Impact of Lorentz Force in Thermally Developed Pulsatile Micropolar Fluid Flow in a Constricted Channel

This work aimed to analyze the heat transfer of micropolar fluid flow in a constricted channel influenced by thermal radiation and the Lorentz force. A finite difference-based flow solver, on a Cartesian grid, is used for the numerical solution after transforming the governing equations into the vor...
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Autor*in:	Muhammad Umar [verfasserIn] Amjad Ali [verfasserIn] Zainab Bukhari [verfasserIn] Gullnaz Shahzadi [verfasserIn] Arshad Saleem [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2021

Schlagwörter:	micropolar fluid constricted channel pulsatile flow thermal radiation Lorentz force heat transfer

Übergeordnetes Werk:	In: Energies - MDPI AG, 2008, 14(2021), 8, p 2173
Übergeordnetes Werk:	volume:14 ; year:2021 ; number:8, p 2173

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.3390/en14082173

Katalog-ID:	DOAJ086778536

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650		4	\|a micropolar fluid
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allfields	10.3390/en14082173 doi (DE-627)DOAJ086778536 (DE-599)DOAJ398d938820fc4918909ceb66f0f8b370 DE-627 ger DE-627 rakwb eng Muhammad Umar verfasserin aut Impact of Lorentz Force in Thermally Developed Pulsatile Micropolar Fluid Flow in a Constricted Channel 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier This work aimed to analyze the heat transfer of micropolar fluid flow in a constricted channel influenced by thermal radiation and the Lorentz force. A finite difference-based flow solver, on a Cartesian grid, is used for the numerical solution after transforming the governing equations into the vorticity-stream function form. The impact of various emerging parameters on the wall shear stress, axial velocity, micro-rotation velocity and temperature profiles is discussed in this paper. The temperature profile is observed to have an inciting trend towards the thermal radiation, whereas it has a declining trend towards the Hartman and Prandtl numbers. The axial velocity profile has an inciting trend towards the Hartman number, whereas it has a declining trend towards the micropolar parameter and Reynolds number. The micro-rotation velocity escalates with the micropolar parameter and Hartman number, whereas it de-escalates with the Reynolds number. The Nusselt number is observed to have a direct relationship with the Prandtl and Reynolds numbers. micropolar fluid constricted channel pulsatile flow thermal radiation Lorentz force heat transfer Technology T Amjad Ali verfasserin aut Zainab Bukhari verfasserin aut Gullnaz Shahzadi verfasserin aut Arshad Saleem verfasserin aut In Energies MDPI AG, 2008 14(2021), 8, p 2173 (DE-627)572083742 (DE-600)2437446-5 19961073 nnns volume:14 year:2021 number:8, p 2173 https://doi.org/10.3390/en14082173 kostenfrei https://doaj.org/article/398d938820fc4918909ceb66f0f8b370 kostenfrei https://www.mdpi.com/1996-1073/14/8/2173 kostenfrei https://doaj.org/toc/1996-1073 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2005 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2055 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2119 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 14 2021 8, p 2173
spelling	10.3390/en14082173 doi (DE-627)DOAJ086778536 (DE-599)DOAJ398d938820fc4918909ceb66f0f8b370 DE-627 ger DE-627 rakwb eng Muhammad Umar verfasserin aut Impact of Lorentz Force in Thermally Developed Pulsatile Micropolar Fluid Flow in a Constricted Channel 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier This work aimed to analyze the heat transfer of micropolar fluid flow in a constricted channel influenced by thermal radiation and the Lorentz force. A finite difference-based flow solver, on a Cartesian grid, is used for the numerical solution after transforming the governing equations into the vorticity-stream function form. The impact of various emerging parameters on the wall shear stress, axial velocity, micro-rotation velocity and temperature profiles is discussed in this paper. The temperature profile is observed to have an inciting trend towards the thermal radiation, whereas it has a declining trend towards the Hartman and Prandtl numbers. The axial velocity profile has an inciting trend towards the Hartman number, whereas