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Muon spin spectroscopy

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limitations for this type of source, however: (i) unrejected charged particles accidentally hitting the detectors produce non-negligible random background counts; this compromises measurements after a few muon lifetimes, when the random background exceeds the true decay events; and (ii) the requirement to detect muons one at a time sets a maximum event rate. The background problem can be reduced by the use of electrostatic deflectors to ensure that no muons enter the sample before the decay of the previous muon. PSI and TRIUMF host the two continuous muon sources available for μSR experiments.
701:). In these beams, muons arise from pions decaying at rest inside but near the surface of the production target. Such muons are 100% polarized, ideally monochromatic, and have a very low momentum of 29.8 MeV/c (corresponding to a kinetic energy of 4.1 MeV). They have a range width in matter of the order of 180 mg/cm. The paramount advantage of this type of beam is the ability to use relatively thin samples. Beams of this type are available at PSI (Swiss Muon Source SμS), TRIUMF, J-PARC, 733:
The tunable energy range of such muon beams corresponds to implantation depths in solids of less than a nanometer up to several hundred nanometers. Therefore, the study of magnetic properties as a function of the distance from the surface of the sample is possible. At the present time, PSI is the only facility where such a low-energy muon beam is available on a regular basis. Technical developments have been also conducted at RIKEN-RAL, but with a strongly reduced low-energy muon rate.
1213:, roughly 10 μs. The asymmetry in the muon decay correlates the positron emission and the muon spin directions. The simplest example is when the spin direction of all muons remains constant in time after implantation (no motion). In this case the asymmetry shows up as an imbalance between the positron counts in two equivalent detectors placed in front and behind the sample, along the beam axis. Each of them records an exponentially decaying rate as a function of the time 33: 772:
after the incoming muon pulse, strongly reducing the accidental background counts. The virtual absence of background allows the extension of the time window for measurements up to about ten times the muon mean lifetime. The principal downside is that the width of the muon pulse limits the time resolution. ISIS Neutron and Muon Source and J-PARC are the two
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order for it to effectively influence the probe's dynamics: for every excitation interacting with the muon (lattice vibrations, charge and electronic spin waves) only those spectral components very closely matching the muon precession frequency in the specific experimental condition can cause a significant muon spin motion.
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Although such a high energy beam requires the use of suitable moderators and samples with sufficient thickness, it guarantees a homogeneous implantation of the muons in the sample volume. Such beams are also used to study specimens inside of recipients, e.g. samples inside pressure cells. Such muon beams are available at
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for the detector looking towards and away from the spin arrow, respectively. Considering that the huge muon spin polarization is completely outside thermal equilibrium, a dynamical relaxation towards the equilibrium unpolarized state typically shows up in the count rate, as an additional decay factor
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Resonance techniques are often characterized by the use of resonant circuits, which is not the case for muon spin spectroscopy. However the true resonant nature of all these techniques, muon spectroscopy included, lies in the very narrow, resonant requirement upon any time dependent perturbation in
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ions (i.e., Mu or μ e e) in vacuum. In 1987, the slow μ production rate was increased 100-fold using thin-film rare-gas solid moderators, producing a usable flux of low-energy positive muons. This production technique was subsequently adopted by PSI for their low-energy positive muon beam facility.
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A special case of LF μSR is Zero Field (ZF) μSR, when the external magnetic field is zero. This experimental condition is particularly important since it allows to probe any internal quasi-static (i.e. static on the muon time-scale) magnetic field of field distribution at the muon site. Internal
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The muons are implanted into the sample of interest where they lose energy very quickly. Fortunately, this deceleration process occurs in such a way that it does not jeopardize a μSR measurement. On one side it is very fast (much faster than 100 ps), which is much shorter than a typical μSR time
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hitting the production target are bunched into short, intense, and widely separated pulses that provide a similar time structure in the secondary muon beam. An advantage of pulsed muon sources is that the event rate is only limited by detector construction. Furthermore, detectors are active only
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with a field of several tesla. If the pion momentum is not too high, a large fraction of the pions will have decayed before they reach the end of the solenoid. In the laboratory frame the polarization of a high-energy muon beam is limited to about 80% and its energy is of the order of ~40-50MeV.
