Advances in Nano Research
Volume 16, Number 4, 2024, pages 427-434
DOI: 10.12989/anr.2024.16.4.427
Influence of thermal radiation and magnetohydrodynamic on the laminar flow: Williamson fluid for velocity profile
Muzamal Hussain , Humaira Sharif , Mohammad Amien Khadimallah , Hamdi Ayed , Abir Mouldi , Muhammad Naeem Mohsin , Sajjad Hussain , Abdelouahed Tounsi
Abstract
Key Words
activation energy; bio-convection; inclined surface; thermal radiation; Williamson nanofluid
Address
- Muzamal Hussain — Department of Mathematics, University of Sahiwal, Sahiwal, 57000, Sahiwal,Pakistan
- Humaira Sharif — Department of Mathematics, Govt. College University Faisalabad, 38000, Faisalabad, Pakistan
- Mohammad Amien Khadimallah — Department of Civil Engineering, College of Engineering in Al-Kharj, Prince Sattam Bin Abdulaziz University, Al-Kharj, 11942, Saudi Arabia
- Hamdi Ayed — Department of Civil Engineering, College of Engineering, King Khalid University, Abha - 61421, Saudi Arabia
- Abir Mouldi — Department of Industrial Engineering, College of Engineering, King Khalid University, Abha - 61421, Saudi Arabia
- Muhammad Naeem Mohsin — Institute for Islamic Theological Studies, University of Vienna, Schenkenstrabe 8-10,1010, Vienna, Austria
- Sajjad Hussain — Department of mathematics, Government Post graduate college, Layyah, Pakistan
- Abdelouahed Tounsi — Materials and Hydrology Laboratory University of Sidi Bel Abbes, Algeria Faculty of Technology Civil Engineering Department, Sidi Bel Abbes 22000-Algeria/ Department of Civil and Environmental Engineering, King Fahd University of Petroleum and Minerals, 31261 Dhahran, Eastern Province, Saudi Arabia
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