Abstract
The QCD instanton can be observed at relatively low energies at Nica collider by studying the spin-spin correlations between the incoming proton and the produced \(\Lambda \) or \(\Sigma \) hyperons (or the \(\Lambda \) and \(\bar{\Lambda }\) hyperons). Low Nica energy will allow to better record and to measure the polarization of the hyperon originated by the polarized valence quark(s) in the proton fragmentation region.
Similar content being viewed by others
Avoid common mistakes on your manuscript.
1 Introduction
Instantons are non-perturbative field configurations [1] which describe semi-classical transitions between topologically inequivalent vacuum sectors in QCD. In the semi-classical limit, instantons provide dominant contributions to the path integral and describe quantum tunnelling between different vacuum sectors of the theory [2,3,4]. Instanton is either directly responsible for generating, or at least contributed to many key aspects of non-perturbative low-energy dynamics of strong interactions [5,6,7,8,9,10,11]. These include the role of instantons in the breaking of the \(U(1)_A\) symmetry and the spontaneous breakdown of the chiral symmetry, the formation of quark and gluon condensates, \(\langle 0|\bar{q}q|0\rangle \) and \(\langle 0|G^a_{\mu \nu }G^a_{\mu \nu }|0\rangle \) and so on.
Instanton solutions [1] have attracted a lot of interest over the years [2, 5, 11,12,13], but so far instanton/sphaleron production have not been observed experimentally in any particle physics settings.Footnote 1
The possibility to observe instantons in inelastic proton–proton collisions at hadron colliders was considered in [17, 18] and more recently in [19,20,21,22,23]. Instanton processes have large production cross-sections at small centre-of-mass partonic energies [19], but discovering them at hadron colliders remains challenging [20].
The problem is that the main signature of the instanton/sphaleron production is the generation of a large number of isotropically distributed mini-jets. That is in inelastic collision we are looking for the high multiplicity event with a large (S close to 1) sphericity. Unfortunately in such a case the background caused by the multiple parton interactions (which also lead to a higher multiplicity and a higher sphericity) in the underlying event is huge.
In the present paper we would like to explore another characteristic feature of the QCD instanton. Due to the presence of zero mode for the massless fermion [2, 5] each instanton/sphaleron production is accompanied by the creation of the light quark-antiquark pairs (one pair for each quark flavour).
Moreover the polarizations of these quarks are fixed. Instanton(I) produced the right quarks and the left antiquarks (for each light flavour) while the anti-instanton (\(\bar{I}\), with the opposite topological charge) – the left quarks and the right antiquarks.
2 Hyperon production
In terms of Feynman diagrams the instanton/sphaleron looks as the non-local vertex with \(n_g\) gluon and \(2n_f\) fermion legs. Here \(n_f\) is the number of light quarks with \(m_q<1/\rho \) (\(m_q\) is the curent quark mass and \(\rho \) is the instanton size). That is 2 (quark + antiquark) legs for each light flavour.
When the instanton was created in the quark-gluon collision the instanton absorbs left-handed quark and emits right-handed quarks (anti-instanton absorbs right-handed antiquarks and emits left-handed antiquarks)
The point is that the strong instanton gluon field rearranges the Dirac basement. One extra level of light left quark appears while the level of right quark goes upstairs to continuum spectra.Footnote 2 Note that the instanton not just flips the helicity of the incoming quark \(q_i\) (like it happens in the case of the pion or the kaon exchange) but simultaneously create the light quarks of another flavour but with the same helicity.
Thus by studying experimentally the spin-spin correlations, say in
process (see Fig. 1) we can observe the effects induced by the instanton production.
First at the quark level the instanton doubles the incoming polarization. Instead of one left \(u_L\)-quark it produces two right quarks – \(u_R\) and \(s_R\). To distinguish the ’left’ and ’right’ quarks we need weak interaction, that is weak decay of \(\Sigma \) or \(\Lambda \) hyperons.
Since within the SU(6) quark model the \(\Sigma \) hyperon contains the vector (ud) diquark (\(\Sigma =s(ud)_V\)) there should be a chance to observe in \(\Sigma \) the presence of two right quarks. This is impossible in \(\Lambda =s(ud)_S\) case where the (ud) diquark is the scalar. On the other hand \(\Lambda \) has the advantage – its polarization (in this model) is equal to the polarization of s-quark.
