Epifanio Ponce | Cosmic Ray Detection | Excellence in Innovation Award

Published on by Physicist Particle

Excellence in Innovation Award

Epifanio Ponce
Researcher Epifanio Ponce
Affiliation Benemérita Universidad Autónoma de Puebla
Country Mexico
Scopus ID 16029702500
Documents 42
Citations 1,181
h-index 11
Subject Area Cosmic Ray Detection
Event Global Particle Physics Excellence Awards

The research profile presented here is framed around cosmic ray detection, an area of particle and astroparticle physics concerned with the observation, characterization, and interpretation of high-energy particles originating from cosmic sources and interacting with Earth’s atmosphere and detection systems. Modern cosmic-ray research combines detector technologies, particle-physics methods, atmospheric observations, statistical analysis, and computational techniques to investigate the properties and origins of energetic particles. [2]

Abstract

This article presents an academic recognition profile for Epifanio Ponce, affiliated with Benemérita Universidad Autónoma de Puebla, Mexico, in connection with the Excellence in Innovation Award associated with the Global Particle Physics Excellence Awards. The profile identifies Cosmic Ray Detection as the principal subject area and summarizes the supplied bibliometric indicators of 42 documents, 1,181 citations, and an h-index of 11. Citation and publication indicators can provide useful quantitative context for assessing the visibility of scholarly research, while the interpretation of research contributions requires consideration of the scientific context, publication record, collaboration patterns, and substantive contribution of the work. [1]

Keywords

  • Cosmic Ray Detection
  • Cosmic Rays
  • Particle Physics
  • Astroparticle Physics
  • High-Energy Particles
  • Particle Detectors
  • Experimental Physics
  • Scientific Innovation

Introduction

Cosmic rays are energetic particles that reach Earth from space and provide an important natural source of information for particle physics and astrophysics. Their study contributes to investigations of particle interactions at energies that can extend beyond the direct reach of some terrestrial accelerator experiments. Cosmic-ray observatories use complementary detector systems to measure particle showers and related physical quantities, supporting studies of particle composition, energy spectra, arrival directions, and interactions in the atmosphere. [2]

Research Profile

The supplied research profile associates Epifanio Ponce with Benemérita Universidad Autónoma de Puebla and identifies Cosmic Ray Detection as the principal subject area. The Scopus author identifier supplied for the profile is 16029702500. The stated record comprises 42 documents, 1,181 citations, and an h-index of 11. These figures should be understood as bibliometric observations associated with the supplied author record and may change as indexing databases are updated. [1]

Research Contributions

Research in cosmic ray detection depends on the reliable acquisition and interpretation of signals generated by energetic particles and their secondary interactions. Relevant scientific contributions may involve detector development, event reconstruction, particle identification, shower characterization, calibration procedures, data analysis, or the interpretation of cosmic-ray observations within broader particle-physics models. [2].

Publications

The supplied Scopus record reports 42 documents associated with the researcher. Scopus author profiles are designed to aggregate indexed scholarly documents and citation information under an author identifier, although author disambiguation and database coverage can affect the completeness of an individual profile. [1]

Research Impact

The supplied bibliometric indicators show 1,181 citations across 42 indexed documents and an h-index of 11. An h-index of 11 indicates that, within the cited database record, at least 11 publications have each received at least 11 citations. Citation counts and h-index values are database-dependent measures and can vary according to indexing coverage, author disambiguation, document type, and the date on which the profile is accessed. [3]

Award Suitability

The Excellence in Innovation Award profile places the researcher within the scientific domain of Cosmic Ray Detection and the broader field of particle physics. The supplied publication and citation indicators provide documented quantitative information that can be considered alongside the substantive content of the research record. [3]

Conclusion

Epifanio Ponce is presented in this academic recognition profile as a researcher affiliated with Benemérita Universidad Autónoma de Puebla, Mexico, with a research focus identified as Cosmic Ray Detection. The supplied Scopus information records 42 documents, 1,181 citations, and an h-index of 11. [1] These indicators provide a quantitative overview of the indexed research record, while assessment of scientific contribution requires examination of the underlying publications and their documented research context.