it has a declining trend towards the micropolar parameter and Reynolds number. The micro-rotation velocity escalates with the micropolar parameter and Hartman number, whereas it de-escalates with the Reynolds number. The Nusselt number is observed to have a direct relationship with the Prandtl and Reynolds numbers. micropolar fluid constricted channel pulsatile flow thermal radiation Lorentz force heat transfer Technology T Amjad Ali verfasserin aut Zainab Bukhari verfasserin aut Gullnaz Shahzadi verfasserin aut Arshad Saleem verfasserin aut In Energies MDPI AG, 2008 14(2021), 8, p 2173 (DE-627)572083742 (DE-600)2437446-5 19961073 nnns volume:14 year:2021 number:8, p 2173 https://doi.org/10.3390/en14082173 kostenfrei https://doaj.org/article/398d938820fc4918909ceb66f0f8b370 kostenfrei https://www.mdpi.com/1996-1073/14/8/2173 kostenfrei https://doaj.org/toc/1996-1073 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2005 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2055 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2119 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 14 2021 8, p 2173
allfields_unstemmed	10.3390/en14082173 doi (DE-627)DOAJ086778536 (DE-599)DOAJ398d938820fc4918909ceb66f0f8b370 DE-627 ger DE-627 rakwb eng Muhammad Umar verfasserin aut Impact of Lorentz Force in Thermally Developed Pulsatile Micropolar Fluid Flow in a Constricted Channel 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier This work aimed to analyze the heat transfer of micropolar fluid flow in a constricted channel influenced by thermal radiation and the Lorentz force. A finite difference-based flow solver, on a Cartesian grid, is used for the numerical solution after transforming the governing equations into the vorticity-stream function form. The impact of various emerging parameters on the wall shear stress, axial velocity, micro-rotation velocity and temperature profiles is discussed in this paper. The temperature profile is observed to have an inciting trend towards the thermal radiation, whereas it has a declining trend towards the Hartman and Prandtl numbers. The axial velocity profile has an inciting trend towards the Hartman number, whereas it has a declining trend towards the micropolar parameter and Reynolds number. The micro-rotation velocity escalates with the micropolar parameter and Hartman number, whereas it de-escalates with the Reynolds number. The Nusselt number is observed to have a direct relationship with the Prandtl and Reynolds numbers. micropolar fluid constricted channel pulsatile flow thermal radiation Lorentz force heat transfer Technology T Amjad Ali verfasserin aut Zainab Bukhari verfasserin aut Gullnaz Shahzadi verfasserin aut Arshad Saleem verfasserin aut In Energies MDPI AG, 2008 14(2021), 8, p 2173 (DE-627)572083742 (DE-600)2437446-5 19961073 nnns volume:14 year:2021 number:8, p 2173 https://doi.org/10.3390/en14082173 kostenfrei https://doaj.org/article/398d938820fc4918909ceb66f0f8b370 kostenfrei https://www.mdpi.com/1996-1073/14/8/2173 kostenfrei https://doaj.org/toc/1996-1073 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2005 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2055 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2119 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 14 2021 8, p 2173
allfieldsGer	10.3390/en14082173 doi (DE-627)DOAJ086778536 (DE-599)DOAJ398d938820fc4918909ceb66f0f8b370 DE-627 ger DE-627 rakwb eng Muhammad Umar verfasserin aut Impact of Lorentz Force in Thermally Developed Pulsatile Micropolar Fluid Flow in a Constricted Channel 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier This work aimed to analyze the heat transfer of micropolar fluid flow in a constricted channel influenced by thermal radiation and the Lorentz force. A finite difference-based flow solver, on a Cartesian grid, is used for the numerical solution after transforming the governing equations into the vorticity-stream function form. The impact of various emerging parameters on the wall shear stress, axial velocity, micro-rotation velocity and temperature profiles is discussed in this paper. The temperature profile is observed to have an inciting trend towards the thermal radiation, whereas it has a declining trend towards the Hartman and Prandtl numbers. The axial velocity profile has an inciting trend towards the Hartman