Transition form factors and angular distributions of the b1520 NKdecay supported by baryon spectroscopy Yu-Shuai Li12Su-Ping Jin3yJing Gao3zand Xiang Liu1245x

2025-05-06 0 0 2.79MB 23 页 10玖币
侵权投诉
Transition form factors and angular distributions of the ΛbΛ(1520)(N¯
K)`+`decay
supported by baryon spectroscopy
Yu-Shuai Li1,2,Su-Ping Jin3,Jing Gao3,and Xiang Liu1,2,4,5§
1School of Physical Science and Technology, Lanzhou University, Lanzhou 730000, China
2Research Center for Hadron and CSR Physics, Lanzhou University and Institute of Modern Physics of CAS, Lanzhou 730000, China
3School of Physics, Nankai University, Tianjin 300071, China
4Lanzhou Center for Theoretical Physics, Key Laboratory of Theoretical Physics of Gansu Province,
and Frontiers Science Center for Rare Isotopes, Lanzhou University, Lanzhou 730000, China
5Key Laboratory of Quantum Theory and Applications of MoE, Lanzhou University, Lanzhou 730000, China
We calculate the weak transition form factors of the ΛbΛ(1520) transition, and further calculate the
angular distributions of the rare decays ΛbΛ(1520)(N¯
K)`+`(N¯
K={pK,n¯
K0}) with unpolarized Λb
and massive leptons. The form factors are calculated by the three-body light-front quark model with the support
of numerical wave functions of Λband Λ(1520) from solving the semirelativistic potential model associated
with the Gaussian expansion method. By fitting the mass spectrum of the observed single bottom and charmed
baryons, the parameters of the potential model are fixed, so this strategy can avoid the uncertainties arising from
the choice of a simple harmonic oscillator wave function of the baryons. With more data accumulated in the
LHCb experiment, our result can help for exploring the ΛbΛ(1520)`+`decay and deepen our understanding
on the bs`+`processes.
I. INTRODUCTION
The flavor-changing neutral-current (FCNC) processes, in-
cluding the high-profile bs`+`process, can play a cru-
cial role in indirect searches for physics beyond the Stan-
dard Model (SM). These transitions are forbidden at the tree
level and can only operate through loop diagrams in the SM,
and are therefore highly sensitive to potential new physics
(NP) eects, such as the much-discussed RD()=B(B
D()τντ)/B(BD()e(µ)νe(µ)) [14]. These processes thus
provided a unique platform to deepen our understanding of
both quantum chromodynamics (QCD) and the dynamics of
weak processes, and to help hunt for NP signs. Therefore,
the rare decays of bshave attracted the attention of both
theorists and experimentalists [511].
For example, the rare decay ΛbΛ`+`has been the-
oretically studied by various approaches, including lattice
QCD (LQCD) [12,13], QCD sum rules [14], light-cone
sum rule [1519], covariant quark model [20], nonrelativistic
quark model [21,22], and the Bethe-Salpeter approach [23],
etc., and was first measured by the CDF Collaboration [7]
and later by the LHCb Collaboration [8,9]. In addition to
the dierential branching ratio, such abundant phenomenolo-
gies of various angular distributions have also been studied.
Compared with the measured data, the angular distribution of
ΛbΛ`+`was studied in Refs. [24,25] with unpolarized
Λbbaryon, and with polarized Λbbaryon in Ref. [26]. Fur-
thermore, the authors studied the bsµ+µWilson coe-
cients in Ref. [27] using the measured full angular distribution
of the rare decay ΛbΛ(pπ)µ+µby the LHCb Collabo-
ration [9].
Electronic address: liysh20@lzu.edu.cn
Electronic address: jinsuping@nankai.edu.cn
Electronic address: 9820210055@nankai.edu.cn
§Electronic address: xiangliu@lzu.edu.cn
With the previous experiences on the decay to the ground
state Λ, it is therefore worth to further testing the bs`+`
transition in the baryon sector decaying to the excited hy-
peron with quantum number being JP=3/2. The form
factors of the weak transition were calculated by the quark
model [21,22], LQCD [28,29], and the heavy quark expan-
sion [30]. The angular analysis was performed in Ref. [31]
and Ref. [32] for massless and massive leptons, respectively.