Another possibility is to produce the \(\bar{\Lambda }\Lambda \) pair and to check that \(\Lambda \) is right-handed while \(\bar{\Lambda }\) is left-handed on the contrary to the situation where the \(\bar{s}s\) pair was produced perturbatively by the gluon(s). Due to the helicity conservation in quark-gluon vertex here we have to get either two left-handed or two right-handed quarks.
To confirm that it was the instanton/sphaleron we could observe a larger than usual (at this energy) multiplicity and a stronger energy (\(\sqrt{s}\)) dependence and/or the additional spin-spin correlation when the second beam is polarized and the instanton is created via the quark-quark collision (instanton absorbs two left-handed quarks only).
2.1 Nica collider
The corresponding study can be performed at the Nica collider [24] where the incoming proton beams may be polarized both in the transverse or the longitudinal directions. The energy, \(\sqrt{s}=12-27\) GeV is not large but it will be sufficient to produce the sphaleron of the size \(\rho \sim 0.3\) Fm and the mass \(M_{inst}\sim 3-5\) GeV. The value \(\rho \sim 0.3\) Fm is the typical size of the instantons in the QCD vacuum [25, 26]. Since \(1/0.3\text{ Fm }\simeq 600\) MeV is larger than the current strange quark mass (\(m_s\sim 150\) MeV) such an instanton/sphaleron should emit u, d and s quarks plus few (\(n_g\sim 1/\alpha _s(\rho )\sim 1-3\)) gluons. Each parton has the energy \(E\sim 1/\rho =0.6\) GeV. That is to create such a sphaleron we need the energy \(M_{inst}\sim 4\) GeV.
It is known that the instanton production cross section steeply increases with \(\rho \) (that is with \(M_{inst}\) decreasing); see for example the Table 2 of [19] where it reaches of about 5 mb already at \(M_{inst}=10\) GeV. This is explained mainly by the decreasing of the instanton action \(S_{inst}=2\pi /\alpha _s\) (which suppresses as \(e^{-S_{inst}}\) the instanton contribution) due to the growth of \(\alpha _s(\rho )\).
Unfortunately at this low scale the precise behavior of QCD coupling \(\alpha _s(\rho )\) is not known. Therefore instead of the straightforward calculation we use the simple geometrical estimate \(\sigma \sim \pi \rho ^2\sim 3\) mb. However besides the probability to create the appropriate sphaleron we have to account for the small probability to form the hyperon in the final state. So we would expect the instanton contribution to the hyperon production to be of the order of few \(\mu \)b.
This is not too small value bearing in mind the Nica luminosity up to \(10^{32}\) cm\(^{-2}\)/s. The 1 \(\mu \)b cross section is comparable with that observed experimentally in the proton fragmentation region. Thus we hope that it will be possible to observe the instanton induced spin-spin correlations between the hyperons and the polarized incoming proton at the Nica collider.
It is not excluded that the QCD instanton/sphaleron does not exist in Nature (see e.g. [27]). This depends on the way used to formulate the theory - whether we allow for the singular gauge or the gluon fields weakly decreasing at infinity. Therefore it is important to search and to observe (or not observe) the instanton induced effects experimentally.
Data availability statement
This manuscript has no associated data or the data will not be deposited. [Authors’ comment: There are no corresponding data on spin-spin correlations at the moment.]
Notes
It was noticed by Bjorken [14] that the large (\(\sim \) 5%) branching of \(\eta _c\rightarrow \eta \pi \pi ,\ \eta '\pi \pi \, \text{ and }\, \bar{K}K\pi \) decays, naturally produced via the ’t Hooft instanton-induced interaction \(\mathcal{L}\sim (\bar{c}c)(\bar{u}u)(\bar{d}d)(\bar{s}s)\) can be considered as the experimental indication of the QCD instantanton presence (see also [15, 16]).
This is connected with the \(\gamma _5\) anomaly. In electro-week case where the \(\gamma _5\) anomaly is canceled between the quarks and the leptons this leads to the baryon charge non-conservation. In QCD this is the helicity non-conservation.