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muon sources no dominating time structure is present. By selecting an appropriate incoming muon rate, muons are implanted into the sample one-by-one. The main advantage is that the time resolution is solely determined by the detector construction and the read-out electronics. There are two main
1892:(JINR) in Dubna, Russia. The International Society for μSR Spectroscopy (ISMS) exists to promote the worldwide advancement of μSR. Membership in the society is open free of charge to all individuals in academia, government laboratories and industry who have an interest in the society's goals. 215:
More generally speaking, muon spin spectroscopy includes any study of the interactions of the muon's magnetic moment with its surroundings when implanted into any kind of matter. Its two most notable features are its ability to study local environments, due to the short effective range of muon
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interactions with matter, and the characteristic time-window (10 – 10 s) of the dynamical processes in atomic, molecular and condensed media. The closest parallel to μSR is "pulsed NMR", in which one observes time-dependent transverse nuclear polarization or the so-called "
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on temperature and magnetic field directly indicates the symmetry of the superconducting gap. Muon spin spectroscopy provides a way to measure the penetration depth, and so has been used to study high-temperature cuprate superconductors since their discovery in 1986.
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quasi-static fields may appear spontaneously, not induced by the magnetic response of the sample to an external field They are produced by disordered nuclear magnetic moments or, more importantly, by ordered electron magnetic moments and orbital currents.
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Mrad(sT), the frequency spectrum obtained by means of this experimental arrangement provides a direct measure of the internal magnetic field intensity distribution. The distribution produces an additional decay factor of the experimental asymmetry
254:. Indeed, with one muon hitting each square centimeter of the earth's surface every minute, the muons constitute the foremost constituent of cosmic rays arriving at ground level. However, μSR experiments require muon fluxes of the order of 817:, markedly distinguished by their electronic (charge) state. The spectroscopy of a muon chemically bound to an unpaired electron is remarkably different from that of all other muon states, which motivates the historical distinction in 1615: 1529: 196:, muon spin spectroscopy is also known as μSR. The acronym stands for muon spin rotation, relaxation, or resonance, depending respectively on whether the muon spin motion is predominantly a rotation (more precisely a 133: 975: 137: 136: 132: 131: 2070:
Harshman, D. R.; Mills, A. P. Jr.; Beveridge, J. L.; Kendall, K. R.; Morris, G. D.; Senba, M.; Warren, J. B.; Rupaal, A. S.; Turner, J. H. (1987). "Generation of Slow Positive Muons from Solid Rare-Gas Moderators".
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spin spectroscopy is an atomic, molecular and condensed matter experimental technique that exploits nuclear detection methods. In analogy with the acronyms for the previously established spectroscopies
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are ejected with spin antiparallel to their momentum in the pion rest frame. This is the key to provide spin-polarised muon beams. According to the value of the pion momentum different types of
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In addition to the above-mentioned classification based on energy, muon beams are also divided according to the time structure of the particle accelerator, i.e. continuous or pulsed.
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to deduce the sample properties. In contrast, the implanted muons are not diffracted but remain in a sample until they decay. Only a careful analysis of the decay product (i.e. a
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As with many of the other nuclear methods, μSR relies on discoveries and developments made in the field of particle physics. Following the discovery of the muon by
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with energy down to the eV-keV range) can be obtained by further reducing the energy of an Arizona beam by utilizing the energy-loss characteristics of large
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is an intrinsic asymmetry parameter determined by the weak decay mechanism. This anisotropic emission constitutes in fact the basics for the μSR technique.
