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Phys. Lett. B 855 (2024) 138802
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Physics Letters B
journal homepage: www.elsevier.com/locate/physletb
Letter
Light-quark mass dependence of the Λ(1405) resonance
Xiu-Lei Ren
Helmholtz Institute Mainz, Staudingerweg 18, Mainz, 55128, Germany
A R T I C L E
I N F O
Editor: A. Schwenk
Keywords:
Kaon-nucleon interaction
Chiral symmetry
Λ(1405)
A B S T R A C T
We present the light-quark mass dependence of the Λ(1405) resonance at leading order in a renormalizable
framework of covariant chiral effective field theory. The meson-baryon scattering amplitudes, which are obtained
by solving the scattering equation within time-ordered perturbation theory, follow the quark mass trajectory of
the Coordinated Lattice Simulations consortium. At 𝑀𝜋 ≈ 200 MeV and 𝑀𝐾 ≈ 487 MeV, our parameter-free
prediction of Λ(1405) poles is consistent with the recent lattice results of BaSc Collaboration [Phys. Rev. Lett.
132, 051901 (2024)]. Varying the pion mass from 135 MeV to 400 MeV, we present the evolution of double-pole
̄ threshold; whereas the lower pole
positions of Λ(1405): the higher pole remains a resonance around the 𝐾𝑁
undergoes a transition from resonance to a virtual state, and ultimately to a bound state of the 𝜋Σ system, which
could be verified by the forthcoming lattice QCD simulations.
1. Introduction
Studying the meson-baryon scattering in the SU(3) sector can deepen
our understanding of nonperturbative QCD. In particular, the attractive interaction between anti-kaon (𝐾̄ ) and nucleon (𝑁 ), which triggers the existence of the Λ(1405) resonance [1], the antikaonic- and
multi-antikaonic nuclei/atoms e.g., in Refs. [2,3], and the possible antikaonic condensation in neutron star [4,5], plays an important role in
the strangeness nuclear physics [6,7].
The Λ(1405) state, which is a 𝐼(𝐽 𝑃 ) = 0(1∕2− ) baryonic resonance
of strangeness 𝑆 = −1, was first predicted by Dalitz and Tuan [8,9]
and then confirmed by hydrogen bubble chamber experiments in the
𝜋Σ spectrum [10]. Λ(1405) does not adhere to the prediction of the
constituent quark model [11], thus categorizing it as an exotic candidate. With the development of chiral perturbation theory (ChPT) [12]
and its unitization technique — chiral unitary approach (CUA) [13],
Oller and Meißner [14] found that the Λ(1405) state could be composed of two dynamically generated 𝐼 = 0 poles, which are located
̄ thresholds. This further arouses tremendous
between the 𝜋Σ and 𝐾𝑁
efforts in experimental and theoretical research to uncover the nature of
the Λ(1405) resonance. The detailed discussion and the references can
be found in the recent reviews [15–17] and the section 83 of Particle
Data Group (PDG) review [1]. Besides, the most up-to-date experimental researches have reported, e.g., the photoproduction cross sections
of 𝐾 + Λ(1405) and Λ(1405) lineshape at the BGOOD experiment [18];
the 𝐾 − 𝑝 → 𝜋 0 Σ0 , 𝜋 0 Λ cross sections near threshold at DAΦNE [19];
the 𝜋Σ invariant mass spectra in 𝐾 − -induced reactions on deuteron
by J-PARC E31 Collaboration [20]; the 𝐾 − 𝑝 femtoscopic correlations
by ALICE Collaboration [21]. On the theoretical side, the most recent
̄ interacstudies can be found e.g., in Ref. [22] to investigate the 𝐾𝑁
tion up to next-to-next-to-leading order of CUA; in Ref. [23] to perform
the uncertainty analysis by including the correlations between the pole
parameters within the next-to-leading order CUA; in Ref. [24] to constrain the chirally motivated models with the 𝜋Σ photoproduction mass
spectra. Note that a consensus has yet to be reached on the one-/twopole structure of Λ(1405). Although the latest PDG review [1] has listed
Λ(1405) as a four-star state and the second pole of Λ(1405) as Λ(1380)
with 2-star rating.
With the rapid progress of computing techniques, lattice QCD simulation is going to be a promising approach to identifying the Λ(1405)
state and clarifying the controversy of the one-/two-pole structure. The
earlier efforts can be found in e.g. Refs. [25–29]. Most recently, Baryon
Scattering (BaSc) Collaboration has performed a first lattice calculation
̄ scattering amplitudes [30,31]. Usof the coupled-channel 𝜋Σ and 𝐾𝑁
ing a single 𝑁𝑓 = 2 + 1 ensemble generated by the Coordinated Lattice
Simulations (CLS) consortium, they found two poles of the Λ(1405) resonance with the pseudoscalar masses 𝑀𝜋 ≈ 200 MeV and 𝑀𝐾 ≈ 487 MeV:
̄ threshold, and the
the higher pole is a resonance just below the 𝐾𝑁
lower pole is a virtual bound state below the 𝜋Σ threshold. Although the
finite-volume correction and the finite-lattice spacing effect are not yet
implemented, the BaSc results provide an ideal playground for checking/verifying the predictive power of existing phenomenological models
and chiral unitary approaches.
E-mail address: xiulei.ren@uni-mainz.de.
https://doi.org/10.1016/j.physletb.2024.138802
Received 5 April 2024; Received in revised form 29 May 2024; Accepted 9 June 2024
Available online 13 June 2024
0370-2693/© 2024 The Author(s).
