Sebastián Mendizabal , Nicolás Viaux M. , Sebastián Tapia , Raquel Pezoa R. , Barbara Gutiérrez , Constanza Valdivieso
{"title":"重新审视电磁风淋室的纵向发展:对具有天顶角依赖性的格雷森形式论的分析改进","authors":"Sebastián Mendizabal , Nicolás Viaux M. , Sebastián Tapia , Raquel Pezoa R. , Barbara Gutiérrez , Constanza Valdivieso","doi":"10.1016/j.astropartphys.2025.103172","DOIUrl":null,"url":null,"abstract":"<div><div>We present a new analytical approach to the longitudinal development of electromagnetic air showers, offering improvements to the classical Greisen formalism. We introduce a modified profile for the slope function <span><math><mrow><msub><mrow><mi>λ</mi></mrow><mrow><mn>1</mn></mrow></msub><mrow><mo>(</mo><mi>s</mi><mo>)</mo></mrow></mrow></math></span> that achieves an agreement less than 0.75% with the original <span><math><msub><mrow><mi>λ</mi></mrow><mrow><mn>1</mn></mrow></msub></math></span> for shower age parameter <span><math><mi>s</mi></math></span> between <span><math><mrow><mn>0</mn><mo>.</mo><mn>3</mn><mo><</mo><mi>s</mi><mo><</mo><mn>1</mn><mo>.</mo><mn>4</mn></mrow></math></span>, where <span><math><mi>s</mi></math></span> represents the stage of shower development. Our new formalism provides an improved representation of shower evolution, particularly near and beyond the shower maximum. In addition, we propose a modified Greisen profile. Our implementation includes the zenith angle dependence on the number of particles at the detector level at high altitudes, making it particularly useful for high-altitude observatories. This expression is suitable for implementing air shower simulation tool fitting procedures over a wide range of energies and geometries. Our analysis shows that the modified Greisen profile provides better agreement with the expected evolution of particle numbers compared to the Greisen formulation when we compare it with CORSIKA simulations.</div></div>","PeriodicalId":55439,"journal":{"name":"Astroparticle Physics","volume":"175 ","pages":"Article 103172"},"PeriodicalIF":2.9000,"publicationDate":"2025-09-12","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Revisiting the longitudinal development of electromagnetic air showers: Analytical improvements to the Greisen formalism with zenith angle dependence\",\"authors\":\"Sebastián Mendizabal , Nicolás Viaux M. , Sebastián Tapia , Raquel Pezoa R. , Barbara Gutiérrez , Constanza Valdivieso\",\"doi\":\"10.1016/j.astropartphys.2025.103172\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><div>We present a new analytical approach to the longitudinal development of electromagnetic air showers, offering improvements to the classical Greisen formalism. We introduce a modified profile for the slope function <span><math><mrow><msub><mrow><mi>λ</mi></mrow><mrow><mn>1</mn></mrow></msub><mrow><mo>(</mo><mi>s</mi><mo>)</mo></mrow></mrow></math></span> that achieves an agreement less than 0.75% with the original <span><math><msub><mrow><mi>λ</mi></mrow><mrow><mn>1</mn></mrow></msub></math></span> for shower age parameter <span><math><mi>s</mi></math></span> between <span><math><mrow><mn>0</mn><mo>.</mo><mn>3</mn><mo><</mo><mi>s</mi><mo><</mo><mn>1</mn><mo>.</mo><mn>4</mn></mrow></math></span>, where <span><math><mi>s</mi></math></span> represents the stage of shower development. Our new formalism provides an improved representation of shower evolution, particularly near and beyond the shower maximum. In addition, we propose a modified Greisen profile. Our implementation includes the zenith angle dependence on the number of particles at the detector level at high altitudes, making it particularly useful for high-altitude observatories. This expression is suitable for implementing air shower simulation tool fitting procedures over a wide range of energies and geometries. Our analysis shows that the modified Greisen profile provides better agreement with the expected evolution of particle numbers compared to the Greisen formulation when we compare it with CORSIKA simulations.</div></div>\",\"PeriodicalId\":55439,\"journal\":{\"name\":\"Astroparticle Physics\",\"volume\":\"175 \",\"pages\":\"Article 103172\"},\"PeriodicalIF\":2.9000,\"publicationDate\":\"2025-09-12\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Astroparticle Physics\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/S0927650525000957\",\"RegionNum\":3,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astroparticle Physics","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0927650525000957","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
Revisiting the longitudinal development of electromagnetic air showers: Analytical improvements to the Greisen formalism with zenith angle dependence
We present a new analytical approach to the longitudinal development of electromagnetic air showers, offering improvements to the classical Greisen formalism. We introduce a modified profile for the slope function that achieves an agreement less than 0.75% with the original for shower age parameter between , where represents the stage of shower development. Our new formalism provides an improved representation of shower evolution, particularly near and beyond the shower maximum. In addition, we propose a modified Greisen profile. Our implementation includes the zenith angle dependence on the number of particles at the detector level at high altitudes, making it particularly useful for high-altitude observatories. This expression is suitable for implementing air shower simulation tool fitting procedures over a wide range of energies and geometries. Our analysis shows that the modified Greisen profile provides better agreement with the expected evolution of particle numbers compared to the Greisen formulation when we compare it with CORSIKA simulations.
期刊介绍:
Astroparticle Physics publishes experimental and theoretical research papers in the interacting fields of Cosmic Ray Physics, Astronomy and Astrophysics, Cosmology and Particle Physics focusing on new developments in the following areas: High-energy cosmic-ray physics and astrophysics; Particle cosmology; Particle astrophysics; Related astrophysics: supernova, AGN, cosmic abundances, dark matter etc.; Gravitational waves; High-energy, VHE and UHE gamma-ray astronomy; High- and low-energy neutrino astronomy; Instrumentation and detector developments related to the above-mentioned fields.