Your browser doesn't support javascript.
loading
Evidence of a Hardening in the Cosmic Ray Proton Spectrum at around 166 TeV Observed by the GRAPES-3 Experiment.
Varsi, F; Ahmad, S; Chakraborty, M; Chandra, A; Dugad, S R; Goswami, U D; Gupta, S K; Hariharan, B; Hayashi, Y; Jagadeesan, P; Jain, A; Jain, P; Kawakami, S; Kojima, H; Lipari, P; Mahapatra, S; Mohanty, P K; Moharana, R; Muraki, Y; Nayak, P K; Nonaka, T; Oshima, A; Pant, B P; Pattanaik, D; Paul, S; Pradhan, G S; Rameez, M; Ramesh, K; Reddy, L V; Saha, S; Sahoo, R; Scaria, R; Shibata, S; Zuberi, M.
Afiliação
  • Varsi F; Indian Institute of Technology Kanpur, Kanpur 208016, India.
  • Ahmad S; Aligarh Muslim University, Aligarh 202002, India.
  • Chakraborty M; Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400005, India.
  • Chandra A; Aligarh Muslim University, Aligarh 202002, India.
  • Dugad SR; Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400005, India.
  • Goswami UD; Dibrugarh University, Dibrugarh 786004, India.
  • Gupta SK; Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400005, India.
  • Hariharan B; Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400005, India.
  • Hayashi Y; Graduate School of Science, Osaka Metropolitan University, Sugimoto, Sumiyoshi, Osaka 558-8585, Japan.
  • Jagadeesan P; Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400005, India.
  • Jain A; Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400005, India.
  • Jain P; Indian Institute of Technology Kanpur, Kanpur 208016, India.
  • Kawakami S; Graduate School of Science, Osaka Metropolitan University, Sugimoto, Sumiyoshi, Osaka 558-8585, Japan.
  • Kojima H; College of Engineering, Chubu University, Kasugai, Aichi 487-8501, Japan.
  • Lipari P; INFN, Sezione Roma "Sapienza", Piazzale Aldo Moro 2, 00185 Roma, Italy.
  • Mahapatra S; Utkal University, Bhubaneswar 751004, India.
  • Mohanty PK; Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400005, India.
  • Moharana R; Indian Institute of Technology Jodhpur, Jodhpur 342037, India.
  • Muraki Y; Institute for Space-Earth Environmental Research, Nagoya University, Nagoya 464-8601, Japan.
  • Nayak PK; Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400005, India.
  • Nonaka T; Institute for Cosmic Ray Research, Tokyo University, Kashiwa, Chiba 277-8582, Japan.
  • Oshima A; College of Engineering, Chubu University, Kasugai, Aichi 487-8501, Japan.
  • Pant BP; Indian Institute of Technology Jodhpur, Jodhpur 342037, India.
  • Pattanaik D; Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400005, India.
  • Paul S; Utkal University, Bhubaneswar 751004, India.
  • Pradhan GS; Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400005, India.
  • Rameez M; Indian Institute of Technology Indore, Indore 453552, India.
  • Ramesh K; Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400005, India.
  • Reddy LV; Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400005, India.
  • Saha S; Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400005, India.
  • Sahoo R; Indian Institute of Technology Kanpur, Kanpur 208016, India.
  • Scaria R; Indian Institute of Technology Indore, Indore 453552, India.
  • Shibata S; Indian Institute of Technology Indore, Indore 453552, India.
  • Zuberi M; College of Engineering, Chubu University, Kasugai, Aichi 487-8501, Japan.
Phys Rev Lett ; 132(5): 051002, 2024 Feb 02.
Article em En | MEDLINE | ID: mdl-38364164
ABSTRACT
We present the measurement of the cosmic ray proton spectrum from 50 TeV to 1.3 PeV using 7.81×10^{6} extensive air shower events recorded by the ground-based GRAPES-3 experiment between 1 January 2014 and 26 October 2015 with a live time of 460 day. Our measurements provide an overlap with direct observations by satellite and balloon-based experiments. The electromagnetic and muon components in the shower were measured by a dense array of plastic scintillator detectors and a tracking muon telescope, respectively. The relative composition of the proton primary from the air shower data containing all primary particles was extracted using the multiplicity distribution of muons which is a sensitive observable for mass composition. The observed proton spectrum suggests a spectral hardening at ∼166 TeV and disfavors a single power law description of the spectrum up to the Knee energy (∼3 PeV).

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2024 Tipo de documento: Article

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2024 Tipo de documento: Article