Published by Elsevier B.V. Funded by SCOAP³.
(http://creativecommons.org/licenses/by/4.0/).
This is an open access article under the CC BY license
Physics Letters B 855 (2024) 138802
X.-L. Ren
That is one purpose of the current work: to examine our renormalizable approach for the meson-baryon scattering, which was proposed
in Ref. [32]. Starting with the covariant chiral effective Lagrangians
and employing the time-ordered perturbation theory (TOPT), we define
an effective potential as the sum of two-particle irreducible contributions of time-ordered diagrams. The corresponding (coupled-channel)
scattering equation 𝑇 = 𝑉 + 𝑉 𝐺𝑇 can be derived self-consistently in
TOPT. At leading order (LO), we take into account the full off-shell
dependence in solving the scattering equation. The renormalized scattering amplitude is obtained by utilizing the subtractive renormalization
scheme [33]. Note that the subtracted terms are fixed by the chiral symmetry, which is different from the often-used strategies in CUA, where
the finite-cutoff or the subtraction constant varies to match the data. In
this sense, our framework at LO provides a model-independent prediction for the meson-baryon scattering.
As shown in Ref. [32], our approach has been successfully applied
to the pion-nucleon system. Then, we extend this framework to the
strangeness 𝑆 = −1 sector with isospin 𝐼 = 0 and study the Λ(1405) resonance at the physical point [34]. We solve the scattering equation with
̄ , 𝜂Λ, and 𝐾Ξ, and obtain the renorthe four coupled channels 𝜋Σ, 𝐾𝑁
malized 𝑇 -matrix in the isospin limit. Two Λ(1405) poles are found on
the second Riemann sheet: the lower pole (1337.7 − 𝑖79.1 MeV) is close
̄
to the 𝜋Σ threshold, the higher pole (1430.9 − 𝑖8.0 MeV) just below 𝐾𝑁
threshold. Our LO results are consistent with the ones of the next-toleading order (NLO) study in CUA [35].
Coming to the unphysical quark mass region, it is interesting to extrapolate our parameter-free prediction of Λ(1405) poles and compare
it with the BaSc lattice data. If such an agreement is reached, it indicates that our approach exhibits the predictive capability to some
extent. Therefore, it enables us to investigate the quark mass dependence of the Λ(1405) state. Similar studies along this line can be found
in Refs. [36–41]. Here we focus on the results along with the quark-mass
trajectory of the CLS ensembles. Our model variables, the pseudoscalar
meson masses, octet baryon masses, vector meson masses, and meson
decay constants, have been calculated in Refs. [42–44] based on the
CLS configuration. It provides a good opportunity to investigate the
light-quark mass dependence of Λ(1405), which could be verified by
the forthcoming results of the BaSc Collaboration. Note that this LO
study can be thought as a first step and the higher order corrections are
planned in the future to refine our conclusion.
This article is organized as follows. In Sect. 2, we briefly present our
renormalizable approach to study the 𝑆 = −1 meson-baryon scattering,
followed by the description of the CLS lattice data. The comparison with
the BaSc results and the quark mass dependence of Λ(1405) poles are
given in Sect. 3. Finally, we summarize our study in Sect. 4.
that we employ the vector-meson exchange (VME) to saturate the oftenused Weinberg-Tomozawa (WT) term since the former has a better
ultraviolet behavior without changing the low-energy physics. For the
strangeness 𝑆 = −1 sector with isospin 𝐼 = 0, the LO interaction for the
process 𝑀𝑖 (𝑞1 ) + 𝐵𝑖 (𝑞2 ) → 𝑀𝑗 (𝑞2 ) + 𝐵𝑗 (𝑝2 ) is given as in TOPT
)
(
𝑀𝑉2
1 ∑ 𝑉
𝐶𝑀 𝐵 ,𝑀 𝐵
𝜔𝑀𝑖 (𝒒 1 ) + 𝜔𝑀𝑗 (𝒒 2 )
2
𝑗
𝑗
𝑖
𝑖
𝜔𝑉 (𝒒 1 − 𝒒 2 )
32𝐹0 𝑉
[
1
×
𝐸 − 𝜔𝐵𝑖 (𝒑1 ) − 𝜔𝑉 (𝒒 1 − 𝒒 2 ) − 𝜔𝑀𝑗 (𝒒 2 )
]
1
+
