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In-medium Properties of B and D Mesons

H. Sundu1,a, K. Azizi2,b, and N. Er3,c

1Department of Physics, Kocaeli University, 41380 Izmit, Turkey

2Department of Physics, Do ˘gu¸s University, Acıbadem-Kadıköy, 34722 ˙Istanbul, Turkey 3Department of Physics, Abant Izzet Baysal University, Gölköy Kampüsü, 14980 Bolu, Turkey

Abstract. The shifts in the masses and decay constants of B and D mesons in nuclear medium are calculated in the frame work of QCD sum rules. The results obtained are compared with the existing theoretical predictions.

1 Introduction

To better analyze the results of heavy ion collision experiments and understand the internal structures of the dense astrophysical objects like neutron stars, we need the study of the in-medium properties of hadrons. Moreover, it can be useful for understanding the non-perturbative dynamics as well as the vacuum structure of QCD. In the literature, both the experimental and theoretical studies on the properties of hadrons in-medium have received considerable attention [1–8]. In the present work, we calculate the shifts in the masses and decay constants ofB and D mesons in nuclear medium in the

framework of QCD sum rules.

2 QCD sum rules for modifications of the masses and decay constants of

the D and B mesons in nuclear medium

In this section, we obtain QCD sum rules for the shifts in the masses and decay constants ofD and B

mesons in nuclear matter. We start with the following two-point correlation function: Π(q) = i  d4xeiq·xT [J B[D](x)JB[D](0)]ρN = Π0(q) + ΠN(q)  Π0(q) + ρN 2MNTN (q), (1) whereΠ0(q) and ΠN(q) are vacuum and the static one-nucleon parts in Fermi gas approximation for the nuclear matter, respectively. Here,T is the time ordering operator, ρNis the density of the nuclear matter, MN is the mass of the nucleon and JB[D](x) denotes the interpolating current of the B[D] meson. In order to calculate the shifts in the values of the masses and decay constants, we consider the following forward scattering amplitudeTN(q)

TN(q0 = ω, q) = i  d4xeiq·xN(p)|T [JB[D](x)JB[D]† (0)]|N(p), (2) ae-mail: hayriye.sundu@kocaeli.edu.tr be-mail: kazizi@dogus.edu.tr ce-mail: nuray@ibu.edu.tr C

Owned by the authors, published by EDP Sciences, 2014

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whereqμ = (ω, q) is the four-momentum of the meson and |N(p) represents the isospin and spin

averaged static nucleon state. The interpolating current of the pseudoscalarB[D]-meson can be written

in terms of the quark fields as

JB[D](x) = ¯

u(x)iγ5b[c](x) + ¯b[¯c](x)iγ5u(x)

2 . (3)

whereu(x), b(x) and c(x) are quark fields.

Following the general philosophy of the QCD sum rule method, the aforementioned correlation function can be calculated both in terms of the hadronic parameters called the physical or phenomeno-logical side, and in terms of the QCD parameters called the theoretical or QCD side. These two representations are matched using dispersion relations to obtain QCD sum rules for the shifts in the masses and leptonic decay constants of theB and D mesons. Finally we apply Borel transformation

to suppress the contribution of the higher states and continuum.

In the physical side, the forward scattering amplitudeTN(ω, q) is calculated in the limit q → 0, around ω = mB[D]. Near the pole position of the pseudoscalar meson, theTN(ω, 0) is related to the T-matrix for the forward B[D]− N scattering amplitude and can be written as the following dispersion integrals [11]: TN(ω, 0)=  +∞ −∞ du ρ(u, q = 0) u − ω − iε =  0 du 2ρ(u, q = 0) u2− ω2 , (4)

where ω2 positive real number and ρ(u, q = 0) is the spin-averaged spectral density. After some

straightforward calculations (see also [12]), the physical side of correlation function is obtained : ΠPHYS(ω, 0) f 2 B[D]m4B[D] m2 b[c](m2B[D]− ω2) + ρN 2MN  a (m2 B[D]− ω2)2 + b m2 B[D]− ω2   2MNf 2 B[D]m4B[D]+ ρNm2b[c]b 2MNm2b[c]  m2 B[D]− ρNm2b[c] 2MNfB[D]2 m4B[D]a  − ω2 (5)

where fB[D] is the leptonic decay constant of the B[D]−meson, a and b are the phenomenological parameters.