number, whereas it has a declining trend towards the micropolar parameter and Reynolds number. The micro-rotation velocity escalates with the micropolar parameter and Hartman number, whereas it de-escalates with the Reynolds number. The Nusselt number is observed to have a direct relationship with the Prandtl and Reynolds numbers. micropolar fluid constricted channel pulsatile flow thermal radiation Lorentz force heat transfer Technology T Amjad Ali verfasserin aut Zainab Bukhari verfasserin aut Gullnaz Shahzadi verfasserin aut Arshad Saleem verfasserin aut In Energies MDPI AG, 2008 14(2021), 8, p 2173 (DE-627)572083742 (DE-600)2437446-5 19961073 nnns volume:14 year:2021 number:8, p 2173 https://doi.org/10.3390/en14082173 kostenfrei https://doaj.org/article/398d938820fc4918909ceb66f0f8b370 kostenfrei https://www.mdpi.com/1996-1073/14/8/2173 kostenfrei https://doaj.org/toc/1996-1073 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2005 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2055 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2119 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 14 2021 8, p 2173
allfieldsSound	10.3390/en14082173 doi (DE-627)DOAJ086778536 (DE-599)DOAJ398d938820fc4918909ceb66f0f8b370 DE-627 ger DE-627 rakwb eng Muhammad Umar verfasserin aut Impact of Lorentz Force in Thermally Developed Pulsatile Micropolar Fluid Flow in a Constricted Channel 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier This work aimed to analyze the heat transfer of micropolar fluid flow in a constricted channel influenced by thermal radiation and the Lorentz force. A finite difference-based flow solver, on a Cartesian grid, is used for the numerical solution after transforming the governing equations into the vorticity-stream function form. The impact of various emerging parameters on the wall shear stress, axial velocity, micro-rotation velocity and temperature profiles is discussed in this paper. The temperature profile is observed to have an inciting trend towards the thermal radiation, whereas it has a declining trend towards the Hartman and Prandtl numbers. The axial velocity profile has an inciting trend towards the Hartman number, whereas it has a declining trend towards the micropolar parameter and Reynolds number. The micro-rotation velocity escalates with the micropolar parameter and Hartman number, whereas it de-escalates with the Reynolds number. The Nusselt number is observed to have a direct relationship with the Prandtl and Reynolds numbers. micropolar fluid constricted channel pulsatile flow thermal radiation Lorentz force heat transfer Technology T Amjad Ali verfasserin aut Zainab Bukhari verfasserin aut Gullnaz Shahzadi verfasserin aut Arshad Saleem verfasserin aut In Energies MDPI AG, 2008 14(2021), 8, p 2173 (DE-627)572083742 (DE-600)2437446-5 19961073 nnns volume:14 year:2021 number:8, p 2173 https://doi.org/10.3390/en14082173 kostenfrei https://doaj.org/article/398d938820fc4918909ceb66f0f8b370 kostenfrei https://www.mdpi.com/1996-1073/14/8/2173 kostenfrei https://doaj.org/toc/1996-1073 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2005 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2055 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2119 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 14 2021 8, p 2173
language	English
source	In Energies 14(2021), 8, p 2173 volume:14 year:2021 number:8, p 2173
sourceStr	In Energies 14(2021), 8, p 2173 volume:14 year:2021 number:8, p 2173
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	micropolar fluid constricted channel pulsatile flow thermal radiation Lorentz force heat transfer Technology T
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container_title	Energies
authorswithroles_txt_mv	Muhammad Umar @@aut@@ Amjad Ali @@aut@@ Zainab Bukhari @@aut@@ Gullnaz Shahzadi @@aut@@ Arshad Saleem @@aut@@
publishDateDaySort_date	2021-01-01T00:00:00Z
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author	Muhammad Umar
spellingShingle	Muhammad Umar misc micropolar fluid misc constricted channel misc pulsatile flow misc thermal radiation misc Lorentz force misc heat transfer misc Technology misc T Impact of Lorentz Force in Thermally Developed Pulsatile Micropolar Fluid Flow in a Constricted Channel