𝐸 − 𝜔𝐵𝑗 (𝒑2 ) − 𝜔𝑉 (𝒒 1 − 𝒒 2 ) − 𝜔𝑀𝑖 (𝒒 1 )
𝑉LO = −
𝑚𝐵 (𝝈 ⋅ 𝒒 2 )(𝝈 ⋅ 𝒒 1 )
1 ∑ 𝐵
𝐶𝑀 𝐵 ,𝑀 𝐵
2
𝑗
𝑗
𝑖
𝑖
𝜔
4𝐹0 𝐵
𝐵 (𝑷 ) 𝐸 − 𝜔𝐵 (𝑷 )
(𝝈 ⋅ 𝒒 1 )(𝝈 ⋅ 𝒒 2 )
𝑚𝐵
1 ∑ ̃𝐵
,
𝐶𝑀 𝐵 ,𝑀 𝐵
+
2
𝑗
𝑗
𝑖
𝑖
𝜔
(𝑲)
𝐸
−
𝜔
(𝒒
4𝐹0 𝐵
𝐵
𝑀𝑖 1 ) − 𝜔𝑀𝑗 (𝒒 2 ) − 𝜔𝐵 (𝑲)
+
(1)
where 𝐹0 and 𝑀𝑉 are the pseudoscalar decay constant and the vector
meson mass, respectively, in the chiral limit. Both are related via the
Kawarabayashi-Suzuki-Riazuddin-Fayyazuddin relation [47–49]: 𝑀𝑉2 =
2𝑔 2 𝐹02 with the coupling 𝑔 of the vector-field self-interaction. The constant coefficients 𝐶 𝑉 of the VME contribution are given in Table 1 of
Ref. [34], and the coefficients of the Born (𝐶 𝐵 ) and crossed-Born (𝐶̃ 𝐵 )
terms, as the functions of the axial vector couplings 𝐷 and 𝐹 , are given
in Tables 2 and 3 of Ref. [34]. In the center-of-mass (c.m.) frame, the
four momenta of initial and final states are
(
)
(
)
𝑞1𝜇 = 𝜔𝑀𝑖 (𝒑), 𝒑 , 𝑝𝜇1 = 𝜔𝐵𝑖 (𝒑), −𝒑 ,
)
)
(
(
𝑞2𝜇 = 𝜔𝑀𝑗 (𝒑′ ), 𝒑′ , 𝑝𝜇2 = 𝜔𝐵𝑗 (𝒑′ ), −𝒑′ ,
(2)
with the relative momenta 𝒑, 𝒑′ , and the on-shell energy 𝜔𝑋 (𝒑) ≡
√
𝑚2𝑋 + 𝒑2 . Furthermore, 𝐸 is the total energy of the meson-baryon
system, and 𝑃 = 𝑞1 + 𝑝1 = 𝑞2 + 𝑝2 , 𝐾 = 𝑝1 − 𝑞2 = 𝑝2 − 𝑞1 . Note that
the crossed Born term introduces poles when iterated in the scattering
equation. To avoid this technical complication, as done in Refs. [50,51],
we take the total energy 𝐸 in the denominator as the lowest threshold
of the relevant channels. Such approximation does not affect the final
results because the contribution of the crossed Born term is rather small
to the 𝑆 -wave meson-baryon scattering.
After performing the 𝑆 -wave projection of the LO interaction, one
can plug it into the coupled-channel scattering equation in the partial
wave basis,
2. Formalism
(
(
)
) ∑
𝑇 𝑗𝑖 𝐸; 𝑝′ , 𝑝 = 𝑉 𝑗𝑖 𝐸; 𝑝′ , 𝑝 +
𝑑𝑘 𝑘2 𝑗𝑛
𝑉 (𝐸; 𝑝′ , 𝑘)
∫
(2𝜋)3
𝑛
In this section, we first lay out the formalism to study the 𝑆 = −1
meson-baryon scattering in the SU(3) unitarized chiral EFT based on a
renormalizable framework. The details can be found in Ref. [34]. After
that, we investigate the light-quark mass dependence of our model variables by the combination of chiral formulae and lattice QCD data based
on the CLS configurations in order to study the evolution of Λ(1405)
poles. It is worth noting that the three-body effects from 𝜋𝜋Λ states
could be involved in the Λ(1405) region, particularly as we move closer
to the physical point. This complicated estimation is beyond the scope of
this Letter, and thus we do not include it, as is usually done in the literature. Interested readers can refer to e.g. Refs. [45,46] for more details
about the three-body scatterings.
(3)
× 𝐺𝑛 (𝐸) 𝑇 𝑛𝑖 (𝐸; 𝑘, 𝑝),
where 𝑖, 𝑗, 𝑛 denote the initial, final and intermediate particle channels of meson and baryon states. The two-body Green function, which
is obtained according to the diagrammatic rules of TOPT [50], has the
following form
𝐺𝑛 (𝐸) =
𝑚𝐵𝑛
1
.
2 𝜔𝑀𝑛 (𝒌) 𝜔𝐵𝑛 (𝒌) 𝐸 − 𝜔𝑀𝑛 (𝒌) − 𝜔𝐵𝑛 (𝒌) + 𝑖𝜖
(4)
In order to obtain the renormalized scattering 𝑇 -matrix, it is convenient to separate the leading order potential into the one-baryon reducible part and irreducible part,
2.1. Meson-baryon scattering in TOPT
𝑉LO = 𝑉𝑅 + 𝑉𝐼 ,
(5)
where 𝑉𝑅 is the Born term, which can separate into two diagrams by
cutting only the single-baryon line, and 𝑉𝐼 includes the remaining terms,
At LO, the meson-baryon scattering potential contains the vectormeson exchange contribution, the Born and crossed-Born terms. Note
2
Physics Letters B 855 (2024) 138802
X.-L. Ren
which cannot do such separation. Then, one can rewrite the scattering
equation (Eq. (3)), 𝑇 = 𝑉 + 𝑉 𝐺𝑇 , as the three coupled equations:
𝑇 = 𝑇𝐼 + (1 + 𝑇𝐼 𝐺) 𝑇𝑅 (1 + 𝐺 𝑇𝐼 ),
𝑇𝐼 = 𝑉𝐼 + 𝑉𝐼 𝐺 𝑇𝐼 ,
(6)
𝑇𝑅 = 𝑉𝑅 + 𝑉𝑅 𝐺 (1 + 𝑇𝐼 𝐺) 𝑇𝑅 .
