3

004

42

2

|)0(|

2

|)0(|)(

2

1)(

|)0(||)(|

||2)2(

|)()0(|)(|)0()(|)(

|)]0(),([|)(

0

Page 15: Scalar D mesons in nuclear matter

Ansatz' ContinuumPole' called so is which

!!function spectral

, If

2

1

, usingby extracted ispart imaginary Its

,

)(Im)(

)(||Im

||||

)(||2

)(||22

1Im

)(1

0222

220

2

22

220

2022

0

20

222

sqmqF

Eqjo

jojo

EqjoE

qEqjo

E

q

xix

P

ix

h

qq

qq

qqq

qqq

Page 16: Scalar D mesons in nuclear matter

2.3. Dispersion relation(in vacuum)

L.H.S .is a function of QCD parameters such as g, mq, <qq>, <G2>…, obtained from OPE.

R.H.S. is a function of physical parameters such as mλ and s0

Page 17: Scalar D mesons in nuclear matter

Dispersion relation (in nuclear matter)

Page 18: Scalar D mesons in nuclear matter

2.4. Borel transformation

dsesdsQs

sB

MNQB

qQdQ

dQ

nB

C

Ms

C

NN

n

n

MnQnQ

2

22

2

/2

22

222

2

/

)(Im)(Imˆ

1

)!1(

11ˆ

)()!1(

1limˆ

part continuum gsuppressinby side ogicalphenomenol theimproves 2)

termscondensate ldimensiona-high gsuppressinby side OPE improves 1)

where, ation transformBorel

Page 19: Scalar D mesons in nuclear matter

3. Application to scalar D mesons

1. Charm scalar meson D0* in vacuum

2. Charm scalar meson D0* in nuclear matter

3. Charm-strange scalar meson Ds0 in vacuum & in nuclear matter

Page 20: Scalar D mesons in nuclear matter

3.1. Charm scalar meson D0* in vacuum

From the dispersion relation

,

the mass of scalar D meson is

22

22

/~

2/~

2~

/1/~

~Mm

Mm

eF

MeFm

Page 21: Scalar D mesons in nuclear matter

Borel windowThe range of M2 satisfying below two conditions

1) continuum/total < 0.3

/ < 0.3

2) Power correction/total < 0.3

/ <0.3

Page 22: Scalar D mesons in nuclear matter

Borel curve for D0*(2400) in vacuum

(adjust s0 to obtain flattest curve within Borel window)

S0=7.7 GeV2

Page 23: Scalar D mesons in nuclear matter

3.2. Charm scalar meson D0* in nuclear matter

• Two dispersion relations for πe and πo exist

• ≡f(s0+,s0

-)

• ≡g(s0+,s0

-)

Page 24: Scalar D mesons in nuclear matter

density, saturationnuclear times0.1 of case in the example,For

method. iterativeby solved are they and

,

is,That

functions, twoofion recombinatproper After

),,(

),,(

.),(),(

),()/1(

),()/1(

),(),(

),()/1(

),()/1(

00

00

0000

0020022

0000

0020022

ssmmm

ssmmm

ssgmssf

ssgMdd

mssfMdd

m

ssgmssf

ssgMdd

mssfMdd

m

iteration No. D+ s0 D+ mass D- s0   D- mass

0     7.7 2.392

1 7.55 2.373    2     7.8 2.391

3 7.5 2.371    4     7.8 2.391

Page 25: Scalar D mesons in nuclear matter

Mass shift of D0*±(2400) in nuclear matter

(The conditions for Borel window are continuum/total<0.5 & power correction/total <0.5)

Page 26: Scalar D mesons in nuclear matter

Physical interpretation of the result

matter.nuclear in ofthat

than more decreases of mass thereason why theisThat

. than attractive more is result, a As

quarks. and in rich ismatter Nuclear

. is of that and , is ofcomponent quark The

*0

*0

*0

*0

*0

*0

D

D

DdcDcd

du

dcDcdD

Page 27: Scalar D mesons in nuclear matter

3.3. Charm-strange scalar meson Ds0 in vacuum & in nuclear matter

ns.calculatio lattice from and

GeV

GeV

belows. as changed are parameters Condensate

.simplicityfor ignored isquark strange of mass The

2

36.0

8

1

8

1

8

1

018.0

0

8.0

8.0

20

20

20

20

20

20

00

y

FdgdyFsgsFdgd

dDdysDsdDd

dFgDdysFgDsdFgDd

nsiDsdiDd

ssdd

ssFsgsFdgd

ddyddssddmattervacuum

Page 28: Scalar D mesons in nuclear matter

Borel curves for Ds0 (2317) in vacuum

(The conditions for Borel window are continuum/total<0.5 & power correction/total <0.5)

Page 29: Scalar D mesons in nuclear matter

Mass shift of Ds0±(2317) in nuclear

matter (The conditions for Borel window are

continuum/total<0.5 & power correction/total <0.5)

Nuclear density (0.17 nucleon/fm3) Nuclear density (0.17 nucleon/fm3)

Page 30: Scalar D mesons in nuclear matter

4. Conclusion1. We successfully reproduced the mass of charm scalar

meson D0* in vacuum and that of charm-strange scalar meson Ds0 by using QCD sum rule

2. Based on this success, their mass shifts in the nuclear matter are estimated by considering the change of condensate parameters and adding new condensate parameters which do not exist in vacuum state.

3. The mass of D0*+ decreases in the nuclear matter more than that of D0*-, as naively expected.

4. But the mass of Ds0+ increases a little in the nuclear matter,

while that of Ds0- decreases.

5. The quark component of these scalar particles are still in question, whether they are conventional mesons or quark-quark states or their combinations or others.

6. We expect that the behavior of their masses in nuclear matter serves to determine the exact quark component of those scalar particles.

Page 31: Scalar D mesons in nuclear matter

4.1. Future work

• QCD sum rule for pseudoscalar D meson, which is the chiral partner of charm scalar meson – the mass difference between scalar and pseudoscalar meson is expected to decrease in nuclear matter due to the partial restoration of chiral symmetry.

• QCD sum rule for charm scalar meson as four quark state – The comparison of its mass shift in nuclear matter with that of conventional meson will reveal the exact component of charm scalar meson.