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antiparallel to their linear momentum (likewise only right-handed anti-neutrino are found in nature). Since the pion is spinless both the neutrino and the
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Although particles are used as a probe, μSR is not a diffraction technique. A clear distinction between the μSR technique and those involving neutrons or
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in matter and on the detection of the influence of the atomic, molecular or crystalline surroundings on their spin motion. The motion of the muon
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is measured over a statistical ensemble of implanted muons and it depends on further experimental parameters, such as the beam spin polarization
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is due to the magnetic field experienced by the particle and may provide information on its local environment in a very similar way to other
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for the production of a muon beam. This is presently achieved at few large scale facilities in the world: the CMMS continuous source at
165: 1178:=1/3 is obtained if all emitted positrons are detected with the same efficiency, irrespective of their energy. Practically, values of 306:
The collision of an accelerated proton beam (typical energy 600 MeV) with the nuclei of a production target produces positive pions (
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with the field direction. In this case the muon spin precession describes a cone which results in both a longitudinal component,
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are formed by the pions escaping the production target at high energies. They are collected over a certain solid angle by
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Muon spin rotation and relaxation are mostly performed with positive muons. They are well suited to the study of
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The decay of the positive muon into a positron and two neutrinos occurs via the weak interaction process after a
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A more general case is when the initial muon spin direction (coinciding with the detector axis) forms an angle
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The figure shows the precession cone of the muon spin around the external magnetic field, that forms an angle
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a collective screening cannot take place and the muon will usually pick up one electron and form a so-called
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Other important fields of application of μSR exploit the fact that positive muons capture electrons to form
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electrons. Thus, in metals, the muon is not bound to a single electron, hence it is in the so-called
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window (up to 20 μs), and on the other side, all the processes involved during the deceleration are
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solid moderators. This technique was pioneered by researchers at the TRIUMF cyclotron facility in
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Harshman, D. R.; et al. (1986). "Observation of Low Energy μ Emission from Solid Surfaces".
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in some of the simplest types of chemical reactions, as well as the early stages of formation of
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muon states really behave like paramagnetic centers, according to the standard definition of a
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as the moderating solid. The same 1986 paper also reported the observation of negative
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of the muons being produced: high-energy, surface or "Arizona", and ultra-slow muon beams.
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Integrated Infrastructure Initiative for Neutron Scattering and Muon Spectroscopy (NMI3)
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in Tsukuba, Japan. Muon beams are also available at the Laboratory of Nuclear Problems,
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muons per second per square centimeter. Such fluxes can only be obtained in high-energy
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facility in Tokai, Japan, where a new pulsed source is being built to replace that at
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The London penetration depth is one of the most important parameters characterizing a
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in the weak interactions implies that only left-handed neutrinos exist, with their
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Pifer, A.E.; Bowen, T.; Kendall, K.R. (1976). "A high stopping density μ+ beam".
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techniques, for example, use the change in energy and/or momentum of a scattered
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encountered in compounds occurring in nature or artificially produced by modern
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at the atomic scale inside matter, such as those produced by various kinds of
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Parity violation in the weak interaction leads in this more complicated case (
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in organic chemicals. Muonium is also studied as an analogue of hydrogen in
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is projecting the development of a high-intensity low-energy muon beam.
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Another simple type of μSR experiment is when implanted all muon spins
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The muon spin motion may be measured over a time scale dictated by the
854: 768: 729: 232: 1614: 2013: 1881: 1865: 1393: 1313:{\displaystyle N_{\alpha }(t)=N_{0}\exp(-t/\tau _{\mu })(1+\alpha A)} 1054:{\displaystyle W(\theta )d\theta \propto (1+a\cos \theta )d\theta ~,} 734: 721: 675: 671: 645: 224: 1611:. This method is usually referred to as Transverse Field (TF) μSR. 250:
in 1936, pioneer experiments on its properties were performed with
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is the angle between the positron trajectory and the μ-spin, and
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because its inverse square provides a measure of the density
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coherently around the external magnetic field of modulus
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Muon beams are classified into three types based on the
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in Vancouver, Canada; the SμS continuous source at the
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and directed onto a decay section consisting of a long
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atom. This allows investigation of the largest known
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state and behaves like a free muon. In insulators or
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which have been developed during the last 50 years.