It is found that the irreducible part 𝑇𝐼 is finite in the removed regulator limit. To demonstrate this fact, we take the vector-meson-exchange
potential as an example. First, we investigate the UV behavior of the
once-iterated contribution 𝑉 𝐺𝑉 at one-loop level:
𝐼𝑉 𝐺𝑉 =
𝑑3𝑘
𝑉
(𝑝′ , 𝑘) 𝐺(𝑘) 𝑉VME (𝑘, 𝑝).
∫ (2𝜋)3 VME
Fig. 1. Left panel: Linear dependence of 𝑀𝐾2 in terms of 𝑀𝜋2 for the quark mass
trajectory 𝑚 = 𝑚symm . Right panel: The octet-baryon masses as the functions
of the pion mass with the mass trajectory 𝑚 = 𝑚symm . The dots are the lattice
results, the stars stand for the experimental masses, corrected for the isospinbreaking effects.
(7)
When the integral momentum 𝑘 goes to infinity, the one-loop integral
becomes
𝐼𝑉 𝐺𝑉 →
𝑑3𝑘 1 1 1
,
∫ (2𝜋)3 𝑘 𝑘3 𝑘
chiral analysis of the meson and baryon masses from the RQCD Collaboration [42] based on the CLS configuration, which is also utilized by
the BaSc Collaboration.
First, we use a linear function of 𝑀𝜋 and 𝑀𝐾
(8)
which converges. This benefit arises from the VME potential, which has
a milder UV behavior compared to the often-used WT term. One can
easily verify that the infinite iteration of 𝑉VME in the ladder diagram
also converges. Besides, the crossed-Born term presents a similar UV
behavior to the VME counterpart. Because the half-off-shell potential
𝑉CB (𝑘, 𝑝) approaches
𝑉CB (𝑘, 𝑝) →
𝝈 ⋅ 𝒑𝝈 ⋅ 𝒌
,
𝑘2
𝑀𝐾2 = 𝑎 + 𝑏𝑀𝜋2 ,
(15)
as done in Ref. [53], to parameterize the quark mass dependence of
the kaon mass for the quark mass trajectory of 𝑚 = 𝑚symm , keeping the
trace of the bare quark-mass matrix fixed 𝑇 𝑟(𝑀) = const., given by the
CLS ensembles. The lattice pion and kaon masses in Ref. [42] have been
corrected by including the finite-volume effects. The values of the pion
and kaon masses at the physical point are
(9)
when the integral momentum 𝑘 goes to infinity.
Regarding the reducible part, because the iteration of the Born term
is quadratically divergent, thus the only divergent term in the total
𝑇 -matrix originates from the reducible part 𝑇𝑅 . To achieve renormalization, we first rewrite the Born potential in a separable form,
𝑀𝜋,phys = 134.8(3) MeV,
𝑀𝐾,phys = 494.2(3) MeV,
(16)
where 𝜉 𝑇 (𝑝) is defined as 𝜉 𝑇 (𝑝) = (1, 𝑝), and 𝐶(𝐸) denotes a 2 ×2 matrix.
representing the electrically neutral isospin-averaged results [54].
The best fitting result is shown in the left panel of Fig. 1 with
𝑎 = 0.25189 GeV2 and 𝑏 = −0.42143. Then, the quark mass dependence of 𝑀𝜂 is determined via the Gell-Mann-Okubo relation 𝑀𝜂2 =
𝑇𝑅 (𝑝′ , 𝑝; 𝐸) = 𝜉 𝑇 (𝑝′ ) 𝜒(𝐸) 𝜉(𝑝),
As to the lowest-lying octet baryon masses, we employ the mass expressions at next-to-leading order in covariant baryon ChPT
𝑉𝑅 (𝑝′ , 𝑝; 𝐸) = 𝜉 𝑇 (𝑝′ ) 𝐶(𝐸) 𝜉(𝑝),
(10)
(4𝑀𝐾2 − 𝑀𝜋2 )∕3.
Then, the reducible 𝑇𝑅 matrix can be expressed in a separable form
(11)
where 𝜒(𝐸), as given below, is divergent,
[
]−1
𝜒(𝐸) = 𝐶(𝐸)−1 − 𝜉 𝐺(𝐸) 𝜉 𝑇 − 𝜉 𝐺(𝐸) 𝑇𝐼𝑆 𝐺(𝐸) 𝜉 𝑇
.
