In particle physics, hexaquarks, alternatively known as sexaquarks,[1] are a large family of hypothetical particles, each particle consisting of six quarks or antiquarks of any flavours. Six constituent quarks in any of several combinations could yield a colour charge of zero; for example a hexaquark might contain either six quarks, resembling two baryons bound together (a dibaryon), or three quarks and three antiquarks.[2] Once formed, dibaryons are predicted to be fairly stable by the standards of particle physics.
A number of experiments have been suggested to detect dibaryon decays and interactions. In the 1990s, several candidate dibaryon decays were observed but they were not confirmed.[3][4][5]
There is a theory that strange particles such as hyperons[6] and dibaryons[7] could form in the interior of a neutron star, changing its mass–radius ratio in ways that might be detectable. Accordingly, measurements of neutron stars could set constraints on possible dibaryon properties.[8] A large fraction of the neutrons in a neutron star could turn into hyperons and merge into dibaryons during the early part of its collapse into a black hole . These dibaryons would very quickly dissolve into quark–gluon plasma during the collapse, or go into some currently unknown state of matter.
D-star hexaquark
In 2014, a potential dibaryon was detected at the Jülich Research Center at about 2380 MeV. The center claimed that the measurements confirm results from 2011, via a more replicable method.[9][10] The particle existed for 10−23 seconds and was named d*(2380).[11] This particle is hypothesized to consist of three up and three down quarks, and has been proposed as a candidate for dark matter.[12][13][14]
The study found that production of stable d*(2830) hexaquarks could account for 85% of the Universe's dark matter.[15][16]
H dibaryon
In 1977, Robert Jaffe proposed that a possibly stable H dibaryon with the quark composition udsuds could notionally result from the combination of two uds hyperons.[17][1][18][19][20][21][22][23]
Others
See also
- Deuteron, the only known stable composite particle that consists of six quarks.
- Dineutron, an extremely unstable dibaryon.
- Diproton, another extremely unstable dibaryon.
- Exotic hadron
- Pentaquark
References
- 1 2 "Oddball sexaquark particles could be immortal, if they exist at all".
- ↑ Vijande, J.; Valcarce, A.; Richard, J.-M. (2011). "Stability of hexaquarks in the string limit of confinement". Physical Review D. 85 (1): 014019. arXiv:1111.5921. Bibcode:2012PhRvD..85a4019V. doi:10.1103/PhysRevD.85.014019. S2CID 53511291.
- ↑ Belz, J.; et al. (BNL-E888 Collaboration) (1996). "Search for the weak decay of an H dibaryon". Physical Review Letters. 76 (18): 3277–3280. arXiv:hep-ex/9603002. Bibcode:1996PhRvL..76.3277B. doi:10.1103/PhysRevLett.76.3277. PMID 10060926. S2CID 15729745.
- ↑ Stotzer, R. W.; et al. (BNL-E888 Collaboration) (1997). "Search for H dibaryon in 3He (K−, K+) Hn". Physical Review Letters. 78 (19): 3646–36490. Bibcode:1997PhRvL..78.3646S. doi:10.1103/PhysRevLett.78.3646.
- ↑ Alavi-Harati, A.; et al. (KTeV Collaboration) (2000). "Search for the weak decay of a lightly bound H0 dibaryon". Physical Review Letters. 84 (12): 2593–2597. arXiv:hep-ex/9910030. Bibcode:2000PhRvL..84.2593A. doi:10.1103/PhysRevLett.84.2593. PMID 11017277. S2CID 119068614.
- ↑ Ambartsumyan, V. A.; Saakyan, G. S. (1960). "The Degenerate Superdense Gas of Elementary Particles". Soviet Astronomy. 37: 193. Bibcode:1960SvA.....4..187A.
- ↑ Kagiyama, S.; Nakamura, A.; Omodaka, T. (1992). "Compressible bag model and dibaryon stars". Zeitschrift für Physik C. 56 (4): 557–560. Bibcode:1992ZPhyC..56..557K. doi:10.1007/BF01474728. S2CID 121769383.