57:. Unsourced material may be challenged and removed. 1767: 1719: 1683: 1659: 1630: 1598: 1562: 1523: 1408: 1384: 1353:in front of the experimental asymmetry parameter, 1344: 1312: 1190: 1170: 1146: 1119: 1096: 1076: 1053: 969: 628: 601: 564: 501: 474: 433: 325: 286: 2133:Video - What are muons and how are they produced? 2122: 685:The second type of muon beam is often called the 1768:{\displaystyle A\sin ^{2}\theta \cos \omega t} 1416:between the same two detectors, according to 873:atom. This is the prototype of the so-called 837:, the muon's positive charge is collectively 693:beam (recalling the pioneering work of Pifer 8: 776:muon sources available for μSR experiments. 1992:Bowen, T. (1985). "The Surface Muon Beam". 636:-beams are available for μSR measurements. 1727:, and a transverse precessing component, 708:Positive muon beams of even lower energy ( 142:Muon Spin Resonance basic principle (Musr) 1741: 1732: 1705: 1696: 1676: 1646: 1645: 1643: 1623: 1584: 1578: 1551: 1539: 1482: 1473: 1452: 1430: 1424: 1401: 1377: 1328: 1283: 1274: 1253: 1231: 1225: 1183: 1163: 1138: 1132: 1112: 1089: 1069: 992: 955: 944: 943: 933: 920: 907: 901: 620: 614: 593: 587: 553: 540: 527: 521: 493: 487: 464: 459: 453: 421: 379: 343: 341: 317: 311: 278: 265: 259: 117:Learn how and when to remove this message 1217:elapsed from implantation, according to 1949: 1928: 1832:atoms which behave chemically as light 1563:{\displaystyle \omega =\gamma _{\mu }B} 1599:{\displaystyle \gamma _{\mu }=851.616} 1155: 444:From the subsequent weak decay of the 2128:The NMI3 Muon Joint Research Activity 1638:with the initial muon spin direction 212:technique to align the probing spin. 7: 1890:Joint Institute for Nuclear Research 1880:in Chilton, United Kingdom; and the 1876:and RIKEN-RAL pulsed sources at the 1872:(PSI) in Villigen, Switzerland; the 227:is that scattering is not involved. 55:adding citations to reliable sources 857:(Mu=μ+e), which has similar size ( 25: 1720:{\displaystyle A\cos ^{2}\theta } 809:The positive muons usually adopt 208:pulses. μSR does not require any 475:{\displaystyle \tau _{\pi ^{+}}} 172:(ESR or EPR) and, more closely, 31: 1959:Nuclear Instruments and Methods 1198:≈ 0.25 are routinely obtained. 42:needs additional citations for 1878:Rutherford Appleton Laboratory 1651: 1534:Since the Larmor frequency is 1518: 1491: 1488: 1464: 1442: 1436: 1307: 1292: 1289: 1265: 1243: 1237: 1036: 1015: 1003: 997: 949: 913: 881:Detection of muon polarization 533: 400: 358: 333:) via the possible reactions: 1: 1917:Perturbed angular correlation 1345:{\displaystyle \alpha =\pm 1} 287:{\displaystyle 10^{4}-10^{7}} 1979:10.1016/0029-554X(76)90823-5 1874:ISIS Neutron and Muon Source 703:ISIS Neutron and Muon Source 640:Energy classes of muon beams 482:= 26.03 ns) positive muons ( 2049:10.1103/PhysRevLett.56.2850 2169: 1912:Nuclear magnetic resonance 1660:{\displaystyle {\hat {x}}} 174:nuclear magnetic