𝑚𝐵 = 𝑚0 +
(12)
+
Then, one can apply the subtractive renormalization [33] by replacing
the meson-baryon Green function 𝐺(𝐸) with the subtracted one
𝑆
𝐺 (𝐸) = 𝐺(𝐸) − 𝐺(𝑚𝐵 ),
𝑃 =𝜋, 𝐾
𝜉𝑃(2)𝐵 𝑀𝑃2
∑
1
𝜉 (3) 𝐻𝐵
(4𝜋𝐹0 )2 𝑃 =𝜋, 𝐾,𝜂 𝑃 𝐵
(
𝑀𝑃
𝑚0
)
(17)
,
(2)
where 𝑚0 is the baryon mass in the chiral limit. The LO coefficients 𝜉𝑃 𝐵 ,
as the function of low-energy constants (LECs) 𝑏0, 𝐷, 𝐹 , can be found
(13)
(3)
in Table 1 of Ref. [53]. The NLO coefficients 𝜉𝑃 𝐵 , the combination of
the baryon axial coupling constants 𝐷 and 𝐹 , are given in Table 2 of
Ref. [53] with the one-loop function 𝐻𝐵 (𝑥)
to systematically remove the divergences. This corresponds to taking
into account the counter-terms generated by the renormalization of the
baryon masses and the meson-baryon coupling constants. Note that such
subtraction, which is an analogy to the extended-on-mass-shell (EOMS)
scheme [52], corresponds to the expansion around the threshold and
can systematically remove the chiral power-counting breaking terms in
the iterated amplitudes. Finally, we obtain a renormalized 𝑇 -matrix
(
(
)
)
𝑇 = 𝑇𝐼𝑆 + 𝜉 𝑇 + 𝑇𝐼𝑆 𝐺𝑆 𝜉 𝑇 𝜒 𝑆 (𝐸) 𝜉 + 𝜉 𝐺𝑆 𝑇𝐼𝑆 ,
∑
[
𝐻𝐵 (𝑥) = −2𝑥
3
𝑥
log(𝑥) +
2
√
]
( )
𝑥
𝑥2
arccos
,
1−
4
2
(18)
which is obtained in the EOMS scheme [52]. The 𝐹0 is the pseudoscalar
meson decay constant in the chiral limit. To obtain the light-quark mass
dependence of the octet baryon mass, we perform the fit of the RQCD
results [42], where the finite-volume corrections and the discretization
effects are taken into account. Furthermore, we also include the experimental value of octet baryon masses, where the isospin-breaking
effects from QED and QCD are removed [42]. We use the SU(6) relation
𝐹 = 2∕3𝐷 and 𝐷 + 𝐹 = 𝑔𝐴 = 1.267 to fix 𝐷 = 0.760 and 𝐹 = 0.507. For
the meson decay constant, we use the SU(3) averaged value 𝐹0 = 1.17𝐹𝜋
with 𝐹𝜋 = 92.4 MeV to achieve a relatively better description of lattice data. Then, we have four free parameters, and the best-fit results
lead to 𝑚0 = 0.813 GeV, 𝑏0 = −0.669 GeV−1 , 𝑏𝐷 = 0.0254 GeV−1 , and
(14)
where the superscript 𝑆 demonstrates the replacement of 𝐺 as 𝐺𝑆 in
the expressions of 𝑇𝐼 and 𝜒(𝐸).
2.2. Quark mass dependence of our model variables
First, we investigate the quark mass dependence of the pseudoscalar
meson masses 𝑀𝑃 and the octet baryon masses 𝑚𝐵 , which appear in
both of the LO chiral potential and the two-body Green function. Confronting the recent lattice results of Λ(1405) [30,31], we conduct the
3
Physics Letters B 855 (2024) 138802
X.-L. Ren
Table 1
̄ coupled channel calculation
Pole positions of two Λ(1405) poles and the corresponding couplings 𝑔𝑖 from the 𝜋Σ-𝐾𝑁
at 𝑀𝜋 = 203.7 MeV and 𝑀𝐾 = 486.4 MeV. Pole positions from the full four-coupled channel calculation are also given.
For comparison, the BaSc results are listed with one combined uncertainty.
BaSc [30,31]
This work
Λ(1405)
𝑧𝑅 [MeV]
𝑧𝑅 a [MeV]
𝑧𝑅 [MeV]
𝑔𝜋Σ
𝑔𝐾𝑁
̄
|𝑔𝜋Σ |∕|𝑔𝐾𝑁
̄ |
Lower pole
Higher pole
1392(18)
1455(21) − 𝑖11.5(6.0)
1389.05
1464.55 − 𝑖9.44
1387.14
1469.86 − 𝑖4.71
0.021 + 𝑖1.87
0.038 + 𝑖0.98
0.017 + 𝑖1.55
1.51 − 𝑖1.22
1.21
0.50
a
̄ , 𝜂Λ, and 𝐾Ξ.
The full calculation with four coupled channels: 𝜋Σ, 𝐾𝑁
MeV2 and 𝐿𝑟8 = 1.143 × 103 MeV2 . Note that 𝐿𝑟8 is slightly changed, but
𝐿𝑟5 decreases around 1∕3 times in comparison with the value given in Fit
I of Ref. [56]. This observation could call for a high-statistics simulation
of 𝐹𝜋 at small pion masses.
3. Results and discussion
We first present our prediction of the Λ(1405) poles with unphysical
quark masses 𝑀𝜋 ≈ 200 MeV and 𝑀𝐾 ≈ 487 MeV. For comparison with
̄
the lattice result of BaSc Collaboration [30,31], we focus on the 𝜋Σ-𝐾𝑁
coupled channel and use the same hadron masses: 𝑀𝜋 = 203.7 MeV,
𝑀𝐾 = 486.4 MeV, 𝑚𝑁 = 979.8 MeV, and 𝑚Σ = 1193.9 MeV to calculate
the scattering amplitudes. The vector meson masses appearing in the
LO potential are estimated through the chiral expansion Eq. (19) with
𝑀𝜋 = 203.7 MeV. For the decay constant, we take 𝐹0 = 𝐹𝜋 = 93.2 MeV,
as used by the BaSc lattice simulation, instead of the chiral limit value.
The difference would be of the higher order. The axial vector couplings
are fixed as 𝐷 = 0.760 and 𝐹 = 0.507 with 𝐷 + 𝐹 = 𝑔𝐴 = 1.267.
To obtain the meson-baryon scattering amplitudes, we first solve the
integral equation by including the full off-shell dependence of the kernel potential. Such treatment is always employed in the study of the
nucleon-nucleon interaction within the chiral EFT, e.g. Refs. [57,58].