The authors of Ref. [33] studied the kinematic endpoint rela-
tions for ΛbΛ(1520)`+`decays and provided the corre-
sponding angular distributions. Amhis et al. [34] used the dis-
persive techniques to provide a model-independent parameter-
ization of the form factors of ΛbΛ(1520) and further inves-
tigated the FCNC decay ΛbΛ(1520)`+`with the LQCD
data. In addition, Xing et al. also studied the multibody decay
ΛbΛ
J(pK)J(`+`) [35]. In addition, Amhis et
al. studied the angular distributions of ΛbΛ(1520)`+`
and talked about the potential to identify NP eects [36]. Ob-
viously, the ΛbΛ(1520) is less studied. Following this
line, we further study the ΛbΛ(1520)(N¯
K)`+`with
the N¯
K={pK,n¯
K0}process and investigate the correspond-
ing angular observables.
From a theoretical point of view, apart from the consider-
ation of new operators beyond the SM, the calculation of the
weak transition form factors is a key issue. In addition, how to
solve the three-body system for the Λbbaryon and Λhyperon
involved is also a challenge. In previous work on baryon weak
decays [3741], the quark-diquark scheme has been widely
adopted as an approximate treatment. Meanwhile, the spa-
tial wave functions of hadrons are often approximated as sim-
ple harmonic oscillator (SHO) wave functions [3743], which
makes the results dependent on the relevant parameters. To
avoid the correlative uncertainties of the above approxima-
tions, in this work we calculate the ΛbΛform factors
by the three-body light-front quark model. Moreover, in the
realistic calculation, we take the numerical spatial wave func-
tions as input, where the semirelativistic potential model com-
bined with the Gaussian expansion method (GEM) [4447] is
arXiv:2210.04640v4 [hep-ph] 1 May 2023
2
adopted. By fitting the mass spectrum of the observed single
bottom and charmed baryons, the parameters of the semirela-
tivistic potential model can be fixed. Compared with the SHO
wave function approximation, our strategy can avoid the un-
certainties arising from the selection of the spatial wave func-
tions of the baryons.
The structure of this paper is as follows. After the Intro-
duction, we derive the helicity amplitudes of ΛbΛ(
N¯
K)`+`(N¯
K={pK,n¯
K0}) processes and define some an-
gular observables with unpolarized Λbbaryons and massive
leptons in Sec. II. The formulas for the weak transition form
factors are derived in the three-body light-front quark model in
Sec. III. And then, to obtain the spatial wave functions of the
involved baryons, the applied semirelativistic potential model
and GEM are briefly introduced in Sec. IV. In Sec. V, we
present our numerical results, including both the relevant form
factors and the physical observables in ΛbΛ(N¯
K)`+`
decays. Finally, this paper ends with a short summary in
Sec. VI.
II. THE ANGULAR DISTRIBUTION OF
ΛbΛ(N¯
K)`+`
In this paper, we use a model-independent approach with
the eective Hamiltonian[48,49]
He(bs`+`)=4GF
2VtbV
ts
10
X
i=1Ci(µ)Oi(µ) (2.1)
to study the bs`+`process, where GF=1.16637 ×
105GeV2is the Fermi coupling constant and |VtbV
ts|=
0.04088 [12] is the product of the Cabibbo-Kobayashi-
Maskawa matrix elements. Furthermore, the Wilson coe-
cients Ci(µ) describe the short-distance physics, while the four
fermion operators Oi(µ) describe the long-distance physics,
where O1,2are the current-current operators, O36are the
QCD penguin operators, O7,8denote the electromagnetic and
chromomagnetic penguin operators respectively, and O9,10
stand for the semileptonic operators.
In our calculation, we follow the treatment given in Refs. [6,
23], adding the factorable quark-loop contributions from O16
and O8to the eective Wilson coecients Ce
7and Ce
9. The
eective Hamiltonian can be written as
He(bs`+`)=4GF
2VtbV
ts
αe
4π(¯s"Ce
9(µ, q2)γµPL
2mb
q2Ce
7(µ)iσµνqνPR#b(¯
µ`)
+C10(µ)( ¯sγµPLb)( ¯
µγ5`)),
(2.2)
where PR(L)=(1 ±γ5)/2 and σµν =i[γµ, γν]/2. The elec-
tromagnetic coupling constant is αe=1/137. For the lead-
ing logarithmic approximation, we take mb=4.80 GeV [50,
51] and the Wilson coecients as Ce
7(mb)=0.313 and
C10(mb)=4.669 in the calculation [5053]. In addition,
the short-distance contributions from the soft-gluon emission
and the one-loop contributions of the four-quark operators O1-
O6, and the long-distance eects due to the charmonium reso-
nances, Jand ψ(2S) are taken into account, where we adopt
the Ce
9(µ, q2) as [50,54,55]
Ce
9(µ, q2)=C9(µ)+Ypert( ˆs)+Yres(q2).(2.3)
The Ypert term can be written as
Ypert( ˆs)=g( ˆmc,ˆs)C(µ)
1
2g(1,ˆs)(4C3(µ)+4C4(µ)+3C5(µ)+C6(µ))
1
2g(0,ˆs)(C3(µ)+3C4(µ))
+2
9(3C3(µ)+C4(µ)+3C5(µ)+C6(µ)),
(2.4)
where ˆmc=mc/mb, ˆs=q2/m2
b,C(µ)=3C1(µ)+C2(µ)+
3C3(µ)+C4(µ)+3C5(µ)+C6(µ), and [50]
g(z,ˆs)=8
9ln z+8
27 +4
9x2
9(2 +x)p|1x|
×(ln |1+1x
11x| − iπfor x4z2/ˆs<1
2 arctan 1
x1for x4z2/ˆs>1,
g(0,ˆs)=8
27 8
9ln mb
µ4
9ln ˆs+4
9iπ.
