Kaon photoproduction from threshold up to 5.5 GeV

V. Veryanta, T. Mart

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

Abstract

By using two different methods we have combined the recent isobar and the Regge models to explain kaon photoproduction process from its threshold up to W = 5.5 GeV. To this end, a transition region at energies between those commonly used by the conventional isobar and the Regge models, i.e., 2.5 ≤ W ≤ 3.0 GeV, is proposed. For the isobar model we use the previous result of Clymton et al. [1]. This model fits experimental data from threshold up to W = 2.8 GeV. In the high energy region the Regge model is utilized, where experimental data up to W = 5.5 GeV can be nicely reproduced. The result is compared with those of previous studies.

Original languageEnglish
Title of host publicationProceedings of the 4th International Symposium on Current Progress in Mathematics and Sciences, ISCPMS 2018
EditorsTerry Mart, Djoko Triyono, Ivandini T. Anggraningrum
PublisherAmerican Institute of Physics Inc.
ISBN (Electronic)9780735419155
DOIs
Publication statusPublished - 4 Nov 2019
Event4th International Symposium on Current Progress in Mathematics and Sciences 2018, ISCPMS 2018 - Depok, Indonesia
Duration: 30 Oct 201831 Oct 2018

Publication series

NameAIP Conference Proceedings
Volume2168
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Conference

Conference4th International Symposium on Current Progress in Mathematics and Sciences 2018, ISCPMS 2018
CountryIndonesia
CityDepok
Period30/10/1831/10/18

Keywords

  • Isobar model
  • kaon photoproduction
  • Regge model

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