Furthermore, the pole positions of resonances can change in solving the
meson-baryon integral loop with the full off-shell dependence [59–61]
in comparison with the approximation of the on-shell factorization. Secondly, as mentioned above, we employ the subtractive renormalization
to obtain the finite 𝑇 -matrix by taking the cutoff limit Λ → ∞. In practice, a sharp cutoff regulator 𝐹Λ (𝑝′ , 𝑝) = 𝜃(Λ − 𝑝′ ) 𝜃(Λ − 𝑝) is employed
with Λ = 10 GeV, which is sufficiently large to get rid of the finiteartifacts (as shown in the following). Therefore, our framework does
not have the usual obstacle of the cutoff dependence of the 𝑇 -matrix
present in the traditional chiral unitary approaches, which results in
parameter-free predictions.
̄
We are in the position to search poles appearing in the 𝜋Σ-𝐾𝑁
coupled-channel 𝑇 -matrix. One can perform an analytic continuation
of the 𝑇 -matrix into the complex 𝑠-plane. The 4 Riemann sheets, which
are labeled by the sign√of the imaginary part of the c.m. momentum
𝑝𝑖 = 𝜆1∕2 (𝑠, 𝑀𝑃2 , 𝑚2𝐵 )∕(2 𝑠) for each channel, are introduced. The most
relevant Riemann sheets in the current work are the physical sheet (+, +)
and the second Riemann sheet (−, +) with only the 𝜋Σ channel open for
decay. Furthermore, in order to investigate the structures of the poles,
one can parameterize the on-shell scattering 𝑇 -matrix around the pole
position 𝑧𝑅 ,
Fig. 2. The vector meson masses (left panel) and the pion decay constant (right
panel) as the functions of the pion mass with the quark mass trajectory 𝑚 =
𝑚symm . Notations are the same as Fig. 1.
𝑏𝐹 = −0.399 GeV−1 . The light-quark mass dependence of the baryon
masses is shown in the right panel of Fig. 1.
Besides, we also require the vector meson mass 𝑀𝑉 and the decay
constant 𝐹0 in the chiral limit to obtain the LO potential (Eq. (1)). In
practice, we use the experimental masses of vector mesons 𝑀𝜌, 𝜔, 𝐾 ∗ , 𝜙
and the pion decay constant 𝐹𝜋 or the SU(3) averaged decay constant
in Ref. [34]. The introduced difference between the chiral limit values
and the physical values of the vector meson masses and the meson decay constant is of higher order. As to the light-quark mass dependence
of 𝑀𝑉 , only rho meson mass 𝑀𝜌 is simulated with the quark mass trajectory 𝑚 = 𝑚symm of the CLS configuration by Mainz lattice group [43].
To determine the quark mass dependence of the vector meson masses,
we use the results of LO ChPT in the SU(3) sector [55],
(
)
𝑀𝜌2 = 𝑀𝜔2 = 𝑀02 + 2𝜆𝑚 𝑀𝜋2 + 𝜆0 2𝑀𝐾2 + 𝑀𝜋2 ,
(
)
𝑀𝐾2 ∗ = 𝑀02 + 2𝜆𝑚 𝑀𝐾2 + 𝜆0 2𝑀𝐾2 + 𝑀𝜋2 ,
(
)
𝑀𝜙2 = 𝑀02 + 4𝜆𝑚 𝑀𝐾2 − 2𝜆𝑚 𝑀𝜋2 + 𝜆0 2𝑀𝐾2 + 𝑀𝜋2 ,
(19)
where 𝑀𝜌 = 𝑀𝜔 . The three LECs 𝑀0 , 𝜆0 , and 𝜆𝑚 are determined by fitting the physical values of vector meson masses and the lattice data of
𝑀𝜌 , resulting in 𝑀0 = 0.538 GeV, 𝜆𝑚 = 0.468, 𝜆0 = 0.593. The reasonable fitting result is presented in the left panel of Fig. 2.
As to the quark mass dependence of the pion decay constant 𝐹𝜋 , the
lattice results of the CLS configuration are reported in Ref. [44] with
the quark mass trajectory 𝑚 = 𝑚symm . From Fig. 2, it seems that the lattice data for the small pion masses are slightly lower than the empirical
value. To describe the lattice results and obtain the pion mass dependence of 𝐹𝜋 , we follow the fitting procedure outlined in Ref. [38]. For
further details and formalism, one can refer to the appendix of Ref. [38].
The lowest order 𝑀0𝜋 , 𝑀0𝐾 , and the chiral limit value 𝐹0 are adjusted
by reproducing the experimental value and each set of lattice results
of 𝑀𝜋 , 𝑀𝐾 and 𝐹𝜋 given in Ref. [44]. We take two strategies to perform the fit: first, the LECs 𝐿𝑟𝑖 , 𝑖 = 4, 5, 6, 8 are fixed as Fit I of Ref. [56],
where the experimental and lattice meson-baryon scattering data are fitted. The pion mass dependence of 𝐹𝜋 is presented as the dashed line in
Fig. 2-(b). Although the lattice data with small pion masses are well covered, the experimental 𝐹𝜋 is underestimated and the lattice data with
large pion masses are overestimated. To achieve a relatively compatible
description, we release 𝐿𝑟5 and 𝐿𝑟8 in the fit, which leads to the solid line
𝑇𝑖𝑗 ≃ 4𝜋
𝑔 𝑖 𝑔𝑗
𝑧 − 𝑧𝑅
,
(20)
where the (complex) 𝑔𝑖 (𝑔𝑗 ) couplings are introduced to denote the
coupling strength of the resonance pole to the initial (final) transition
channel. Those couplings can be extracted from the residues of the 𝑇 matrix.