(2.5)
The Wilson coecients are used as C1(mb)=0.248,
C2(mb)=1.107, C3(mb)=0.011, C4(mb)=0.026,
C5(mb)=0.007, and C6(mb)=0.031 [50]. Besides,
mc=1.4 GeV [50]. The Yres term can be parametrized by
using the Breit-Wigner ansatz (it is a model-dependent treat-
ment, and one can refer to Refs. [56,57] for more detailed
discussions) as [51]
Yres(q2)=3π
α2
e
C(0) X
Vi=J/ψ,ψ(2S)
κVi
Γ(Vi`+`)mVi
m2
Viq2imViΓVi
,(2.6)
where C(0) =0.362, κJ=1, and κψ(2S)=2. The masses
and total widths associated with the relevant charmonium res-
onances are taken to be 3.096 GeV and 92.9 keV for J, and
3.686 GeV and 294 keV for ψ(2S) [58]. The decay widths are
taken as Γ(J`+`)=5.53 keV and Γ(ψ(2S)`+`)=
2.33 keV [58].
Since the quarks are confined in hadron, the weak transi-
tion matrix element cannot be calculated in the framework of
perturbative QCD. They are conventionally parametrized in
terms of eight (axial-)vector and six (pseudo-)tensor type di-
mensionless form factors [21,25,31,32,5961]. In this work,
we adopt the helicity-based form as [31,32]
3
hΛ(k,sΛ)|¯sγµb|Λb(p,sΛb)i=¯uα(k,sΛ)(pα"fV
t(q2)(mΛbmΛ)qµ
q2
+fV
0(q2)mΛb+mΛ
s+ pµ+kµ(m2
Λbm2
Λ)qµ
q2!
+fV
(q2) γµ2mΛ
s+
pµ2mΛb
s+
kµ!#
+fV
g(q2)"gαµ +mΛ
pα
s γµ2kµ
mΛ
+2(mΛpµ+mΛbkµ)
s+!#)u(p,sΛb),
(2.7)
hΛ(k,sΛ)|¯sγµγ5b|Λb(p,sΛb)i=¯uα(k,sΛ)γ5(pα"fA
t(q2)(mΛb+mΛ)qµ
q2
+fA
0(q2)mΛbmΛ
s pµ+kµ(m2
Λbm2
Λ)qµ
q2!
+fA
(q2) γµ+2mΛ
s
pµ2mΛb
s
kµ!#
+fA
g(q2)"gαµ mΛ
pα
s+ γµ+2kµ
mΛ2(mΛpµmΛbkµ)
s!#)u(p,sΛb),
(2.8)
hΛ(k,sΛ)|¯siσµνqνb|Λb(p,sΛb)i=¯uα(k,sΛ)(pα"fT
0(q2)q2
s+ pµ+kµ(m2
Λbm2
Λ)qµ
q2!
+fT
(q2)(mΛb+mΛ) γµ2mΛ
s+
pµ2mΛb
s+
kµ!#
+fT
g(q2)"gαµ +mΛ
pα
s γµ2kµ
mΛ
+2(mΛpµ+mΛbkµ)
s+!#)u(p,sΛb),
(2.9)
hΛ(k,sΛ)|¯siσµνqνγ5b|Λb(p,sΛb)i=¯uα(k,sΛ)γ5(pα"fT5
0(q2)q2
s pµ+kµ(m2
Λbm2
Λ)qµ
q2!