References
A.A. Belavin, A.M. Polyakov, A.S. Schwartz, Y.S. Tyupkin, Phys. Lett. 59B, 85 (1975)
G. ’t Hooft, Phys. Rev. D 14, 343 (1976) [Erratum: Phys. Rev. D 18 (1978) 2199]
C.G. Callan Jr., R.F. Dashen, D.J. Gross, Phys. Lett. 63B, 334 (1976)
R. Jackiw, C. Rebbi, Phys. Rev. Lett. 37, 172 (1976)
G. ’t Hooft, Phys. Rep. 142, 357 (1986)
C.G. Callan Jr., R.F. Dashen, D.J. Gross, Phys. Rev. D 17, 2717 (1978)
V.A. Novikov, M.A. Shifman, A.I. Vainshtein, V.I. Zakharov, Nucl. Phys. B 191, 301 (1981)
E.V. Shuryak, Nucl. Phys. B 203, 116 (1982)
D. Diakonov, V.Y. Petrov, Phys. Lett. 147B, 351 (1984)
D. Diakonov, V.Y. Petrov, Nucl. Phys. B 272, 457 (1986)
T. Schäfer, E.V. Shuryak, Rev. Mod. Phys. 70, 323 (1998). (hep-ph/9610451)
A.I. Vainshtein, V.I. Zakharov, V.A. Novikov, M.A. Shifman, Sov. Phys. Usp. 25, 195 (1982) [Usp. Fiz. Nauk 136 (1982) 553]
N. Dorey, T.J. Hollowood, V.V. Khoze, M.P. Mattis, Phys. Rep. 371, 231 (2002). hep-th/0206063
J.D. Bjorken, AIP Conf. Proc. 549(1), 211–229 (2000). arXiv:hep-ph/0008048
E. Shuryak, I. Zahed, arXiv:2102.00256 [hep-ph]
Valeriu Zetocha, Thomas Schäfer, Phys. Rev. D 67, 114003 (2003). arXiv:hep-ph/0212125
I.I. Balitsky, M.G. Ryskin, Phys. At. Nucl. 56, 1106 (1993) [Yad. Fiz. 56N8, 196 (1993)]
I.I. Balitsky, M.G. Ryskin, Phys. Lett. B 296, 185 (1992)
V.V. Khoze, F. Krauss, M. Schott, JHEP 2004, 201 (2020). arXiv:1911.09726 [hep-ph]
V.V. Khoze, D.L. Milne, M. Spannowsky, Phys. Rev. D 103(1), 014017 (2021). arXiv:2010.02287 [hep-ph]
S. Amoroso, D. Kar, M. Schott, Eur. Phys. J. C 81(7), 624 (2021). arXiv:2012.09120 [hep-ph]
V.A. Khoze, V.V. Khoze, D.L. Milne, M.G. Ryskin, Phys. Rev. D 104(5), 054013 (2021). arXiv:2104.01861 [hep-ph]
M. Tasevsky, V.A. Khoze, D.L. Milne, M.G. Ryskin, Eur. Phys. J. C 83, 35 (2023). arXiv:2208.14089 [hep-ph]
O. Brovko et al., JPS Conf. Proc. 35, 011003 (2021) [Contribution to: STORI’17; NICA Collaboration \(\bullet \) Alexander D. Kovalenko et al. PoS SPIN2018 (2019) 007 \(\bullet \) Contribution to: SPIN 2018, 007]
D. Diakonov, V.Yu. Petrov, Nucl. Phys. B 245, 259 (1984)
E. Shuryak, I. Zahed, e-Print: arXiv:2102.00256 [hep-ph]
M. Yamanaka, arXiv: 2212.10994 [hep-ph]
Acknowledgements
Author thanks V.A. Khoze for reading the manuscript.
Author information
Authors and Affiliations
Corresponding author
Ethics declarations
Funding
No funds, grants, or other support was received.
Rights and permissions
Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/.
Funded by SCOAP3. SCOAP3 supports the goals of the International Year of Basic Sciences for Sustainable Development.
About this article
Cite this article
Ryskin, M.G. Instanton induced spin–spin correlations. Eur. Phys. J. C 83, 674 (2023). https://doi.org/10.1140/epjc/s10052-023-11850-y
Received:
Accepted:
Published:
DOI: https://doi.org/10.1140/epjc/s10052-023-11850-y