We find two poles on the (−, +) Riemann sheet, one is resonance
̄ threshold (denoted as “higher pole”), and another is the
around 𝐾𝑁
virtual bound state just below 𝜋Σ threshold (denoted as “lower pole”).
Their pole positions and the coupling strengths are tabulated in Table 1.
One can see that our prediction of pole positions is consistent with the
in Fig. 2-(b). In this case, the values of 𝐿𝑟5,8 come to 𝐿𝑟5 = 0.484 × 103
4
Physics Letters B 855 (2024) 138802
X.-L. Ren
the right panel of Fig. 4. At the physical point 𝑀𝜋 ≈ 135 MeV, the lower
pole is found on the (−, +, +, +) sheet and is recognized as a resonance.
Its position 𝑧𝑅 = 1320.5 − 𝑖80.4 MeV is above the 𝜋Σ threshold with a
relatively large imaginary part. As 𝑀𝜋 increases, the mass of the lower
pole slightly rises (but remains below the 𝜋Σ threshold when 𝑀𝜋 > 146
MeV), while the width decreases rapidly. Correspondingly, the effective
coupling of the lower pole to the 𝜋Σ channel also increases. This indicates that the interaction strength of 𝜋Σ is enhanced along with the
increase of 𝑀𝜋 . When the interaction is strong enough, the resonance
nature becomes a virtual bound state with 𝑀𝜋 ≥ 197 MeV. Because the
𝜋Σ interaction strength is continually enhanced, when 𝑀𝜋 ≥ 269 MeV,
the lower pole becomes a bound state, which is located on the physical
sheet. And the binding energy increases as the pion mass increases.
From the significantly different pictures of both poles’ evaluations,
̄ interaction gradually strengthens with the
one could infer that the 𝐾𝑁
increase of pion mass. Meanwhile, the strength of the 𝜋Σ interaction
changes rapidly and is enhanced sufficiently to render the lower pole of
Λ(1405) as a bound state.
We would like to remark that the similar analysis of the evolution of
the Λ(1405) pole positions at different quark masses has been reported
̄
in the 𝜋Σ-𝐾𝑁
coupled-channel study [40] by using the WeinbergTomozawa term within the traditional CUA, where the light-quark mass
dependence of the decay constant and the adjustable subtraction constants are neglected. In contrast, we incorporate the pion mass dependence of all the model variables based on the CLS configuration. Avoid
introducing the finite cutoff or the subtractive constants, we obtain the
renormalized scattering amplitudes. In this sense that, our LO results
of the quark mass dependence of Λ(1405), illustrated in Fig. 4, is a
model-independent prediction. The tendency of pole evolution could be
checked by the forthcoming studies from the BaSc Collaboration.
Furthermore, it is worth mentioning that in Refs. [36,39,41], the
evolution of two Λ(1405) poles has been studied in the SU(3) trajectory.
That’s corresponding to a trajectory from the SU(3) flavor limit to the
1
physical point by keeping the average quark mass 𝑚̄ = (2𝑚𝑢∕𝑑 + 𝑚𝑠 )
3
as a constant and varying a scaling parameter 𝑥 ∈ [0, 1], which is introduced in the pseudoscalar meson masses, octet baryon masses, the
meson decay constants, and the subtraction constants. At LO studies,
the higher pole changes from a bound state to a resonance varying 𝑥
from 0 to 1; correspondingly, the lower pole undergoes the bound state
to a virtual state and finally comes to a resonance. However, in the recent NLO study [41], the evolutions of both Λ(1405) poles along the
SU(3) trajectory are changed a lot by including the NLO corrections. It
gives us a hint that one needs to go a step further and include the NLO
corrections in our framework, at least, to see the changes of the evolution results shown in Fig. 4. Such a study is beyond the scope of the
present manuscript and will be reported in future publications.
Fig. 3. Evolution of lower pole position as a function of the momentum cutoff
Λ.
lattice results of BaSc Collaboration [30,31], except for the width of
the higher pole, which approaches the lower bound of lattice value. It
is interesting to note that the pole positions (𝑧𝑅 = 1389.05 MeV and
1464.55 − 𝑖9.44 MeV) are closer to the lattice results if we perform a full
̄ , 𝜂Λ, and 𝐾Ξ. Furthercalculation with four coupled channels 𝜋Σ, 𝐾𝑁
more, the values of 𝑔𝜋Σ,𝐾𝑁
and their ratios indicate that the lower pole
̄
couples predominantly to the 𝜋Σ channel, while the higher pole couples
̄ channel. The ratios of couplings are also consistent
strongly to the 𝐾𝑁
with the BaSc results [30,31]. Additionally, in Fig. 3, we present the
evolution of the lower pole position1 by varying the momentum cutoff
Λ from 700 MeV to 10 GeV. One can see that the finite-cutoff (Λ = 700
MeV) artifact changes the lower pole position up to 27 MeV. When Λ is
up to 3 GeV, the cutoff-independent result is achieved, which guaran̄ scattering amplitudes in our
tees the renormalizability of the 𝜋Σ-𝐾𝑁
scheme.