+fT5
(q2)(mΛbmΛ) γµ+2mΛ
s
pµ2mΛb
s
kµ!#
+fT5
g(q2)"gαµ mΛ
pα
s+ γµ+2kµ
mΛ2(mΛpµmΛbkµ)
s!#)u(p,sΛb).
(2.10)
This form defined above is convenient for calculating the corresponding helicity amplitudes, where q2is the transferred momen-
tum square and s±=(mΛb±mΛ)2q2.
A. The helicity amplitudes of the ΛbΛ`+`decay
To calculate the ΛbΛ`+`process, we define the corresponding helicity amplitudes of the Λb(sΛb)Λ(sΛ) transition
as
H(V,A,T,T5)(sΛb,sΛ, λW)=
µ(λW)hΛ(sΛ)|¯sγµ, γµγ5,iσµνqν,iσµνqνγ5b|Λb(sΛb)i,(2.11)
where µ(λW=t,±,0) are the polarization vectors of the virtual gauge boson in the Λbrest frame, sΛband sΛare the polarizations
of Λband Λ, respectively. For the vector current, the complete helicity amplitudes HV(sΛb,sΛ, λW) read [31]
HV(sΛb,sΛ,t)=
µ(t)hΛ(k,sΛ)|¯sγµb|Λb(p,sΛb)i
=fV
t(q2)mΛbmΛ
pq2¯uα(k,sΛ)pαu(p,sΛb),(2.12)
4
HV(sΛb,sΛ,0) =
µ(0)hΛ(k,sΛ)|¯sγµb|Λb(p,sΛb)i
=2fV
0(q2)mΛb+mΛ
s+
k·(0)¯uα(k,sΛ)pαu(p,sΛb),(2.13)
HV(sΛb,sΛ,±)=
µ(±)hΛ(k,sΛ)|¯sγµb|Λb(p,sΛb)i
=fV
(q2)+fV
g(q2)mΛ
s¯uα(k,sΛ)pα/
(±)u(p,sΛb)
+fV
g(q2)¯uα(k,sΛ)α(±)u(p,sΛb).(2.14)
Analogous expressions for the helicity amplitudes of the axial-vector, tensor, and pseudotensor currents are written as
HA(sΛb,sΛ,t)=
µ(t)hΛ(k,sΛ)|¯sγµγ5b|Λb(p,sΛb)i
=fA
t(q2)mΛb+mΛ
pq2¯uα(k,sΛ)pαγ5u(p,sΛb),(2.15)
HA(sΛb,sΛ,0) =
µ(0)hΛ(k,sΛ)|¯sγµγ5b|Λb(p,sΛb)i
=2fA
0(q2)mΛbmΛ
s
k·(0)¯uα(k,sΛ)pαγ5u(p,sΛb),(2.16)
HA(sΛb,sΛ,±)=
µ(±)hΛ(k,sΛ)|¯sγµγ5b|Λb(p,sΛb)i
=fA
(q2)fA
g(q2)mΛ
s+¯uα(k,sΛ)pα/
(±)γ5u(p,sΛb)
fA
g(q2)¯uα(k,sΛ)α(±)γ5u(p,sΛb),(2.17)
HT(sΛb,sΛ,0) =
µ(0)hΛ(k,sΛ)|¯siσµνqνb|Λb(p,sΛb)i
=2fT
0(q2)q2
s+
k·ε(0)¯uα(k,sΛ)pαu(p,sΛb),(2.18)
HT(sΛb,sΛ,±)=
µ(±)hΛ(k,sΛ)|¯siσµνqνb|Λb(p,sΛb)i
=fT
(q2)(mΛb+mΛ)+fT
g(q2)mΛ
s¯uα(k,sΛ)pα/
(±)u(p,sΛb)
fT
g(q2)¯uα(k,sΛ)α(±)u(p,sΛb),(2.19)
HT5(sΛb,sΛ,0) =
µ(0)hΛ(k,sΛ)|¯siσµνqνγ5b|Λb(p,sΛb)i
=2fT5
0(q2)q2
s
k·(0)¯uα(k,sΛ)pαγ5u(p,sΛb),(2.20)
HT5(sΛb,sΛ,±)=
µ(±)hΛ(k,sΛ)|¯siσµνqνγ5b|Λb(p,sΛb)i
=fT5
(q2)(mΛbmΛ)fT5
g(q2)mΛ
s+¯uα(k,sΛ)pα/
(±)γ5u(p,sΛb)
fT5
g(q2)¯uα(k,sΛ)α(±)γ5u(p,sΛb),(2.21)
respectively. Using the kinematic conventions presented in Appendix B 1, the nonzero terms for the above helicity amplitudes
of the vector, axial-vector, tensor, and pseudotensor currents are [31]
HV(+1/2,+1/2,t)=HV(1/2,1/2,t)=fV
t(q2)mΛbmΛ
pq2
s+s
6mΛ
,
