Generated by DeepSeek V3.2| strange quark | |
|---|---|
| Name | strange quark |
| Composition | Elementary particle |
| Statistics | Fermionic |
| Group | Quark |
| Generation | Second |
| Interaction | Strong, Weak, Electromagnetic, Gravity |
| Antiparticle | Strange antiquark (s) |
| Theorized | Murray Gell-Mann (1964), George Zweig (1964) |
| Discovered | SLAC (1968) |
| Mass | 95±5 MeV/c² |
| Electric charge | –1/3 ''e'' |
| Spin | 1/2 |
| Weak isospin | L: –1/2, R: 0 |
| Weak hypercharge | L: 1/3, R: –2/3 |
strange quark. It is a second-generation Fermion and a fundamental constituent of Matter, carrying a fractional Electric charge of –1/3. The particle was postulated to explain the unexpectedly long lifetimes of certain Hadrons discovered in Cosmic ray experiments, a property termed "strangeness." Its existence was a cornerstone in the development of the Quark model and the broader Standard Model of Particle physics.
The strange quark is characterized by a relatively large Rest mass compared to the lighter Up quark and Down quark, with a value around 95 MeV/c² as defined within the MS-bar scheme. It possesses Spin-½ and carries Color charge, participating in the Strong interaction mediated by Gluons. Its flavor quantum number, strangeness, is defined as –1 for the quark and +1 for its Antiparticle, the strange antiquark. The quark decays into lighter quarks via the Weak interaction, governed by the CKM matrix, with a Mean lifetime on the order of 10–10 seconds for bound states, which is long by particle physics standards.
The concept of the strange quark emerged from the study of Strange particles like the Kaon and the Lambda baryon, first observed in Cloud chamber photographs of Cosmic ray interactions in the late 1940s by groups including those at the University of Manchester. Their slow decay rates, explained by Murray Gell-Mann and Kazuhiko Nishijima through the new quantum number of strangeness, defied the expectations of the then-prevalent theories. In 1964, Murray Gell-Mann and, independently, George Zweig proposed the Quark model, positing the strange quark as one of the fundamental building blocks. Direct evidence for quarks, including strangeness, came from Deep inelastic scattering experiments conducted at the SLAC National Accelerator Laboratory in 1968, led by researchers like Jerome I. Friedman, Henry W. Kendall, and Richard E. Taylor.
The strange quark is a key constituent in many Hadrons classified as either Mesons or Baryons. In mesons, it forms bound states with its own Antiquark (e.g., the Phi meson) or with lighter antiquarks, such as in the charged Kaon (K+ = u). Among baryons, it is a component of the Lambda baryon (uds), the Sigma baryon (uus, uds, dds), the Xi baryon (uss, dss), and the triply-strange Omega baryon (sss). The mass and decay patterns of these particles, studied at facilities like CERN and Fermilab, provided critical tests for the Quark model and Quantum chromodynamics.
Hypothetical forms of matter rich in strange quarks, such as Strange matter and Strangelets, have been proposed as possible constituents of ultra-dense astrophysical objects. Some models suggest that the core of Neutron stars may undergo a phase transition to form Quark matter or a Quark–gluon plasma containing strange quarks, potentially observable through the mass-radius relationship measured by observatories like the Chandra X-ray Observatory. The concept of a Strange star, a celestial body composed almost entirely of strange matter, remains a speculative but active area of research in Astrophysics. Searches for strangelets have been conducted in experiments at the Relativistic Heavy Ion Collider and the Large Hadron Collider.
Strange quarks are routinely produced in high-energy particle collisions. In Particle accelerator experiments at CERN, Fermilab, and Brookhaven National Laboratory, they are generated via Strong interaction processes in collisions of Protons or Heavy ions, or through Weak interaction decays of heavier quarks like the Charm quark or Bottom quark. They are never observed in isolation due to Color confinement; detection instead relies on identifying their decay products. Sophisticated Particle detector systems, such as those in ATLAS, CMS, ALICE, and STAR, track the jets of Hadrons and Leptons resulting from strange hadron decays, allowing physicists to reconstruct the presence and properties of the primordial strange quark.
Category:Quarks Category:Elementary particles Category:Standard Model