Basics of doubly heavy tetraquarks
A. Valcarce, J.-M. Richard, J. Vijande

TL;DR
This paper reviews the stability of doubly heavy tetraquarks, analyzing four-body dynamics, color-mixing, and spin effects, concluding stability for certain configurations like $bbar uar d$ but instability for all-heavy tetraquarks.
Contribution
It provides a detailed analysis of the stability conditions of doubly heavy tetraquarks considering color and spin effects, with implications for all-heavy tetraquark states.
Findings
Stability is favored when $M_Q/m_q o ext{large}$.
The $bbar uar d$ tetraquark is predicted to be stable.
All-heavy tetraquarks are generally unstable.
Abstract
We outline the most important results regarding the stability of doubly heavy tetraquarks with an adequate treatment of the four-body dynamics. We consider both color-mixing and spin-dependent effects. Our results are straightforwardly applied to the case of all-heavy tetraquarks . We conclude that the stability is favored in the limit pointing to the stability of the state and the instability of all-heavy tetraquarks.
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Basics of doubly heavy tetraquarks
A Valcarce1
JM Richard2 and J Vijande3
1 Departamento de Física Fundamental e IUFFyM, Universidad de Salamanca, E-37008 Salamanca, Spain
2 Université de Lyon, Institut de Physique Nucléaire de Lyon, IN2P3-CNRS–UCBL,
4 rue Enrico Fermi, 69622 Villeurbanne, France
3 Unidad Mixta de Investigación en Radiofísica e Instrumentación Nuclear en Medicina (IRIMED), Instituto de Investigación Sanitaria La Fe (IIS-La Fe), Universitat de Valencia (UV) and IFIC (UV-CSIC), Valencia, Spain [email protected], [email protected], [email protected]
Abstract
We outline the most important results regarding the stability of doubly heavy tetraquarks with an adequate treatment of the four-body dynamics. We consider both color-mixing and spin-dependent effects. Our results are straightforwardly applied to the case of all-heavy tetraquarks . We conclude that the stability is favored in the limit pointing to the stability of the state and the instability of all-heavy tetraquarks.
1 Introduction
Despite the impression given by the recent flurry of studies dealing with multiquark states, flavor-exotic multiquarks have already a long history [1] and have motivated an abundant literature (see Ref. [2] for a recent compendium). In the pioneering work of Ader, Richard and Taxil [1] it was shown that four-quark configurations become more and more bound when the mass ratio increases. The critical value of for binding is somewhat model dependent.
Currently, a broad theoretical consensus about the existence of a stable axial vector doubly bottom tetraquark has been reached. Lattice QCD calculations find unambiguous signals for a stable bottom-light tetraquark [3]. Based on a diquark hypothesis, Ref. [4] uses the discovery of the baryon to calibrate the binding energy in a diquark. Assuming that the same relation is true for the binding energy in a tetraquark, it concludes that the axial vector state is stable. The Heavy-Quark Symmetry analysis of Ref. [5] predicts the existence of narrow doubly heavy tetraquarks. Using as input for the doubly bottom baryons, not yet experimentally measured, the diquark-model calculations of Ref. [4] also leads to a bound axial vector tetraquark. Other approaches, using Wilson twisted mass lattice QCD [6], also find a bound state. Few-body calculations using quark-quark Cornell-like interactions [7], simple color magnetic models [8], QCD sum rule analysis [9], or phenomenological studies [10] come to similar conclusions. More doubtful has become the prediction about the stability of all-heavy tetraquarks [11].
In the present note, we stress that a careful treatment of the few-body problem is required before drawing any conclusion about the existence of stable states in a particular model. There is, indeed, a dramatic spread of strategies: some authors use the full machinery of a variational method based on correlated Gaussians or hyperspherical expansion, and others use a crude trial wave function or a cluster approximation.
2 General results based on symmetry breaking
The analogy between the stability of few-charge systems and multiquarks in additive chromoelectric potentials offers a good guidance for identifying the favorable configurations. There are, however, some differences mainly due to the color algebra replacing the simpler algebra of electric charges. Unlike in the case of the positronium molecule, the equal-mass tetraquarks are unstable in the chromoelectric model with frozen color wave functions [12, 13]. In both the atom and quark cases, the four-body system and its threshold, after simple rescaling, are governed by a generic Hamiltonian
[TABLE]
with in the atomic case, and in the quark case [14].