References

  1. Elsevier. (n.d.). Scopus author details: Epifanio Ponce, Author ID 16029702500. Scopus.
    https://www.scopus.com/authid/detail.uri?authorId=16029702500
  2. HAWC performance enhanced by machine learning in gamma-hadron separation. The Astrophysical Journal, 992(1), Article 156.
    https://doi.org/10.3847/1538-4357/ae0186
  3. Internet-based experiment to measure the muon lifetime in real time. Revista Mexicana de Física E, 23(1), 010217.
    https://doi.org/10.31349/RevMexFisE.23.010217

Abdul Kabir | Nuclear astrophysics | Young Scientist Award

Published on by Physicist Particle

Assist. Prof. Dr. Abdul Kabir | Nuclear astrophysics | Young Scientist Award

Assistant Professor at Institute of Space Technology Islamabad, Pakistan

Dr. Abdul Kabir Khan 🎓, born on 11 March 1991 🇵🇰, is an Assistant Professor of Physics at the Institute of Space Technology (IST), Islamabad. He specializes in Theoretical Nuclear Astrophysics 🔭 and is an HEC-approved Ph.D. supervisor. His research bridges nuclear physics and astrophysics, focusing on nuclear properties under extreme conditions 🌌. He earned his Ph.D. and MS from GIK Institute 🏛️, with multiple Gold Medals 🥇. Dr. Khan has published and reviewed for leading journals 📖 and has also contributed significantly to curriculum development 📚 and project management 🛠️ at IST.

Professional Profile:

Orcid

Scopus

Google Scholar

🎓 Education & Experience 

Education:

  • 🎓 Ph.D. in Theoretical Nuclear Astrophysics — GIK Institute (2018-2021)

  • 🎓 MS in Theoretical Nuclear Astrophysics — GIK Institute (2016-2018) 🥇

  • 🎓 M.Sc. in Theoretical Physics — Abdul Wali Khan University, Mardan (2014-2016) 🥇

  • 🎓 B.Sc. (Physics, Maths-A, Electronics) — Abdul Wali Khan University, Mardan (2011-2013) 🥇

  • 🎓 F.Sc. (Pre-Engineering & Biology) — BISE Mardan (2008-2010)

  • 🎓 SSC (Sciences) — BISE Peshawar (2005-2007)

Experience:

  • 👨‍🏫 Assistant Professor, Department of Space Science, IST Islamabad (2021–Present)

  • 👨‍🏫 Lecturer, Govt Post Graduate College Mardan (2021)

  • 👨‍🔬 Research & Graduate Assistant, GIK Institute (2016–2021)

  • 👨‍🏫 Teaching Assistant, GIK Institute (2016–2018)

  • 👨‍🏫 Lecturer, Govt Degree College Mardan (2015–2016)

  • 🚀 Co-PI, Space and Astrophysics Research Lab (2023–Present)

🧠 Professional Development 

Dr. Abdul Kabir Khan has actively participated in academic and administrative roles alongside his teaching 📚. He has contributed to curriculum design 🛠️, managed program specifications 🧩, and supervised BS/MS/Ph.D. Self-Assessment Reports 📄 at IST. As a scholarship and social media focal person 🎯, he has enhanced outreach and student engagement 📢. He has also managed Final Year Projects 🏆, showing commitment to research mentoring. His professional growth is evident from his multiple academic appointments, conference participation 📜, and his role as a reviewer for esteemed journals 🔍. Dr. Khan remains devoted to bridging education and research excellence 🌟.

🔬 Research Focus 

Dr. Abdul Kabir Khan’s research domain is Theoretical Nuclear Astrophysics 🚀. His focus lies in studying nuclear properties under extreme conditions 🌋, radiative capture reactions, nuclear weak interaction rates, and stellar evolution 🔥. He develops and applies models like the relativistic mean field, R-matrix approach, and potential models to investigate nucleosynthesis processes (r-, s-, p-, rp-processes) 🌌. His work extends from low-energy nuclear reactions to stellar explosion mechanisms 🌟. Dr. Khan aims to bridge fundamental nuclear physics and astrophysical phenomena, thus contributing crucial insights into cosmic element formation and the behavior of matter under extreme astrophysical environments 💫.

