deduce the general relatio n7, Pr .The shape of the cross-section - energy graph at resonance is given by the Breit-Wigne rformula6, = 1/((E-Fr)1+ (7/ 2 )2 ) ,where n is the energy at renorace, and 8 is the energy at which the width of th ecurve, V, has beer measured . The spin of a resonance is measured by the carefu lobservation of the angular distribution of its d e cay products, and, in the case of th eit is 3/2 . We know that the orbital angular momentum, 1, of the pion and nucleon i nthe A. particle is 1 . Thus we know that its parity i sP(11) P(N) (-1)~ 43 -The A. particle was the first resonance discovered in a formation experiment ,using cross-section - energy graphs . However, its statue as a resonance was no tconfirmed until it was also detected in a production experiment, where it acted as aparticle, rather than a favourite interaction energy . It was not, in fact, the firs tresonance to be revealed in a production experiment, but, for the sake of homogeneitywe will discuss its production experiment . We consider the reactio nPP — anA'" --a. nprt '.If there were no intermediate stage, then the neutron produced ahould have a complet erange of different energies . However, when protons of 2 .8 GeV were used, only a verysmall spread of value ., corre sp onding to the macs uncertainty of the 0 , peaked aroun d1 .62 GeV was found . It can be shown that this corresponds to the neutrons recoilin gfrom a single particle of mass 12.36 MeV, which is an acceptable experimental error .The first particle to be discovered in a resonance production experiment was th eY* particle . In late 1960, Alston, Alvarez, 3berhard, Good, Graziano, Ticho, and Wojkick iset out, using the accelerator at the Lawrence radiation Laboratory, to study th eprocessK 7+ p -4/47+7 7to see if any resonances could be produced . They allowed a magnetically-separate dkaon beam to enter a liquid hydrogen bubble chamber, and steadily increased its energy .Every 20 - 100 MeV, batches of photographs were taken of the reactions in the bubbl echamber . By 1960, there was good evidence from decay product momentum analysis, t oshow that the processK-+ p —~ - +1T -+ —~ +-++r 4. -was occurring . The mass of the Y " resonance was found to be about 1385 MeV and it sbandwidth to be about 60 MeV .We will not, at this point, follow the historical development of resonance<strong>physics</strong>, but we will consider our current knowledge of the baryon resonances . No tonly have a considerable number of S• 0 and S= -1 baryon resonances been found, bu talso a few S .-2 ones . An example of one of these is the particle with a mass o f1530 MeV discovered by Bertanza et al . in 1962 . They showed that the proces sK +p--,=* K --s1T Ktook place by measuring the recoil energies of the K particle, and demonstrating tha tthey were consistent with recoil from one rather than tKo other <strong>particles</strong> . Theangular distribution of the decay products favoured a J of 3/ 2 + or 5/2 , but the
A large number of n -N resonances have been discovered to date, and it has beenfound that these fall into two distinct group s . Then we plot the total cross-section sof the n'p and T' p systems, we find that tine ratio of peak heights at resonance i seither 0 :1 or 3 :1 . Thus we can produce resonances with i-spins of either + or 3/ 2in 7f -N reactions . It is the convention to term those with 1-s-+ N4 resonances, andthose with I" 3/2 L. resonances . :f N resonances also fall into two groups, one wit hI ). and the other with Ia.- O . These are conventionally represented as and 'o, o rg and t respectively. Similarly resonances with S e -2 are represented as Y„ or .It is common practice to put the mass as it was first measured in brackets after th ename of a resonance . Hence one eight write N(1750), although this resonance actuall yhas a mass of about 1785 NeV according to modern, measurements . There is some movemen ttowards a completely new nomenclature for resonances . It makes use of the essentia lquantum numbers conected with a resonance, and the letters denoting orbital moment aborrowed from atomic spectroscopy . A given resonance would be writtenISOSPIN(ORBITAL, TiON.r1^lUT ;) TOTAL ANGULAR KONNTDiiThe atomic spectroscopy letters are, in order, starting from 1= 0 : S, P, D, F, G, . . .Thus, using this nomenclature, the A(1238) particle would be represented : P .It is unlikely that there exist any baryon resonances other than those type smentioned above . The easiest type of resonance to study is obviously the N-N resonance ,but it is almost certain that no resonances of this type exist . There are also th eN-N resonances, but convincing proof of these is still lacking . It is also unlikelythat any <strong>particles</strong> with isospins higher than 3/2 exist, although it is possible tha tthere exist two strange resonances : 4(1451) and D(2520) with I= 2, though these hav enot yet Been confirmed .In 1957 and 1959 respectively Nambu and Chew showed that the vector part of th enucleon's internal electromagnetic field observed by Hofstader could be explained i nterms of boson resonances . In 1960 Frazer and =Lilco applied dispersion-relation method sto Hofstader's findings and again predicted boson resonances . Accordingly, in 1961 ,Hofstader et al . found a di-pion resonance at about 750 keV which they named the eparticle . It was produced in the reactio nTf e'+P-->n i 1T+'ntf.P •However, the interesting thing about the particle is that its decay :appears to violate the law of the conservation of mass-energy, since the total energyof its decay products is rarely above 350 NeV . According to a new theory by Gestalt ,it becomes a new type of matter which absorbs much of its energy before decay . However ,the P particle becomes more enigmatic as time goes on : in 1968 the reactione-e+ ewas observed, indicating that the fparticle was similar to the photon in some way .Regge's theory, which we will discuss later in this chapter, suggests that the e i san excited state of the vacuum, which would poosibly account for some of its oddcharacteristics .Late in 1959, Chew suggested that the scalar part of charge lately observed b yHofstader in the nucleon could be explained in terms of a tri-pion resonance . In 1961Naglic, Alvarea, Rosenfeld, and Stevenson studied the annihilation of antiprotons byprotons in the 72" bubble chamber at the Lawrence Radiation Laboratory, according tothe_reactio np +P -~ n*+ n'+lt ++'n' + Tt ° .
- Page 1 and 2: ~~N ."$ II itOL'it At .AQo
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- Page 49 and 50: where s and t are the riandelstam v
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- Page 55 and 56: is 1 .3 x 10 s . The leaders o; is,
- Page 57 and 58: called 'parallelogram rule' of Matt
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CHAPTER NINE: THE ACCELERATION OF P
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1931 Sloan and Lawrence built a thi
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faster than light . instead, the ph
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employed for each function . In act
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and again by Budker and Veksler in
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BIBLIOGRAPHY .General works :The Ph
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Scalar : .esons may ihplain by the
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Name S J I I s U P GY ND ND 1 ND ND
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p5,55' 77 6570p 070601,.635 67.7355
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A .3 Quark combinations to fora sta
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s+ki # 13 .41M.V I9mo. dxry nvla)33
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k.1515e.pr rim
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° Prix.-.,a..u(14751 o IMfon.ly ca
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A .5 Conservation and invariance la
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F_AG Fixed field alternating gradie
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S Scalar gamma matrix product .S En
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Elastic cross—section .Inelastic
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C .3 Compound SI units used in this
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w oE >< k)- c; ev--o ;,o»,--.@r«-
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APPENDIX F : PHYSICAL CONSTANTS .(F