Interactions of High Energy Particles with NucleiNational Bureau of Standards, 1975 - 69 pages |
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Results 6-10 of 12
Page 42
... possible hadronic states which can be coupled to a photon . We can also write , as before , the expansion of a hadronic state n ( n ) ) - { 10 , - ( kn ) | k , 0 ) + } . 0 + ... } . | ¥ ( n ) ) = Z { | 0 , n ) – ≥ k γ H ' E - En Note ...
... possible hadronic states which can be coupled to a photon . We can also write , as before , the expansion of a hadronic state n ( n ) ) - { 10 , - ( kn ) | k , 0 ) + } . 0 + ... } . | ¥ ( n ) ) = Z { | 0 , n ) – ≥ k γ H ' E - En Note ...
Page 43
... possible interactions of the same order of magnitude ( ~ e ) whose role one should discuss : for instance all kinds of such Compton - like processes which do not belong to the VMD model , where the photon is absorbed by the target ( or ...
... possible interactions of the same order of magnitude ( ~ e ) whose role one should discuss : for instance all kinds of such Compton - like processes which do not belong to the VMD model , where the photon is absorbed by the target ( or ...
Page 44
... possible test is , e.g. , the equation σT ( Y , hadron ) = π k , Σ V Απα Y12 Im M ( V → V ) . Assuming M ( V → V ) purely imaginary ( in the high energy limit ) this becomes πα στ ( γ , hadron ) = Σ σVN . V Yv2 ( 4.9 ) First , let us ...
... possible test is , e.g. , the equation σT ( Y , hadron ) = π k , Σ V Απα Y12 Im M ( V → V ) . Assuming M ( V → V ) purely imaginary ( in the high energy limit ) this becomes πα στ ( γ , hadron ) = Σ σVN . V Yv2 ( 4.9 ) First , let us ...
Page 50
... possible because the vector mesons interact with nucleons before they decay . The differential photoproduction cross sections look very much like elastic hadron - nucleus cross sections . They exhibit a steep slope at small q2 and then ...
... possible because the vector mesons interact with nucleons before they decay . The differential photoproduction cross sections look very much like elastic hadron - nucleus cross sections . They exhibit a steep slope at small q2 and then ...
Page 65
... possible " histories " - ( mer ) | 1 ) ( 1 − ( 1 | г | 1 ) ) . ... ( 1- ( 11 ) ) . A " history " is a sequence of intermediate states | mc ) , . . . | m " ) , | m ′ ) , | m ) . One can perform the sum S by diagonalizing ( m 65.
... possible " histories " - ( mer ) | 1 ) ( 1 − ( 1 | г | 1 ) ) . ... ( 1- ( 11 ) ) . A " history " is a sequence of intermediate states | mc ) , . . . | m " ) , | m ′ ) , | m ) . One can perform the sum S by diagonalizing ( m 65.
Common terms and phrases
absorption additivity of phase anomalous magnetic moment ú approximately assume attenuation b+½s beam Bureau of Standards coherent diffractive production collision Compton scattering compute Coulomb interactions Czyż d³r db exp i▲·b deuteron diagonalization diffractive production processes diffractive scattering discussed double scattering elastic scattering amplitude electromagnetic equation example excited experiments factor Feynman diagrams formula four-momentum Glauber model hadrons Hence high energy limit incident particle incident wave inelastic shadowing Interactions of High invariant mass K mesons multiple scattering National Bureau neutrino neutrons ññ Note nuclear matter nuclear targets nuclei nucleon obtained optical theorem parameters phase shifts photon photoproduction of vector physical pion production amplitude profiles quantum numbers regeneration Řº shadowing effects single scattering spin strongly interacting target nucleus total cross section vector meson VMD model wave function γν Σ Σ