Zobrazeno 1 - 10
of 43
pro vyhledávání: '"Ramoona Shehzadi"'
Autor:
Muhammad Ajaz, Abd Haj Ismail, Muhammad Waqas, Ramoona Shehzadi, Ishrat Asghar, Hannan Younis, Mateen Ullah Mian, Atef AbdelKader, Muhammad Adil Khan, Kashif Safeen
Publikováno v:
Atmosphere, Vol 14, Iss 6, p 1028 (2023)
In this work, we performed a comparative study between HIJING, Sibyll, and QGSJET model-based event generators. Such Monte Carlo (MC) models are used to simulate the interaction and propagation of high-energy cosmic radiation (e.g., coming from the s
Externí odkaz:
https://doaj.org/article/67ff954a50b34bcabc99cc5faa7b3b47
Autor:
Muhammad Ajaz, Abd Al Karim Haj Ismail, Mateen Ullah Mian, Rashid Khan, Ramoona Shehzadi, Muhammad Adil Khan, Atef AbdelKader, Muhammad Waqas, Elmuez A. Dawi, Uzma Tabassam
Publikováno v:
Entropy, Vol 25, Iss 3, p 452 (2023)
We present an analysis of the pseudorapidity η and transverse momentum pT distributions of charged hadrons in pp collisions for the kinematic range of 0
Externí odkaz:
https://doaj.org/article/4d43038e047c4805bba3c274d1a0151b
Autor:
Muhammad Ajaz, Abd Al Karim Haj Ismail, Awais Ahmed, Zafar Wazir, Ramoona Shehzadi, Hannan Younis, Gulzar Khan, Rashid Khan, Sajad Ali, Muhammad Waqas, Pei-Pin Yang, Elmuez A. Dawi
Publikováno v:
Results in Physics, Vol 30, Iss , Pp 104790- (2021)
The simulation of transverse momentum (PT) spectra of inclusive charged hadrons computed with absolute pseudorapidity below 0.8 (|η|
Externí odkaz:
https://doaj.org/article/665ed68c3e8b409ea6fd51b182f9fafd
Autor:
Hannan Younis, Farooq Ahmad, Ramoona Shehzadi, Ishrat Asghar, Tanveer Ahmad, Muhammad Ajaz, Muhammad Waqas, Khurram Mehboob, Aziz Ahmad Qureshi, Abd Al Karim Haj Ismail
Publikováno v:
Atmosphere, Vol 12, Iss 11, p 1385 (2021)
Radioactivity in Granites of Pakistan systematically increases from south to north. The Ambella Granite found at the northern edge of Pakistan is highly radioactive. Radioactivity measurements made on, so called, Bajaur Granite, located in northern P
Externí odkaz:
https://doaj.org/article/dd869beadcbf4c90a24ee71fe3f71b32
Autor:
Muhammad Waqas, Huai-Min Chen, Guang-Xiong Peng, Abd Al Karim Haj Ismail, Muhammad Ajaz, Zafar Wazir, Ramoona Shehzadi, Sabiha Jamal, Atef AbdelKader
Publikováno v:
Entropy, Vol 23, Iss 10, p 1363 (2021)
We used the blast wave model with the Boltzmann–Gibbs statistics and analyzed the experimental data measured by the NA61/SHINE Collaboration in inelastic (INEL) proton–proton collisions at different rapidity slices at different center-of-mass ene
Externí odkaz:
https://doaj.org/article/ed17445b0eeb45bd8c8b6518390b12a3
Autor:
Safeen, Muhammad Ajaz, Abd Haj Ismail, Muhammad Waqas, Ramoona Shehzadi, Ishrat Asghar, Hannan Younis, Mateen Ullah Mian, Atef AbdelKader, Muhammad Adil Khan, Kashif
Publikováno v:
Atmosphere; Volume 14; Issue 6; Pages: 1028
In this work, we performed a comparative study between HIJING, Sibyll, and QGSJET model-based event generators. Such Monte Carlo (MC) models are used to simulate the interaction and propagation of high-energy cosmic radiation (e.g., coming from the s
Publikováno v:
New Astronomy. 98:101937
Autor:
Ramoona Shehzadi, Muhammad Ajaz, Huai-Min Chen, Muhammad Waqas, G. X. Peng, Sabiha Jamal, Atef Abdelkader, Z. Wazir, Abd Al Karim Haj Ismail
Publikováno v:
Entropy; Volume 23; Issue 10; Pages: 1363
Entropy
Entropy, Vol 23, Iss 1363, p 1363 (2021)
Entropy
Entropy, Vol 23, Iss 1363, p 1363 (2021)
We used the blast wave model with the Boltzmann–Gibbs statistics and analyzed the experimental data measured by the NA61/SHINE Collaboration in inelastic (INEL) proton–proton collisions at different rapidity slices at different center-of-mass ene
Publikováno v:
Physica Scripta. 97:115301
β-decay is amongst the key properties of nuclei required for the modeling of r-process nucleosynthesis. It also governs the flow of abundances among neighboring isotopic chains of high-mass elements. In the present work, a simple proton-neutron quas
Publikováno v:
Astrophysics and Space Science. 366
In late progressive-stages of heavy stars, electron capture and $\beta^{\pm}$ -decay are the governing processes. The weak rates are essential inputs for the modeling of the stages of high-mass stars before supernova explosions. As per results obtain