Next, we investigate the evolution of Λ(1405) poles by varying the
pion mass from 𝑀𝜋 ≈ 135 MeV to 400 MeV along with the quark mass
trajectory 𝑚 = 𝑚symm of the CLS configuration.
̄ coupled-channel calculation, we
Instead of performing the 𝜋Σ-𝐾𝑁
̄ , 𝜂Λ, and 𝐾Ξ to obtain
prefer to span all four coupled channels 𝜋Σ, 𝐾𝑁
the meson-baryon scattering amplitudes in the 𝑆 = −1 sector. Numerically, the LO potential (Eq. (1)) varies along with the pion mass since
the masses of pseudoscalar mesons, octet baryons, octet vector mesons,
and the pion decay constant,2 are determined by applying the chiral
expansion formulas with the CLS quark mass trajectory 𝑚 = 𝑚symm . Correspondingly, the pion mass dependence also enters the meson-baryon
Green function. Thus, by solving the integral equation (Eq. (3)) and utilizing the subtractive renormalization, one can obtain the renormalized
𝑇 -matrix. To search poles of 𝑇 -matrix on the complex 𝑠-plane, one needs
̄
to introduce 16 Riemann sheets for the 𝜋Σ, 𝐾𝑁,
𝜂Λ, and 𝐾Ξ couple
channels. Similar to the two coupled-channel case, the most relevant
Riemann sheets are the physical sheet (+, +, +, +) and the second Riemann sheet (−, +, +, +).
By changing the pion mass from the physical point 𝑀𝜋 = 135 MeV
̄ threshto 400 MeV, we always obtain two poles around the 𝜋Σ and 𝐾𝑁
olds in the coupled-channel 𝑇 -matrix. The corresponding pole positions
of Λ(1405) are presented in Fig. 4 as the function of pion mass. The
higher pole of Λ(1405) is always a resonance, located on the (−, +, +, +)
sheet. Its mass (width) increases (decreases) when the pion mass increases. For the small pion mass region, the higher pole is slightly below
̄ threshold, while for 𝑀𝜋 > 225 MeV, it begins above. This inthe 𝐾𝑁
̄ channel. Regarding
dicates the higher pole couples strongly to the 𝐾𝑁
the lower pole of Λ(1405), it is intriguing to observe that the evolution
of its position becomes more complicated as 𝑀𝜋 increase, as shown in
4. Conclusion
We applied a renormalizable framework of meson-baryon scattering
within covariant chiral effective field theory to investigate the Λ(1405)
resonance in the unphysical quark mass region. Confronting the recent
lattice calculation of BaSc Collaboration, our leading order analysis focuses on the quark mass trajectory 𝑚 = 𝑚symm of the CLS configuration.
First, we compared our parameter-free prediction of Λ(1405) double
poles with the lattice data of BaSc at 𝑀𝜋 ≈ 200 MeV and 𝑀𝐾 ≈ 487
MeV. The consistency result indicates the predictive capability of our
renormalizable approach.
Therefore, we investigated the quark mass dependence of the
Λ(1405) state along with the CLS quark mass trajectory 𝑚 = 𝑚symm . The
̄ threshold
higher pole of Λ(1405) is always a resonance around the 𝐾𝑁
by changing 𝑀𝜋 from 135 MeV to 400 MeV, while the evolution of the
lower pole of Λ(1405) is complicated: transitioning from a resonance to
a virtual state, and ultimately to a bound state of 𝜋Σ system. Such behavior could be verified by the forthcoming lattice calculation of the
BaSc Collaboration.
1
As to the higher pole, its mass and width have a similar Λ dependence.
Note that our description of 𝐹𝜋 is higher than the lattice data when 𝑀𝜋 ≤ 200
MeV, as shown in Fig. 2.
2
5
Physics Letters B 855 (2024) 138802
X.-L. Ren
Fig. 4. Λ(1405) poles as the function of pion mass with the CLS quark mass trajectory 𝑚 = 𝑚symm . The upper (lower) panel is the real (imaginary) part of the pole
position. The black-, red-, and blue-solid curves denote the pole as the resonance, virtual state, and bound state, respectively. The dashed lines correspond to the
̄ (left panel) and 𝜋Σ (right panel) thresholds.
𝐾𝑁
In order to polish the current results, we plan to extend the study to
next-to-leading order (at least) in our renormalizable framework. By incorporating the constraints from the experimental data (see the recent
review [15]), such as a large amount of cross sections for 𝐾 − 𝑝 scattering into different final channels, the relevant branching ratios, and the
precise energy shift and width of the 1𝑠 state in kaonic hydrogen by the
SIDDHARTA Collaboration [62] etc., we can improve the description of
̄ scattering to better determine the pole positions of Λ(1405). At
the 𝐾𝑁
this level, one could provide a moderately reliable prediction about the
light-quark dependence of Λ(1405) poles.
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Declaration of competing interest
The authors declare that they have no known competing financial
interests or personal relationships that could have appeared to influence
the work reported in this paper.
Data availability
No data was used for the research described in the article.
Acknowledgements
We appreciate the valuable discussions with Daniel Mohler during
the MENU 2023 conference. This work was supported by the Deutsche
Forschungsgemeinschaft (DFG, German Research Foundation), in part
through the Research Unit (Photonphoton interactions in the Standard
Model and beyond, Projektnummer 458854507—FOR 5327), and in
part through the Cluster of Excellence (Precision Physics, Fundamental
Interactions, and Structure of Matter) (PRISMA+ EXC 2118/1) within
the German Excellence Strategy (Project ID 39083149).
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