In quantum mechanics, the minimum of a Hamiltonian containing a symmetric and an antisymmetric term is always lower than the minimum of the symmetric part. From this result, one can analyze the effect of symmetry breaking in systems of four-charged particles. Let us first consider the hydrogen molecule, . The Hamiltonian for this system reads,
[TABLE]
where . The -parity breaking term, , lowers the ground state energy of with respect to the -parity even part, , which is simply a rescaled version of the Hamiltonian of the positronium molecule. Since and have the same threshold, and since the positronium molecule is stable, the hydrogen molecule is even more stable, and stability improves when increases. Clearly, the Coulomb character of hardly matters in this reasoning. The key property is that the potential does not change when the masses are modified.
One can use the same reasoning to study the stability of four-charged particles when -parity is preserved but particle symmetry is broken, in other words the configuration. The Hamiltonian is that of Eq. (2) by exchanging . The same arguments used above lead to the conclusion that this configuration gains binding with respect to the threshold that it shares with . However, there is another threshold that lies lower, . This threshold gains more from the symmetry breaking than the four-body molecule, and, indeed, it is found that the molecule becomes unstable for .
The above arguments can be directly translated to four-quark systems: the configuration becomes more and more bound when the mass ratio increases. This has been first established in Ref. [1], and discussed and confirmed in further studies. Arguments based on diquarks, as e.g. [4], might considerably overestimate the binding, as analyzed in [2]. There are many variants of the so-called diquark model. An extreme point of view is that diquarks are almost-elementary objects, with their specific interaction with quarks and between them. In the case of doubly heavy baryons there is obviously a clustering which makes it tempting to use a two-step approach: first a diquark and then a quasi-meson, as the diquark has the same color as an antiquark. The exercise can be repeated for the states. For simplicity, we consider only the case of a frozen color wave function, i.e., the Hamiltonian (1). In Fig. 1, we compare the exact solution of (1) with the approximation consisting of first computing the diquark with alone and with alone, and then as a meson with a potential and constituent masses and .
A remaining problem is to understand why the positronium molecule lies slightly below its dissociation threshold, while a chromoelectric model associated with the color additive rule does not bind (at least according to most computations). This is due to a larger disorder in the color coefficients than in the electrostatic strength factors entering the Coulomb potential [13]. An alternative proof is based on the so-called Hall-Post inequalities [15, 16]. The principle is rather simple. If a Hamiltonian is decomposed as a sum of Hamiltonians,
[TABLE]
then for the lowest energy,
[TABLE]
With a color wave function and a quark mass set to for simplicity, the Hamiltonian of the all-heavy tetraquark can be written as [13],
[TABLE]
where is the quarkonium potential. Now, we can rewrite this expression as,
[TABLE]
where is the quarkonium Hamiltonian. By using Eq.( 4) one gets,
[TABLE]
that demonstrates the instability of all-heavy tetraquarks. The above reasoning on the ground state holds for a single color channel. It is observed in explicit computations than the mixing of color states does no help much [7, 17]. The lower bound (7) can even be significantly improved if one relates Hamiltonians that are free of center-of-mass motion [2].
3 Color dynamics.
In the heavy-quark limit, the lowest lying tetraquark configuration resembles the helium atom [5], a factorized system with separate dynamics for the compact color nucleus and for the light quarks bound to the stationary color state, to construct a color singlet. This argument has been mathematically proved and numerically checked time ago [18], see the probabilities for the axial vector tetraquark shown in Table II (note that the probability in a compact tetraquark tends to zero for ).
The model of Eq. (1), with a pairwise potential due to color-octet exchange, induces mixing between and states in the basis. If one starts from a state with in a spin triplet, and, for instance with spin and isospin , then its orbital wave function is mainly made of an -wave in all coordinates. It can mix with a color with orbital excitations in the and linking and , respectively. A minimal wave function in this sector can be chosen as:
[TABLE]
To illustrate the role of color-mixing we use the potential AL1 [19]. Its central part is a Coulomb-plus-linear potential. Its spin-spin part is a regularized Breit-Fermi interaction, with a smearing parameter that depends on the reduced mass.
