Interactions of High Energy Particles with Nuclei |
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Page 15
This formula was used successfully to : ( i ) reproduce the proton charge form factors from elastic scattering hadron - hadron cross sections . ( ii ) predict diffractive structure ( e.g. , diffractive minima ) of the high energy hadron ...
This formula was used successfully to : ( i ) reproduce the proton charge form factors from elastic scattering hadron - hadron cross sections . ( ii ) predict diffractive structure ( e.g. , diffractive minima ) of the high energy hadron ...
Page 22
These two factors make Coulomb corrections insignificant in do DT / do . How important are the details of the target nucleus wave function ? Not very important . The most important are general characteristics : density distributions ...
These two factors make Coulomb corrections insignificant in do DT / do . How important are the details of the target nucleus wave function ? Not very important . The most important are general characteristics : density distributions ...
Page 23
( i ) the shapes of target nuclei are the most important factors determining the cross sections ( ii ) the internal correlations of nucleons in the nucleus are unimportant for dose / dî or do 。 dî . They are of some importance for do ...
( i ) the shapes of target nuclei are the most important factors determining the cross sections ( ii ) the internal correlations of nucleons in the nucleus are unimportant for dose / dî or do 。 dî . They are of some importance for do ...
Page 24
Hence if we can factor out the c.m. wave function from the product = II ; ; ( r ; ) we can stick to calculating M with Yo but we have to multiply it by a correction factor : ( R ( r ) | exp ( i △ · r ) | R ( r ) ) −1 .
Hence if we can factor out the c.m. wave function from the product = II ; ; ( r ; ) we can stick to calculating M with Yo but we have to multiply it by a correction factor : ( R ( r ) | exp ( i △ · r ) | R ( r ) ) −1 .
Page 25
( iii ) The importance of the c.m. motion correction can be seen from the factor exp ( R242 / 4A ) . For small A ( say A = 2 , 3 or 4 ) it can be a correction of as much as 2 orders of magnitude for A2 0.3 GeV2 .
( iii ) The importance of the c.m. motion correction can be seen from the factor exp ( R242 / 4A ) . For small A ( say A = 2 , 3 or 4 ) it can be a correction of as much as 2 orders of magnitude for A2 0.3 GeV2 .
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