Using the modified mass in nuclear matter,mB[D]= mB[D]+δmB[D]=

m2

B[D]+ Δm2B[D], we obtain the shifts in the mass and leptonic decay constant ofB[D] meson as:

δmB[D] = 2πMN + mB[D] MNmB[D] ρNaB[D], δ fB[D] = m2 b[c] 2fB[D]m4B[D]  ρN 2MNb − 4f2 B[D]m3B[D] m2 b[c] δmB[D]  , (6)

where the parameteraB[D]is theB[D] − N scattering length [11]. In order to calculate the shifts in the mass and decay constant, we need to calculate the phenomenological parametersa and b using the

forward scattering amplitude calculated both in hadronic and QCD sides. In the low energy limit ω→ 0, the THAD

N (ω, 0) is equivalent to the Born termTNBorn(ω, 0). Hence, we can write the forward scattering amplitude in hadronic side as:

TNHAD(ω, 0)= TNBorn(ω, 0)+ a (m2 B[D]− ω2)2 + b m2 B[D]− ω2 + c s2 0− ω2 , (7)

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with the condition a m4 B[D] + b m2 B[D] + c s0 = 0. (8)

The Born term can be determined by the Born diagrams at the tree level [9, 11]. To calculate it, we consider the contributions of the baryonsΛb[c]andΣb[c]in the medium produced by the interaction of B[D] with the nucleon, i.e.

B−(bu) + p(uud) or n(udd) → Λ0b(udb) or Σb(ddb),

D0(cu) + p(uud) or n(udd) → Λ+

c, Σ+c(udc) or Σ0c(ddc) (9)

We obtain the Born termTBorn

N (ω, 0) as [9]: TBorn(ω, 0)= 2MN(MN+ MB)m 4 B[D]fB[D]2 [ω2− (M N+ MB)2](ω2− mB[D]2 )2(mu+ mb[c])2 g2 NB[D]B(ω2). (10)

whereB denotes the Λb[c]orΣb[c]baryon and gNB[D]B(ω2) is the strong coupling constant among the

B[D] meson, nucleon and B baryon.

The final form of the hadronic side of the current-nucleon forward scattering amplitude is obtained after double Borel transformation as (see also [9, 12])

BTPHYS N = a  1 M2e −m2 B[D]/M2− s0 m4 B[D] e−s0/M2+ be−m2B[D]/M2− s0 m2 B[D] e−s0/M2 + 2f 2 B[D]m4B[D]MN(MN+ MB) [(MN+ MB)2− m2B[D]](mu+ mb[c])2 g2 NB[D]B × − e−(MN+MB) 2/M2 (MN+ MB)2− m2B[D] + 1 (MN+ MB)2− m2B[D] − 1 M2  e−m2B[D]/M 2 . (11)

In the QCD side, we obtain the forward scattering amplitude by inserting the explicit form of the interpolating currentJB[D]into Eq. (2) as:

TNOPE = i 4  d4xeiq.x N(p) TrSQ(−x)γ5Su(x)γ5+ Su(−x)γ5SQ(x)γ5 N(p) , (12) whereSu is light quark andSQ withQ = b or c is the heavy quark propagator. The next step is to use the expressions of the quark propagators and perform the trace and integrals. After lengthy calculations, we get the QCD side of theTNfunction in the rest frame of the nuclear matter in Borel

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scheme as: BTQCD N = 1 3 e−m2Q/M2 M4  − mQ  − 2m2 Q+ M2+ 2p20  ¯qgsσGqN −4mQ  m2Q− 2M2+ 4p20  ¯qD0D0qN +4M2− m2 Q+ M2+ 4p20  qiD 0qN +2M2  2m2Qmu− 3mQM2+ mu  M2− 2p20  ¯qqN  + 1 12π2g 2 sG2N  0 dαe m2 Q/(4α−M2)mQ  4α− M24  16α2mQ+ 3mu  +M2− m2 Qmu+ 3mQM2+ 3muM2  −4αm3Q− m2Qmu+ 4mQM2+ 6muM2  θ  1 −4α + M2  −mQe−m 2 Q/M2 M2 ¯qgsσGqN. (13)

whereM is the Borel mass parameter.

Finally, we equate the Borel transformed physical and QCD sides of the BTN function to find QCD sum rules for the parametersa and b. Since the functions a and b are very lengthy functions, we

do not present their explicit expression here.