- ↑ Faessler, A.; Buchmann, A. J.; Krivoruchenko, M. I. (1997). "Constraints to coupling constants of the ω- and σ-mesons with dibaryons". Physical Review C. 56 (3): 1576–1581. arXiv:nucl-th/9706080. Bibcode:1997PhRvC..56.1576F. doi:10.1103/PhysRevC.56.1576. S2CID 119392781.
- ↑ "Forschungszentrum Jülich press release".
- ↑ "Massive news in the micro-world: a hexaquark particle".
- ↑ Adlarson, P.; et al. (2014). "Evidence for a New Resonance from Polarized Neutron-Proton Scattering". Physical Review Letters. 112 (2): 202301. arXiv:1402.6844. Bibcode:2014PhRvL.112t2301A. doi:10.1103/PhysRevLett.112.202301. S2CID 2280323.
- ↑ Bashkanov, M. (2020). "A new possibility for light-quark dark matter". Journal of Physics G. 47 (3): 03LT01. arXiv:2001.08654. Bibcode:2020JPhG...47cLT01B. doi:10.1088/1361-6471/ab67e8. S2CID 210861179.
- ↑ "Physicists Think We Might Have a New, Exciting Dark Matter Candidate".
- ↑ "Did this newfound particle form the universe's dark matter?".
- ↑ Williams, M. (11 March 2020). "Is the "D-star Hexaquark" the Dark Matter Particle?". Universe Today.
- ↑ "Ask Ethan: It's Absurd To Think Dark Matter Might Be Made Of Hexaquarks, Right?".
- ↑ Jaffe, R. L. (1977). "Perhaps a Stable Dihyperon?" (PDF). Physical Review Letters. 38 (5): 195–198. Bibcode:1977PhRvL..38..195J. doi:10.1103/PhysRevLett.38.195. OSTI 1446298.
- ↑ Farrar, G. R. (2017). "Stable Sexaquark". arXiv:1708.08951 [hep-ph].
- ↑ Kolb, E. W.; Turner, M. S. (2019). "Dibaryons cannot be the dark matter". Physical Review D. 99 (6): 063519. arXiv:1809.06003. Bibcode:2019PhRvD..99f3519K. doi:10.1103/PhysRevD.99.063519. S2CID 86859713.
- ↑ Gross, C.; Polosa, A.; Strumia, A.; Urbano, A.; Xue, W. (2018). "Dark matter in the standard model?". Physical Review D. 98 (6): 063005. arXiv:1803.10242. Bibcode:2018PhRvD..98f3005G. doi:10.1103/PhysRevD.98.063005. S2CID 119213361.
- ↑ Farrar, G. R. (2003). "A Stable H-Dibaryon: Dark Matter, Candidate Within QCD?". International Journal of Theoretical Physics. 42 (6): 1211–1218. doi:10.1023/A:1025702431127. S2CID 122452089.
- ↑ Farrar, G. R. (4 July 2019). "Stable Sexaquark: Dark Matter predictions, constraints and lab detection" (PDF). Quy Nhon Workshop.
- ↑ Azizi, K.; Agaev, S. S.; Sundu, H. (2020). "The Scalar Hexaquark uuddss: a Candidate to Dark Matter?". Journal of Physics G: Nuclear and Particle Physics. 47 (9): 095001. arXiv:1904.09913. Bibcode:2020JPhG...47i5001A. doi:10.1088/1361-6471/ab9a0e. S2CID 127956495.
- ↑ Lyu, Yan; Tong, Hui; Sugiura, Takuya; Aoki, Sinya; Doi, Takumi; Hatsuda, Tetsuo; Meng, Jie; Miyamoto, Takaya (2021-08-11). "Dibaryon with Highest Charm Number near Unitarity from Lattice QCD". Physical Review Letters. 127 (7): 072003. doi:10.1103/PhysRevLett.127.072003. hdl:2433/265092.
- ↑ "Exotic six-quark particle predicted by supercomputers". www.riken.jp. Retrieved 2022-01-21.