Knowledge (XXG)

Neutral current

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53: 1042: 850: 602:, etc. Because there is no transfer of electrical charge involved, exchange of Z particles is referred to as "neutral" in the phrase "neutral current". However the word "current" here has nothing to do with electricity – it simply refers to the exchange of the Z particle. 1187: 865: 712: 1388:
would also be an exception, if they were found to exist). However, any interaction between two charged particles that can occur via the exchange of a virtual Z boson can also occur via the exchange of a virtual
506: 1252: 1450: 1053: 1393:. Unless the interacting particles have energies on the order of the Z boson mass (91 GeV) or higher, the virtual Z boson exchange has an effect of a tiny correction, 1363: 68: 1320: 1037:{\displaystyle J^{{\mathsf {(NC)}}\ \mu }(f)={\bar {u}}_{f}\ \gamma ^{\mu }\ {\frac {1}{2}}\left(g_{\mathsf {V}}^{f}-g_{\mathsf {A}}^{f}\ \gamma ^{5}\right)\ u_{f}\ ,} 499: 1288: 559:. Like other subatomic forces, the weak force is mediated via exchange particles. Perhaps the most well known of the exchange particles for the weak force is the 146: 1455:
Particle accelerators with energies necessary to observe neutral current interactions and to measure the mass of Z boson weren't available until 1983.
492: 845:{\displaystyle {\mathfrak {M}}^{\mathsf {NC}}~\propto ~J_{\mu }^{\mathsf {(NC)}}(\nu _{\mathrm {e} })\;J^{{\mathsf {(NC)}}\ \mu }(\mathrm {e^{-}} )\ ,} 142: 571:– there are both positive and negative W particles – however the Z boson is also an exchange particle for the weak force but does 555:
The weak force is best known for its role in nuclear decay. It has very short range but (apart from gravity) is the only force to interact with
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of neutrinos in matter; neutrinos are almost as likely to scatter elastically (via Z boson exchange) as inelastically (via
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Gordon Fraser looks back at how confirmation of the existence of neutral currents ushered in a new understanding of physics.
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This article is about weak nuclear force interactions. For neutral currents in electric power systems, see
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The Z boson's neutral current interaction is determined by a derived quantum number called
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The neutral current that gives the interaction its name is that of the interacting particles.
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couplings amount to essentially left chiral for neutrinos and axial for charged leptons
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Sanje Fenkart reounts the discovery of neutral currents in its 50 years anniversary
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have distinctive signatures: They provide the only known mechanism for
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The Z boson can couple to any Standard Model particle, except
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exchange), of major experimental significance, in, e.g. , the
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Sudbury Neutrino Observatory#Neutral current interaction
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On the other hand, Z boson interactions involving
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Nieves, J.; Valverde, M.; Vicente Vacas, M.J. (2006).
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where the neutral currents describing the flow of the
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For example, the neutral current contribution to the
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Particle Physics (course notes). 1358:{\displaystyle \ Q_{\mathsf {W}}\ } 719: 1754:Fraser, Gordon (3 November 1998). 1420: 859:and of the electron are given by: 823: 779: 543:, and led to the discovery of the 25: 1792:"Gargamelle and neutral currents" 1615:"The Nobel Prize in Physics 1979" 173:Physics beyond the Standard Model 1586:"Lecture 11 - Weak Interactions" 1677:"Neutral current interaction". 1523:Flavor changing neutral current 27:Weak force particle interaction 1770:Fenkart, Sanje (3 July 2023). 1427: 1403: 1238: 1232: 1176: 1170: 1139: 1133: 1093: 1087: 917: 904: 898: 833: 818: 785: 770: 1: 527:can interact by means of the 117:Spontaneous symmetry breaking 1528:Neutral particle oscillation 1472:Sudbury Neutrino Observatory 575:have any electrical charge. 539:and the weak force into the 1833: 1661:. Research. Archived from 1330:their electric charge and 1256:vector and axial couplings 611:, which acts similarly to 147:Standard Model mathematics 29: 1786:Padilla, Antonio (Tony). 1772:"CERN's neutrino odyssey" 1315:{\displaystyle \ T_{3}\ } 1800:University of Nottingham 567:. W particles have 1706:Acta Physica Polonica B 1593:University of Edinburgh 135:Electroweak interaction 1538:Quantum chromodynamics 1446: 1359: 1316: 1284: 1248: 1183: 1038: 846: 139:Quantum chromodynamics 83: 1447: 1360: 1317: 1285: 1283:{\displaystyle \ f~.} 1249: 1184: 1039: 847: 563:which is involved in 169:Neutrino oscillations 89:of the Standard Model 82: 1481:developed mainly by 1397: 1334: 1293: 1265: 1196: 1054: 866: 713: 704:scattering amplitude 109:Quantum field theory 87:Elementary particles 1737:on 21 January 2012. 1728:2006AcPPB..37.2295N 1218: 1073: 996: 976: 769: 525:subatomic particles 1817:Electroweak theory 1479:electroweak theory 1464:elastic scattering 1442: 1355: 1312: 1280: 1244: 1202: 1179: 1057: 1034: 980: 960: 842: 744: 84: 32:Ground and neutral 1747:Symmetry Magazine 1690:"Neutral current" 1649:. 3 October 2004. 1569:"Neutral current" 1438: 1402: 1386:sterile neutrinos 1354: 1339: 1326:of the fermions, 1311: 1298: 1276: 1270: 1243: 1201: 1157: 1153: 1129: 1030: 1017: 999: 953: 944: 931: 920: 892: 838: 812: 743: 737: 541:electroweak force 517: 516: 165:Hierarchy problem 161:Strong CP problem 16:(Redirected from 1824: 1803: 1782: 1766: 1750: 1738: 1736: 1730:. 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Retrieved 1663:the original 1658: 1655:"Gargamelle" 1647:CERN Courier 1646: 1622:. Retrieved 1609: 1597:. Retrieved 1562: 1476: 1474:experiment. 1468:W boson 1457: 1454: 1375: 1324:weak isospin 1322:denotes the 1191: 1046: 854: 625: 622: 613:weak isospin 606: 604: 577: 572: 554: 533:Z boson 520: 518: 131:Constituents 113:Gauge theory 1788:Brady Haran 1595:. p. 7 1548:Weak charge 1483:Abdus Salam 1367:weak charge 608:weak charge 309:Chamberlain 157:Limitations 1680:Britannica 1669:2011-08-27 1624:2008-09-10 1554:References 1499:Gargamelle 619:Definition 565:beta decay 529:weak force 279:Iliopoulos 189:Rutherford 183:Scientists 143:CKM matrix 97:Background 1762:. 27904. 1688:Nave, R. 1567:Nave, R. 1460:neutrinos 1117:θ 1113:⁡ 1097:− 1002:γ 978:− 938:μ 934:γ 918:¯ 894:μ 828:− 814:μ 775:ν 750:μ 739:∝ 557:neutrinos 469:de Mayolo 414:Schwinger 354:Kobayashi 244:Gell-Mann 209:Sudarshan 1811:Category 1512:See also 1369:. 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Index

Neutral currents
Ground and neutral
Standard Model
particle physics
Elementary particles
Particle physics
Standard Model
Quantum field theory
Gauge theory
Spontaneous symmetry breaking
Higgs mechanism
Electroweak interaction
Quantum chromodynamics
CKM matrix
Standard Model mathematics
Strong CP problem
Hierarchy problem
Neutrino oscillations
Physics beyond the Standard Model
Rutherford
Thomson
Chadwick
Bose
Sudarshan
Davis Jr
Anderson
Fermi
Dirac
Feynman
Rubbia

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