Matches in SemOpenAlex for { <https://semopenalex.org/work/W144996327> ?p ?o ?g. }
Showing items 1 to 69 of
69
with 100 items per page.
- W144996327 startingPage "286" @default.
- W144996327 abstract "The Institute of Space and Astronautical Science, Yoshinodai, Sagamihara 229–8510, JapanAbstract. Moliere theory of multiple Coulomb scattering`has been far improved to take account ionization loss by useof Kamata-Nishimura formulation of the theory. The newformulation only introduce the scale factor to the traversedthickness for effects of ionization process, and is simply re-duced to the traditional Moliere-Bethe formulation by use`of our translation formula. Introducing Kamata-Nishimuraconstants and Kspecific to the traversed substance, wecan simplify the configuration of Moli ere theory, so that the`sequence to derive Moliere angular distributions has become`much easy. Based on the new formulation, we propose apractical and efficient method to obtain Moli `ere angular dis-tributions. The method is accurate enough to apply in MonteCarlo simulations as well as designings and analyses of ex-periments concerning charged particles.1 IntroductionReconstruction of Moli`ere’s multiple scattering theory (Moli ere,`1947, 1948; Bethe, 1953) by Kamata-Nishimura formulation(Kamata and Nishimura, 1958; Nishimura, 1967) is contin-uing. The new formulation is equivalent to the traditionalMoliere-Bethe formulation, both cutting off the higher terms`of Fourier component at the same order (Nakatsuka, 1999b).We have found various superior aspects of the new formula-tion: ionization loss is taken into account (Nakatsuka, 1999a);properties of substance are all reflected in the Kamata-Nishimuraconstants, and K(Kamata and Nishimura, 1958; Nishimura,1967; Nakatsuka, 2001a); mixed or compound substancescan easily be treated; the formulation is simple as a thor-ough extension of the Rossi-Greisen or the Fermi-Yang the-ory (Rossi and Greisen, 1941; Yang, 1951); the theory is eas-ily applicable to other problems; and so on.Although the Moliere theory has been improved by the`new formulation, a few problems still remain in actual ap-plications. In case we take account ionization loss, the scaleCorrespondence to: T. Nakatsuka (nakatuka@osu.ac.jp)factor is newly introduced (Nakatsuka, 1999a). It makesthe expansion parameter Bof the Moli`ere angular distribu-tion smaller. Namely, we should take the smaller value of Bat the times shallower thickness, compared with the fixedenergy condition. Under the moderate relativistic condition,evaluation of the scale factor requires heavy calculationsof numerical integration. In case we get the Moliere angular`distribution for charged particles propagating through mixedor compound substances, we have to carry out multiple se-quence of evaluations according to the number of mixed sub-stances to get the stochastic mean among substances (Nakat-suka, 2001a). These facts will bring serious inefficiencies toour frequent derivations of the distribution.In this paper, we derive simple methods to avoid thesecomplicated sequences, and propose a practical and efficientprocedure of getting Moliere angular distribution with ion-`ization applicable widely in simulations and analyses (Hecket al., 1998).2 Sequence to Obtain Exact Moliere Angular Distribu-`tion With IonizationFor derivations of Moli`ere angular distribution under the mod-erate relativistic condition with ionization, we found it isenough to introduce a scale factor for the traversed thick-ness (Nakatsuka, 2001b). If we assume ionization loss ofcharged particles of zwith a constant rate asE= E" @default.
- W144996327 created "2016-06-24" @default.
- W144996327 creator A5008934389 @default.
- W144996327 creator A5049439519 @default.
- W144996327 date "2001-01-01" @default.
- W144996327 modified "2023-09-24" @default.
- W144996327 title "Practical and efficient derivations of Moli ` ere angular distribution with ionization" @default.
- W144996327 hasPublicationYear "2001" @default.
- W144996327 type Work @default.
- W144996327 sameAs 144996327 @default.
- W144996327 citedByCount "0" @default.
- W144996327 crossrefType "journal-article" @default.
- W144996327 hasAuthorship W144996327A5008934389 @default.
- W144996327 hasAuthorship W144996327A5049439519 @default.
- W144996327 hasConcept C105795698 @default.
- W144996327 hasConcept C111472728 @default.
- W144996327 hasConcept C121332964 @default.
- W144996327 hasConcept C138885662 @default.
- W144996327 hasConcept C145148216 @default.
- W144996327 hasConcept C147120987 @default.
- W144996327 hasConcept C191486275 @default.
- W144996327 hasConcept C19499675 @default.
- W144996327 hasConcept C198291218 @default.
- W144996327 hasConcept C2780586882 @default.
- W144996327 hasConcept C33923547 @default.
- W144996327 hasConcept C62520636 @default.
- W144996327 hasConcept C9342510 @default.
- W144996327 hasConceptScore W144996327C105795698 @default.
- W144996327 hasConceptScore W144996327C111472728 @default.
- W144996327 hasConceptScore W144996327C121332964 @default.
- W144996327 hasConceptScore W144996327C138885662 @default.
- W144996327 hasConceptScore W144996327C145148216 @default.
- W144996327 hasConceptScore W144996327C147120987 @default.
- W144996327 hasConceptScore W144996327C191486275 @default.
- W144996327 hasConceptScore W144996327C19499675 @default.
- W144996327 hasConceptScore W144996327C198291218 @default.
- W144996327 hasConceptScore W144996327C2780586882 @default.
- W144996327 hasConceptScore W144996327C33923547 @default.
- W144996327 hasConceptScore W144996327C62520636 @default.
- W144996327 hasConceptScore W144996327C9342510 @default.
- W144996327 hasLocation W1449963271 @default.
- W144996327 hasOpenAccess W144996327 @default.
- W144996327 hasPrimaryLocation W1449963271 @default.
- W144996327 hasRelatedWork W1536836988 @default.
- W144996327 hasRelatedWork W1964984182 @default.
- W144996327 hasRelatedWork W1975597129 @default.
- W144996327 hasRelatedWork W1984536682 @default.
- W144996327 hasRelatedWork W1987029007 @default.
- W144996327 hasRelatedWork W1990927250 @default.
- W144996327 hasRelatedWork W1993756833 @default.
- W144996327 hasRelatedWork W2013927962 @default.
- W144996327 hasRelatedWork W2022937806 @default.
- W144996327 hasRelatedWork W2024649460 @default.
- W144996327 hasRelatedWork W2025204006 @default.
- W144996327 hasRelatedWork W2037510502 @default.
- W144996327 hasRelatedWork W2041259029 @default.
- W144996327 hasRelatedWork W2067514149 @default.
- W144996327 hasRelatedWork W2069671806 @default.
- W144996327 hasRelatedWork W2091536812 @default.
- W144996327 hasRelatedWork W2097690519 @default.
- W144996327 hasRelatedWork W2144625094 @default.
- W144996327 hasRelatedWork W2599498397 @default.
- W144996327 hasRelatedWork W55190534 @default.
- W144996327 hasVolume "1" @default.
- W144996327 isParatext "false" @default.
- W144996327 isRetracted "false" @default.
- W144996327 magId "144996327" @default.
- W144996327 workType "article" @default.