The energy as a function of without and with color-mixing is shown in the left panel of Fig. 2. The ground state of the , candidate for stability with , has its main component with color , and spin in the basis. The main admixture consists of with spin and an antisymmetric orbital wave function of which (3) is a prototype, and of with spin with a symmetric orbital wave function.
Note how the diquark hypothesis and color mixing have opposite effects that tend to cancel in the charm sector.
4 Spin-dependent corrections
In Ref. [20] it was acknowledged that, within current models, a pure additive interaction such as (1) will not bind , on the sole basis that this tetraquark configuration benefits from the strong chromoelectric attraction that is absent in the threshold. When , there is in addition a favorable chromomagnetic interaction in the tetraquark, while the threshold experiences only heavy-light spin-spin interaction, whose strength is suppressed by a factor .
For illustration, we use the again the potential AL1 [19]. The results are shown in the right panel of Fig. 2 for , as a function of the mass ratio . The system is barely bound without the spin-spin term, though the mass ratio is very large. It acquires its binding energy of the order of 150 MeV when the spin-spin is restored. The system is clearly unbound when the spin-spin interaction is switched off. This is shown here for the AL1 model, but this is true for any realistic interaction, including an early model by Bhaduri et al. [21]. The case of is actually remarkable. Here the binding requires both the color mixing of with , and the spin-spin interaction. Moreover, the binding is so tiny that it cannot be obtained with a simple variational method. One needs either a fully converged expansion on a basis of correlated Gaussians, or a hyperspherical expansion up to a grand orbital momentum of the order of 12. Semay and Silvestre-Brac [19], who used the AL1 potential, missed the binding, but their method of systematic expansion on the eigenstates of an harmonic oscillator is not very efficient to account for the short-range correlations. Janc and Rosina [22] were the first to obtain binding with such potentials, and their calculation was checked in Ref. [7]. The stability of with is with respect to the nominal threshold. Depending on its binding energy, it decays into or . The analog decays weakly.
5 Conclusions
The four-body problem of tetraquarks is rather delicate, especially for systems at the edge of stability. The analogy with atomic physics is a good guidance to indicate the most favorable configurations. However, unlike the positronium molecule, the all-heavy configuration is not stable if one adopts a standard quark model and solve the four-body problem correctly. The mixing of the and color configurations is important, especially for states very near the threshold. This mixing occurs by both the spin-independent and the spin-dependent parts of the potential.
Approximations are welcome, especially if they shed some light on the four-body dynamics. The diquark-antidiquark approximation is not supported by a rigorous solution of the 4-body problem, but benefits of a stroke of luck, as the erroneous extra attraction introduced in the color channel is somewhat compensated by the neglect of the coupling to the color channel.
Finally, with is at the edge of binding within current quark models. For this state, all contributions should be added, in particular the mixing of states with different color structure, and the four-body problem should be solved with extreme accuracy. In comparison, achieving the binding of looks easier. Still, with a typical quark model, the stability of the ground state cannot be reached if spin-effects and color mixing are both neglected.
\ack
Work funded by Ministerio de Economía, Industria y Competitividad and EU FEDER under Contract No. FPA2016-77177 and by Generalitat Valenciana PrometeoII/2014/066.
References
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The reference list from the paper itself. Each links out to its DOI / PubMed record.
- 1[1] Ader J P, Richard J M and Taxil P 1982 Phys. Rev. D 25 2370
- 2[2] Richard J M, Valcarce A and Vijande J 2018 Phys. Rev. C 97 035211
- 3[3] Francis A, Hudspith R J, Lewis R and Maltman K 2017 Phys. Rev. Lett. 118 142001
- 4[4] Karliner M and Rosner J L 2017 Phys. Rev. Lett. 119 202001
- 5[5] Eichten E J and Quigg C 2017 Phys. Rev. Lett. 119 202002
- 6[6] Bicudo P, Cichy K, Peters A and Wagner M 2016 Phys. Rev. D 93 034501
- 7[7] Vijande J, Valcarce A and Barnea N 2009 Phys. Rev. D 79 074010
- 8[8] Luo S Q, Chen K, Liu X, Liu Y R and Zhu S L 2017 Eur. Phys. J. C 77 709
