f+K +84Ptakes place, so that S=1 for the K , and hence I . -) This implies that the K+ is onemember of an isotopic doublet, whose other member is neutrally charged . We are forcedto conclude that this other member is the K° . But that, then, is the status of the K °?The only reasonable conclusion is that this has Se -1, and that it is the antiparticl eof the K } . But it too mist form a doublet, the other member of which must be the antiparticleof the K ' , the 7° particle . Thus we see that, unlike, for example, than. .. ,the K° is not its own antiparticle . As we shall see in chapter 7, this fact ha sprofound results on particle symmetries .Let us now consider the quantum number of parity . We first define an operator, P ,such that?1 .4f(x,y,z) _ y(-x,-y,-z) ,which corresponds to a rotation through 180 about the x-axis, followed by a reflectionin the plane x= O . From our studies of angular momentum, we know that all wave function sare invariant under the transformation of rotation, and so the only real significanc eof the operator P is in its space reflection component . It is a fact of wave mechanic sthat for all physically meaningful waves 'f , l(r ~' must be invariant under the Por fl operation . Hut, taking a snuare root, we find thatP'1(f(x,y,z) _ +1 14r ( x ,y, z ) or -l`}r(x,y,z) •In the first case we say that the wave function Nr has even parity, and in the second ,that it has odd parity . Hence, by knowing the wave function of a given particle, w emay assign to that particle an intrinsic parity, P, which can take the values of eithe rt 1 or -1 . There can be no absolute measure of parity, and so we measure all paritie srelative to that of the proton, which we cal lIn particle <strong>physics</strong>, however, we are often concerned with systems containing mor ethan one particle, and thus we need to know what the parity of a system of two <strong>particles</strong> ,A and B, which are rotating around each other with a an angular momentum of L ;'(, is .We know that the wave function of the complete system i slir ( A )• ( B )•1f ( L ) ,and that thereforeP(A+B) e P(A) .P(B) .P(L) .We find that P(L) is given by the formul aP(1, ) ' (- I ) L ,by studying the spherical harmonics . Let us now attempt to deduce theoretically th eintrinsic parities of the charged pions . We know that the reaction-,f - d-wn n ,where d is the deuteron, takes place . It has been shown that nearly all-n - <strong>particles</strong>are captured and cascade into the lowest energy level orbit in about . 1C" °s . Thus ,since the angular momentum in this orbit is zero, the parity of the d-r system wil lbe the same as the parity of the ir - particle on its own . Now let us consider the totalparity of the n-n system . The bxclusion Principle (see chapter 3) forbids L= 0 fo rthis system, and therefore the lowest possible value is L= 1 . Since the neutron ha seven parity, we see that the n-n system must therfore have odd parity, so that th eparity of the charged pions is odd, because parity is conserved in a strong interactio nof this type .The assumption that parity is conserved in strong interactions brings about som einteresting comments . It implies that the laws of nature are the same on both side sof a mirror . In a comparatively macrocosmic sense, this is not true, since comple xorganic molecules are more often right- than left-handed . However, if we have a beamof, for example, polarised - ° <strong>particles</strong>, then we find that the direction in r ;hich
lambda <strong>particles</strong> are preferentially emitted by - e <strong>particles</strong> travelling in the +- 7direction is precisely the same as the image of that of emitted by particle stravelling in the -7 direction under reflection in the 7= 0 plane . Thu :, in this decay ,total parity is conserved, or this decay is invariant under the space reflectio noperator P . We might note that in some books intrinsic parity is denoted bye and no tP .There is not only parity in real, but also in charge or i-space . There exists anoperator C which reverses the charge of any particle, so that, for instanc eC( rr) = (-rr+) ,and <strong>particles</strong> are transformed into their anti<strong>particles</strong> . For <strong>particles</strong> where B . S = 0 ,the effect of the operator C is purely to reverse their charges . There is anothe roperator, R, which inverts the third component of the i-spin of a given particle, o rrotates its charge vector in i-space through 1800 about the y- or It -axis . Thus R i sdefinedR -- e Iulz ,working in radians . We define another operator, G, a sG = CR .The net effect of the G operator is to reflect a given particle ' s charge vector inthe plane I3 = 0, and then to rotate it through -cr ` about the Ia-axis, which is thesame as the P operator's effect in real space . We find thatG (TTO) _ -(Tr°) ,and so we say that the G-parity, G, of the pion is -1 or odd . G is sometimes defined a sG e C(-1)=where I is the isospin of the particle in question . It is an experimental fact thatG-parity is conserved in strong interactions, so that, in a reaction where only pion sor other <strong>particles</strong> for which B e S- 0 and G = -1 are involved, the difference betweenthe initial and final number of pions in the eystem must be even . G-parity is usefulin theoretical work on w and q resonances, though of no practical value, since target sof pure pions can not be obtained with present technology .One type of radioactive decay, that in which electrons are released, is known a sbeta decay . The free neutron is an example of a <strong>subatomic</strong> particle which decays i nthis way . L'ver since the discovery of this type of decay, physicists could not understandwhere the extra decay energy went to . At one point, the law of the conservatio nof energy was actually thrown into doubt . In, for example, the decay of the neutron ,780 keV seemed to be dissappearing . But, in 1931, W.Pauli proposed a hypothesis whic hwould account for this . He postulated that there exists another particle, which h ecalled the neutrino or neutretto, which takes away this extra energy . By 1935, Pauliand Fermi had worked out all the quantum numbers of this particle, and had found thatit had practically no detectable properties, and, moreover, it was hardly produce din any reactions except for the rare beta decay . The first thing to do was to measurethe angles and momenta at which the proton and electron left the scene of the decayn ---N p + e - . . . .If no neutrinowere produced, then these two <strong>particles</strong> should be coplanar and mono -energetic . However, this was found not to be the case, and so it was assumed thatthe neutrino existed .But the neutrino is the most unreactive of all <strong>subatomic</strong> <strong>particles</strong> known at present ,and a neutrino is calculated to interact with only 1 out of 10' 3 <strong>particles</strong> which it scomes near to . Thus the detection of the neutrino was a difficult problem, since i tdid not interact with any sort of detector, and it did not, so far as anyone knew,
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on their spins . We find that if we
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device : scalers, which record the
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In appearance, semiconductor partic
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Usually, photons passing through a
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during this short time, worthwhile
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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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A .3 Quark combinations to fora sta
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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