HV(+1/2,+1/2,0) =HV(1/2,1/2,0) =fV
0(q2)mΛb+mΛ
pq2
ss+
6mΛ
,
HV(+1/2,1/2,+)=HV(1/2,+1/2,)=fV
(q2)ss+
3mΛ
,
HV(1/2,3/2,+)=HV(+1/2,+3/2,)=fV
g(q2)s+,
(2.22)
5
HA(+1/2,+1/2,t)=HA(1/2,1/2,t)=fA
t(q2)mΛb+mΛ
pq2
ss+
6mΛ
,
HA(+1/2,+1/2,0) =HA(1/2,1/2,0) =fA
0(q2)mΛbmΛ
pq2
s+s
6mΛ
,
HA(+1/2,1/2,+)=HA(1/2,+1/2,)=fA
(q2)s+s
3mΛ
,
HA(1/2,3/2,+)=HA(+1/2,+3/2,)=fA
g(q2)s,
(2.23)
HT(+1/2,+1/2,0) =HT(1/2,1/2,0) =fT
0(q2)qq2ss+
6mΛ
,
HT(+1/2,1/2,+)=HT(1/2,+1/2,)=fT
(q2)(mΛb+mΛ)ss+
3mΛ
,
HT(1/2,3/2,+)=HT(+1/2,+3/2,)=fT
g(q2)s+,
(2.24)
HT5(+1/2,+1/2,0) =HT5(1/2,1/2,0) =fT5
0(q2)qq2s+s
6mΛ
,
HT5(+1/2,1/2,+)=HT5(1/2,+1/2,)=fT5
(q2)(mΛbmΛ)s+s
3mΛ
,
HT5(1/2,3/2,+)=HT5(+1/2,+3/2,)=fT5
g(q2)s,
(2.25)
respectively.
Similarly, we define the leptonic helicity amplitudes as
L(V,A)(s`,s`+, λW)=¯µ(λW)h``+|¯
`γµ, γµγ5`+|0i
=¯µ(λW)¯u(p`,s`)γµ, γµγ5v(p`,s`+),(2.26)
where ¯µ(λW=t,±,0) are the polarization vectors of the virtual gauge boson in the dilepton rest frame. Using the kinematic
conventions presented in Appendix B 2, the nonzero terms are obtained as [32]
LV(±1/2,±1/2,0) =±2m`cos θ`,LV(±1/2,1/2,0) =qq2sin θ`,
LV(+1/2,+1/2,±)=2m`sin θ`,LV(1/2,1/2,)=2m`sin θ`,
LV(±1/2,1/2,±)=pq2
2(1 +cos θ`),LV(±1/2,1/2,)=pq2
2(1 cos θ`),
LA(±1/2,±1/2,t)=2m`,LA(±1/2,1/2,0) =sin θ`qq2β`,
LA(±1/2,1/2,±)=pq2
2(1 +cos θ`)β`,LA(±1/2,1/2,)=pq2
2(1 cos θ`)β`,
(2.27)
where β`q14m2
`/q2.
B. The helicity amplitudes of the ΛN¯
K decay
We use the eective Lagrangian approach to describe the strong decay process ΛN¯
K. The concerned eective Lagrangian
is
LΛKN =gΛKN ¯
Nγ5Λ
ααK,(2.28)
where gΛKN is the coupling constant. So the decay amplitude for the ΛN¯
Kprocess can be expressed as
MΛN¯
K(sΛ,sN)=gΛKN ¯uN(sN)γ5uΛ(sΛ)kα
2,(2.29)
摘要:

Transitionformfactorsandangulardistributionsoftheb!(1520)(!NK)`+`decaysupportedbybaryonspectroscopyYu-ShuaiLi1;2,Su-PingJin3,yJingGao3,zandXiangLiu1;2;4;5x1SchoolofPhysicalScienceandTechnology,LanzhouUniversity,Lanzhou730000,China2ResearchCenterforHadronandCSRPhysics,LanzhouUniversityandInstitut...

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Transition form factors and angular distributions of the b1520 NKdecay supported by baryon spectroscopy Yu-Shuai Li12Su-Ping Jin3yJing Gao3zand Xiang Liu1245x.pdf

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