resonance 2093:10.1103/PhysRevB.36.8850 1147:{\displaystyle P_{\mu }} 815:crystallographic lattice 629:{\displaystyle \mu ^{+}} 602:{\displaystyle \mu ^{+}} 502:{\displaystyle \mu ^{+}} 326:{\displaystyle \pi ^{+}} 66:"Muon spin spectroscopy" 2029:Physical Review Letters 1684:{\displaystyle \theta } 1631:{\displaystyle \theta } 1409:{\displaystyle \omega } 1077:{\displaystyle \theta } 825:states. Note that many 780:Spectroscopic technique 170:electron spin resonance 1870:Paul Scherrer Institut 1842:kinetic isotope effect 1769: 1721: 1685: 1668: 1661: 1632: 1600: 1564: 1525: 1410: 1386: 1346: 1314: 1192: 1172: 1148: 1121: 1107:The average asymmetry 1098: 1078: 1055: 971: 652:High-energy muon beams 630: 603: 566: 503: 476: 435: 327: 288: 147:Muon spin spectroscopy 143: 2153:Scientific techniques 1817:. The dependence of 1770: 1722: 1686: 1662: 1633: 1617: 1601: 1565: 1526: 1411: 1387: 1347: 1315: 1193: 1173: 1149: 1122: 1099: 1079: 1056: 972: 699:University of Arizona 631: 604: 567: 509:) are formed via the 504: 477: 436: 328: 296:particle accelerators 289: 141: 2118:μSR basic literature 2079:(16): 8850–8853(R). 1862:particle accelerator 1731: 1695: 1675: 1642: 1622: 1577: 1538: 1423: 1400: 1376: 1327: 1224: 1182: 1162: 1131: 1111: 1088: 1068: 991: 900: 613: 586: 520: 486: 452: 340: 310: 258: 218:free induction decay 168:techniques, such as 51:improve this article 2085:1987PhRvB..36.8850H 2041:1986PhRvL..56.2850H 2006:1985PhT....38g..22B 1971:1976NucIM.135...39P 1154:, close to one, as 893:= 2.197034(21) μs: 800:electron scattering 229:Neutron diffraction 18:Muon spin resonance 1765: 1717: 1681: 1669: 1657: 1628: 1596: 1572:gyromagnetic ratio 1560: 1521: 1406: 1382: 1342: 1310: 1188: 1168: 1144: 1117: 1094: 1074: 1051: 967: 656:quadrupole magnets 626: 599: 562: 499: 472: 431: 429: 323: 284: 166:magnetic resonance 144: 2073:Physical Review B 2035:(26): 2850–2853. 1793:superconductivity 1654: 1385:{\displaystyle B} 1191:{\displaystyle A} 1171:{\displaystyle A} 1156:already mentioned 1120:{\displaystyle A} 1097:{\displaystyle a} 1047: 963: 952: 867:ionization energy 835:Pauli paramagnets 785:Muon implantation 139: 127: 126: 119: 101: 16:(Redirected from 2160: 2105: 2104: 2067: 2061: 2060: 2024: 2018: 2017: 2014:10.1063/1.881018 1989: 1983: 1982: 1954: 1937: 1933: 1797:material science 1774: 1772: 1771: 1766: 1746: 1745: 1726: 1724: 1723: 1718: 1710: 1709: 1690: 1688: 1687: 1682: 1666: 1664: 1663: 1658: 1656: 1655: 1647: 1637: 1635: 1634: 1629: 1605: 1603: 1602: 1597: 1589: 1588: 1569: 1567: 1566: 1561: 1556: 1555: 1530: 1528: 1527: 1522: 1487: 1486: 1477: 1457: 1456: 1435: 1434: 1415: 1413: 1412: 1407: 1391: 1389: 1388: 1383: 1351: 1349: 1348: 1343: 1319: 1317: 1316: 1311: 1288: 1287: 1278: 1258: 1257: 1236: 1235: 1197: 1195: 1194: 1189: 1177: 1175: 1174: 1169: 1158:. 