🏅 Awards & Honors 

  • 🥇 Gold Medalist in M.S. — GIK Institute

  • 🥇 Gold Medalist in M.Sc. — Abdul Wali Khan University

  • 🥇 Gold Medalist in B.Sc. — Abdul Wali Khan University

  • 🏆 Best Final Year Project Award (2021–2022) — IST Islamabad

  • 🏆 Best Final Year Project Award (2022–2023) — IST Islamabad

  • 🏆 Best Final Year Project Award (2023–2024) — IST Islamabad

  • 🏅 Young Scientist Award (AI & Robotics) — 2023

  • 🎖️ Secured First Position in SSC (Science Group) — 2007

  • 🏅 Research Assistantship (Ph.D. and MS) — GIK Institute

  • 📜 HEC Approved PhD Supervisor — Since June 2022

  • 🧪 Reviewer for leading journals like Nuclear Physics A, Scientific Reports, Physica Scripta, Advances in Space Research, and Chinese Physics

Publication Top Notes

1. Investigation of ground state and the β-decay properties of 156−162Nd

  • Journal: Nuclear Physics A

  • Publication Date: May 2025

  • Type: Journal Article

  • DOI: 10.1016/j.nuclphysa.2025.123057

  • Source: Crossref

  • Summary: This study explores the ground-state structures and β-decay behaviors of neodymium isotopes 156−162^{156-162}Nd. It likely involves theoretical nuclear models and experimental comparisons relevant to nuclear structure physics.

2. Investigation of 14C(p, γ)15N at low energies

  • Journal: Modern Physics Letters A

  • Publication Date: January 20, 2025

  • Type: Journal Article

  • DOI: 10.1142/S0217732324502080

  • Source: Crossref

  • Summary: Focuses on the proton capture reaction 14C(p,γ)15N^{14}\text{C}(p,\gamma)^{15}\text{N} at low energy ranges, which is important for astrophysical processes like stellar nucleosynthesis and primordial element formation.

3. Arbitrary amplitude electron-acoustic solitary waves in magnetoplasma with Kaniadakis distributed electrons

  • Journal: AIP Advances

  • Publication Date: December 1, 2024

  • Type: Journal Article

  • DOI: 10.1063/5.0240816

  • Source: Crossref

  • Summary: Studies electron-acoustic solitary waves in magnetized plasma considering Kaniadakis statistics (a generalized statistical framework), possibly useful for understanding space and astrophysical plasma behaviors.

4. Effect of ions anisotropy pressure on the ion-acoustic cnoidal waves in electron–positron–ion magnetoplasmas

  • Journal: AIP Advances

  • Publication Date: September 1, 2024

  • Type: Journal Article

  • DOI: 10.1063/5.0232570

  • Source: Crossref

  • Summary: Analyzes how anisotropic ion pressures affect ion-acoustic cnoidal waves in plasmas containing electrons, positrons, and ions under magnetic fields. Cnoidal waves are periodic solutions of nonlinear wave equations.

5. Re-investigation of Neutron Capture by 84^{84}Kr and 86^{86}Kr in the s-Process Nucleosynthesis

  • Journal: Brazilian Journal of Physics

  • Publication Date: June 2024

  • Type: Journal Article

  • DOI: 10.1007/s13538-024-01455-5

  • Source: Crossref

  • Summary: Re-evaluates the neutron capture cross-sections of krypton isotopes 84^{84}Kr and 86^{86}Kr, which are important for modeling the slow neutron capture (s-process) in stellar environments.

Conclusion

Dr. Abdul Kabir Khan demonstrates the perfect blend of scientific excellence, leadership ability, innovation, and community service required for a Young Scientist Award. His contributions in theoretical nuclear astrophysics significantly advance understanding in a challenging frontier of physics. His academic record, research depth, leadership in institutional development, and recognition by the scientific community make him a highly deserving and outstanding candidate for the award.