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topic_title	Impact of Lorentz Force in Thermally Developed Pulsatile Micropolar Fluid Flow in a Constricted Channel micropolar fluid constricted channel pulsatile flow thermal radiation Lorentz force heat transfer
topic	misc micropolar fluid misc constricted channel misc pulsatile flow misc thermal radiation misc Lorentz force misc heat transfer misc Technology misc T
topic_unstemmed	misc micropolar fluid misc constricted channel misc pulsatile flow misc thermal radiation misc Lorentz force misc heat transfer misc Technology misc T
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title	Impact of Lorentz Force in Thermally Developed Pulsatile Micropolar Fluid Flow in a Constricted Channel
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title_sort	impact of lorentz force in thermally developed pulsatile micropolar fluid flow in a constricted channel
title_auth	Impact of Lorentz Force in Thermally Developed Pulsatile Micropolar Fluid Flow in a Constricted Channel
abstract	This work aimed to analyze the heat transfer of micropolar fluid flow in a constricted channel influenced by thermal radiation and the Lorentz force. A finite difference-based flow solver, on a Cartesian grid, is used for the numerical solution after transforming the governing equations into the vorticity-stream function form. The impact of various emerging parameters on the wall shear stress, axial velocity, micro-rotation velocity and temperature profiles is discussed in this paper. The temperature profile is observed to have an inciting trend towards the thermal radiation, whereas it has a declining trend towards the Hartman and Prandtl numbers. The axial velocity profile has an inciting trend towards the Hartman number, whereas it has a declining trend towards the micropolar parameter and Reynolds number. The micro-rotation velocity escalates with the micropolar parameter and Hartman number, whereas it de-escalates with the Reynolds number. The Nusselt number is observed to have a direct relationship with the Prandtl and Reynolds numbers.
abstractGer	This work aimed to analyze the heat transfer of micropolar fluid flow in a constricted channel influenced by thermal radiation and the Lorentz force. A finite difference-based flow solver, on a Cartesian grid, is used for the numerical solution after transforming the governing equations into the vorticity-stream function form. The impact of various emerging parameters on the wall shear stress, axial velocity, micro-rotation velocity and temperature profiles is discussed in this paper. The temperature profile is observed to have an inciting trend towards the thermal radiation, whereas it has a declining trend towards the Hartman and Prandtl numbers. The axial velocity profile has an inciting trend towards the Hartman number, whereas it has a declining trend towards the micropolar parameter and Reynolds number. The micro-rotation velocity escalates with the micropolar parameter and Hartman number, whereas it de-escalates with the Reynolds number. The Nusselt number is observed to have a direct relationship with the Prandtl and Reynolds numbers.
abstract_unstemmed	This work aimed to analyze the heat transfer of micropolar fluid flow in a constricted channel influenced by thermal radiation and the Lorentz force. A finite difference-based flow solver, on a Cartesian grid, is used for the numerical solution after transforming the governing equations into the vorticity-stream function form. The impact of various emerging parameters on the wall shear stress, axial velocity, micro-rotation velocity and temperature profiles is discussed in this paper. The temperature profile is observed to have an inciting trend towards the thermal radiation, whereas it has a declining trend towards the Hartman and Prandtl numbers. The axial velocity profile has an inciting trend towards the Hartman number, whereas it has a declining trend towards the micropolar parameter and Reynolds number. The micro-rotation velocity escalates with the micropolar parameter and Hartman number, whereas it de-escalates with the Reynolds number. The Nusselt number is observed to have a direct relationship with the Prandtl and Reynolds numbers.
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title_short	Impact of Lorentz Force in Thermally Developed Pulsatile Micropolar Fluid Flow in a Constricted Channel
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