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Anderson 244:Seth Neddermeyer 149:, also known as 140: 122: 115: 111: 108: 102: 100: 59: 35: 27: 21: 2168: 2167: 2163: 2162: 2161: 2159: 2158: 2157: 2138: 2137: 2114: 2109: 2108: 2069: 2068: 2064: 2026: 2025: 2021: 1991: 1990: 1986: 1956: 1955: 1951: 1946: 1941: 1940: 1934: 1930: 1925: 1898: 1860:μSR requires a 1858: 1822: 1811: 1785:magnetic fields 1781: 1737: 1729: 1728: 1701: 1693: 1692: 1673: 1672: 1640: 1639: 1620: 1619: 1580: 1575: 1574: 1547: 1536: 1535: 1478: 1448: 1426: 1421: 1420: 1398: 1397: 1374: 1373: 1325: 1324: 1279: 1249: 1227: 1222: 1221: 1212: 1180: 1179: 1160: 1159: 1134: 1129: 1128: 1109: 1108: 1086: 1085: 1066: 1065: 989: 988: 942: 929: 916: 903: 898: 897: 892: 883: 787: 782: 750: 718:Vancouver, B.C. 705:and RIKEN-RAL. 660:superconducting 642: 616: 611: 610: 589: 584: 583: 549: 536: 523: 518: 517: 489: 484: 483: 460: 455: 450: 449: 448:(MEAN lifetime 428: 427: 417: 403: 398: 386: 385: 375: 361: 356: 338: 337: 313: 308: 307: 304: 302:Muon production 274: 261: 256: 255: 210:radio-frequency 206:radio frequency 200:around a still 182: 129: 123: 112: 106: 103: 60: 58: 48: 36: 23: 22: 15: 12: 11: 5: 2166: 2164: 2156: 2155: 2150: 2140: 2139: 2136: 2135: 2130: 2125: 2120: 2113: 2112:External links 2110: 2107: 2106: 2062: 2019: 1984: 1948: 1947: 1945: 1942: 1939: 1938: 1927: 1926: 1924: 1921: 1920: 1919: 1914: 1909: 1904: 1897: 1894: 1857: 1854: 1850:semiconductors 1820: 1809: 1804:superconductor 1780: 1777: 1764: 1761: 1758: 1755: 1752: 1749: 1744: 1740: 1736: 1716: 1713: 1708: 1704: 1700: 1680: 1653: 1650: 1627: 1595: 1592: 1587: 1583: 1559: 1554: 1550: 1546: 1543: 1532: 1531: 1520: 1517: 1514: 1511: 1508: 1505: 1502: 1499: 1496: 1493: 1490: 1485: 1481: 1476: 1472: 1469: 1466: 1463: 1460: 1455: 1451: 1447: 1444: 1441: 1438: 1433: 1429: 1405: 1381: 1341: 1338: 1335: 1332: 1321: 1320: 1309: 1306: 1303: 1300: 1297: 1294: 1291: 1286: 1282: 1277: 1273: 1270: 1267: 1264: 1261: 1256: 1252: 1248: 1245: 1242: 1239: 1234: 1230: 1210: 1187: 1167: 1141: 1137: 1116: 1093: 1073: 1062: 1061: 1050: 1044: 1041: 1038: 1035: 1032: 1029: 1026: 1023: 1020: 1017: 1014: 1011: 1008: 1005: 1002: 999: 996: 978: 977: 966: 958: 951: 948: 941: 936: 932: 928: 923: 919: 915: 910: 906: 890: 882: 879: 851:semiconductors 841:by a cloud of 786: 783: 781: 778: 749: 739: 641: 638: 623: 619: 596: 592: 573: 572: 561: 556: 552: 548: 543: 539: 535: 530: 526: 511:two body decay 496: 492: 467: 463: 458: 442: 441: 424: 420: 416: 413: 410: 407: 404: 402: 399: 397: 394: 391: 388: 387: 382: 378: 374: 371: 368: 365: 362: 360: 357: 355: 352: 349: 346: 345: 320: 316: 303: 300: 281: 277: 273: 268: 264: 202:magnetic field 181: 178: 155:spin-polarized 125: 124: 39: 37: 30: 24: 14: 13: 10: 9: 6: 4: 3: 2: 2165: 2154: 2151: 2149: 2146: 2145: 2143: 2134: 2131: 2129: 2126: 2124: 2121: 2119: 2116: 2115: 2111: 2102: 2098: 2094: 2090: 2086: 2082: 2078: 2074: 2066: 2063: 2058: 2054: 2050: 2046: 2042: 2038: 2034: 2030: 2023: 2020: 2015: 2011: 2007: 2003: 1999: 1995: 1988: 1985: 1980: 1976: 