3 Numerical results

The sum rules for the parametersa and b contain two auxiliary parameters: the Borel parameter M2

and the continuum thresholds0. Since these are not physical parameters, the results of the parameters

a and b should be practically independent of them. Therefore, we shall find their working regions such

that these parameters weakly depend on these auxiliary parameters. Our numerical analysis show that in the intervals 25GeV2 ≤ M2 ≤ 40 GeV2 and 4GeV2 ≤ M2 ≤ 8 GeV2respectively in theB and

D channels, the dependence of the shifts in the physical quantities are weak. Also, we see that in

the intervals 34GeV2 ≤ s

0 ≤ 38 GeV2and 5.6GeV2 ≤ s0 ≤ 6.4 GeV2 respectively for theB and

D mesons, the results demonstrate weak dependence on the continuum threshold. To see how the

results depend on the Borel mass parameter, we plot the dependence of the shift of the decay constant of theB[D]−meson under consideration versus M2 for different values of the continuum threshold

in figure 1. Making use of the working regions for auxiliary parameters and taking into account all systematic uncertainties, we obtain the numerical results of the shifts in mass and decay constant for

B[D]−meson as presented in table 1. We also compare our results on the mass shifts with the existing

theoretical predictions. Our result on the mass shift inD channel is in a good consistency with the

result of [9]. On the other hand, we see that our result in this channel is the same in magnitude with the prediction of [10], but with opposite sign. As far as the shift in the mass ofB channel is considered,

our result is different in both sign and magnitude with the only existing prediction [10]. Our results on the leptonic decay constant shifts inB and D channels can be checked in future experiments.

In summary, we calculated the shifts in the masses and decay constants of the pseudoscalarB and D mesons in nuclear matter via the QCD sum rules. Our results obtained in the present work can help

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s034 GeV2 s036 GeV2 s038 GeV2 26 28 30 32 34 36 38 40 0.10 0.08 0.06 0.04 0.02 0.00 M2GeV2 ΔfB GeV  s05.6 GeV2 s06.0 GeV2 s06.4 GeV2 4 5 6 7 8 0.010 0.008 0.006 0.004 0.002 0.000 M2GeV2 ΔfD GeV 

Figure 1. The shift of B meson’s decay constant in nuclear matter versus Borel mass M2at three different values of continuum threshold (left panel). The same, but for shift in decay constant of theD meson (right panel).

Table 1. Average values of the shifts in the masses and decay constants of the B and D mesons.

δmB(GeV) δmD(GeV) δ fB(GeV) δ fD(GeV) Present Work −0.242 ± 0.062 −0.046 ± 0.007 −0.023 ± 0.007 −0.002 ± 0.001

[9] − −0.048 ± 0.008 − −

[10] ∼ 0.060 ∼ 0.045 − −

better understand the perturbative and non-perturbative natures of QCD. The results obtained for the shifts in masses especially for those in the decay constants can also be used in theoretical calculations of the electromagnetic properties of the considered mesons as well as their strong couplings with other hadrons in nuclear medium.

Acknowledgment

This work has been supported in part by the Scientific and Technological Research Council of Turkey (TUBITAK) under the research project 114F018.

References

[1] Elisa Fioravanti, AIP Conf.Proc. 1432, 1-434 (2012); arXiv:1206.2214.

[2] B. Friman et al, “The CBM physics book: Compressed Baryonic Matter in Laboratory Experi-ments”, Springer Heidelberg.

[3] http://www.gsi.de/fair/experiments/CBM/index e.html. [4] http://www-panda.gsi.de/auto/phy/ home.htm.

[5] E. G. Drukarev and E. M. Levin, Pis’ma Zh. Eksp. Teor. Fiz. 48, 307 (1988).

[6] E. G. Drukarev and E. M. Levin, Nucl. Phys. A 511, 679, (1990); 516, 715(E) (1990). [7] T. Hatsuda, H. Hogaasen, M. Prakash, Phys. Rev. Lett. 66, 2851 (1991).

[8] C. Adami, G. E. Brown, Z. Phys. A 340, 93 (1991). [9] A. Hayashigaki, Phys. Lett. B 487, 96 (2000).

[10] T. Hilger, R. Thomas, B. Kämpfer, Phys. Rev. C 79, 025202 (2009). [11] Y. Koike and A. Hayashigaki, Prog. Theo. Phys. 98, 631 (1997). [12] K. Azizi, N. Er, H. Sundu, arXiv:1405.3058[hep-ph].

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Şekil

Table 1. Average values of the shifts in the masses and decay constants of the B and D mesons.

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