1972: 1968: 1964: 1960: 1953: 1950: 1943: 1932: 1929: 1922: 1918: 1915: 1913: 1910: 1908: 1905: 1903: 1900: 1899: 1895: 1893: 1891: 1887: 1883: 1879: 1875: 1871: 1867: 1863: 1855: 1853: 1851: 1847: 1843: 1839: 1835: 1831: 1826: 1823: 1816: 1812: 1805: 1800: 1798: 1794: 1790: 1786: 1778: 1776: 1762: 1759: 1756: 1753: 1750: 1747: 1742: 1738: 1734: 1714: 1711: 1706: 1702: 1698: 1678: 1648: 1625: 1616: 1612: 1610: 1593: 1590: 1585: 1581: 1573: 1557: 1552: 1548: 1544: 1541: 1515: 1512: 1509: 1506: 1503: 1500: 1497: 1494: 1483: 1479: 1474: 1470: 1467: 1461: 1458: 1453: 1449: 1445: 1439: 1431: 1427: 1419: 1418: 1417: 1403: 1395: 1379: 1371: 1366: 1362: 1360: 1359:Zeeman energy 1356: 1339: 1336: 1333: 1330: 1304: 1301: 1298: 1295: 1284: 1280: 1275: 1271: 1268: 1262: 1259: 1254: 1250: 1246: 1240: 1232: 1228: 1220: 1219: 1218: 1216: 1209:a few times τ 1208: 1204: 1199: 1185: 1165: 1157: 1139: 1135: 1114: 1105: 1091: 1071: 1048: 1042: 1039: 1033: 1030: 1027: 1024: 1021: 1018: 1012: 1009: 1006: 1000: 994: 987: 986: 985: 983: 964: 956: 946: 939: 934: 930: 926: 921: 917: 908: 904: 896: 895: 894: 888: 887:mean lifetime 880: 878: 876: 872: 868: 864: 860: 856: 852: 848: 844: 840: 836: 832: 828: 824: 820: 816: 813:sites of the 812: 807: 805: 801: 797: 793: 784: 779: 777: 775: 770: 767:muon sources 766: 761: 758: 753: 747: 743: 740: 738: 736: 731: 727: 723: 719: 715: 711: 706: 704: 700: 696: 692: 688: 683: 681: 677: 673: 669: 664: 661: 657: 653: 649: 647: 639: 637: 621: 617: 594: 590: 581: 577: 559: 554: 550: 546: 541: 537: 528: 524: 516: 515: 514: 512: 494: 490: 465: 461: 456: 447: 422: 418: 414: 411: 408: 405: 395: 392: 389: 380: 376: 372: 369: 366: 363: 353: 350: 347: 336: 335: 334: 318: 314: 301: 299: 297: 279: 275: 271: 266: 262: 253: 249: 245: 240: 238: 234: 230: 226: 221: 219: 213: 211: 207: 203: 199: 195: 191: 186: 179: 177: 175: 171: 167: 163: 159: 156: 152: 148: 121: 118: 110: 107:December 2010 99: 96: 92: 89: 85: 82: 78: 75: 71: 68: –  67: 63: 62:Find sources: 56: 52: 46: 45: 40:This article 38: 34: 29: 28: 19: 2148:Spectroscopy 2076: 2072: 2065: 2032: 2028: 2022: 1997: 1993: 1987: 1965:(1): 39–46. 1962: 1958: 1952: 1931: 1859: 1827: 1818: 1815:Cooper pairs 1807: 1801: 1782: 1779:Applications 1670: 1608: 1533: 1367: 1363: 1354: 1322: 1214: 1206: 1200: 1106: 1063: 979: 884: 875:paramagnetic 874: 863:reduced mass 846: 826: 822: 819:paramagnetic 818: 811:interstitial 808: 788: 773: 764: 762: 756: 754: 751: 745: 741: 709: 707: 694: 690: 686: 684: 651: 650: 643: 574: 443: 305: 241: 222: 214: 183: 180:Introduction 150: 146: 145: 113: 104: 94: 87: 80: 73: 61: 49:Please help 44:verification 41: 1994:Phys. Today 859:Bohr radius 847:diamagnetic 827:diamagnetic 823:diamagnetic 252:cosmic rays 2142:Categories 1944:References 1856:Facilities 1396:frequency 1203:muon decay 843:conduction 831:paramagnet 798:of atoms, 796:ionization 757:continuous 748:muon beams 742:Continuous 198:precession 77:newspapers 2000:(7): 22. 1789:magnetism 1760:ω 1757:⁡ 1751:θ 1748:⁡ 1715:θ 1712:⁡ 1679:θ 1652:^ 1626:θ 1586:μ 1582:γ 1570:, with a 1553:μ 1549:γ 1542:ω 1513:ω 1510:⁡ 1501:α 1484:μ 1480:τ 1468:− 1462:⁡ 1432:α 1404:ω 1337:± 1331:α 1302:α 1285:μ 1281:τ 1269:− 1263:⁡ 1233:α 1140:μ 1072:θ 1043:θ 1034:θ 1031:⁡ 1013:∝ 1010:θ 1001:θ 957:μ 950:¯ 947:ν 931:ν 914:→ 905:μ 792:Coulombic 697:from the 680:RIKEN-RAL 618:μ 591:μ 555:μ 551:ν 538:μ 534:→ 525:π 491:μ 462:π 457:τ 419:π 401:→ 377:π 359:→ 315:π 272:− 2057:10033111 1896:See also 1846:radicals 1838:hydrogen 1834:isotopes 871:hydrogen 839:screened 714:band gap 663:solenoid 237:positron 2101:9942727 2081:Bibcode 2037:Bibcode 2002:Bibcode 1967:Bibcode 1907:Muonium 1836:of the 1830:muonium 1791:and/or 1594:851.616 1370:precess 877:state. 869:to the 855:muonium 769:protons 730:muonium 691:Arizona 687:surface 233:neutron 176:(NMR). 91:scholar 2099:  2055:  1882:J-PARC 1866:TRIUMF 1394:Larmor 1064:where 1046:  962:  865:, and 774:pulsed 765:pulsed 746:pulsed 735:J-PARC 722:Canada 695:et al. 676:J-PARC 672:TRIUMF 646:energy 225:X-rays 93:  86:  79:  72:  64:  1923:Notes 1323:with 446:pions 158:muons 98:JSTOR 84:books 2097:PMID 2053:PMID 1902:Muon 1207:i.e. 889:of τ 821:and 755:For 744:vs. 678:and 580:spin 246:and 192:and 185:Muon 162:spin 70:news 2089:doi 2045:doi 2010:doi 1975:doi 1963:135 1886:KEK 1813:of 1754:cos 1739:sin 1703:cos 1507:cos 1459:exp 1260:exp 1028:cos 861:), 763:At 726:LiF 689:or 668:PSI 194:ESR 190:NMR 151:μSR 53:by 2144:: 2095:. 2087:. 2077:36 2075:. 2051:. 2043:. 2033:56 2031:. 2008:. 1998:38 1996:. 1973:. 1961:. 1799:. 1205:, 802:, 720:, 682:. 674:, 670:, 513:: 276:10 263:10 2103:. 2091:: 2083:: 2059:. 2047:: 2039:: 2016:. 2012:: 2004:: 1981:. 1977:: 1969:: 1821:s 1819:n 1810:s 1808:n 1763:t 1743:2 1735:A 1707:2 1699:A 1649:x 1609:A 1591:= 1558:B 1545:= 1519:) 1516:t 1504:A 1498:+ 1495:1 1492:( 1489:) 1475:/ 1471:t 1465:( 1454:0 1450:N 1446:= 1443:) 1440:t 1437:( 1428:N 1380:B 1355:A 1340:1 1334:= 1308:) 1305:A 1299:+ 1296:1 1293:( 1290:) 1276:/ 1272:t 1266:( 1255:0 1251:N 1247:= 1244:) 1241:t 1238:( 1229:N 1215:t 1211:μ 1186:A 1166:A 1136:P 1115:A 1092:a 1049:, 1040:d 1037:) 1025:a 1022:+ 1019:1 1016:( 1007:d 1004:) 998:( 995:W 965:. 940:+ 935:e 927:+ 922:+ 918:e 909:+ 891:μ 794:( 622:+ 595:+ 560:. 547:+ 542:+ 529:+ 495:+ 466:+ 423:+ 415:+ 412:n 409:+ 406:n 396:n 393:+ 390:p 381:+ 373:+ 370:n 367:+ 364:p 354:p 351:+ 348:p 319:+ 280:7 267:4 120:) 114:( 109:) 105:( 95:· 88:· 81:· 74:· 47:. 20:)

Index

Muon spin resonance

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"Muon spin spectroscopy"
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spin-polarized
muons
spin
magnetic resonance
electron spin resonance
nuclear magnetic resonance
Muon
NMR
ESR
precession
magnetic field
radio frequency
radio-frequency
free induction decay
X-rays
Neutron diffraction
neutron
positron

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