Effect of Non-linear Thermal Radiation and Binary Chemical Reaction on the Williamson Nanofluid Flow Past a Linearly Stretching Sheet
Abstract The presentation of the current article leads to analyze the magnetohydrodynamic flow of Williamson nanofluid past a linearly expanding sheet. Thermodynamical properties of the second law are proposed for the heat transport phenomena using the Buongiorno model with the influential propertie...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Sharma, Ram Prakash [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2022 |
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| Schlagwörter: |
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| Anmerkung: |
© The Author(s), under exclusive licence to Springer Nature India Private Limited 2022 |
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| Übergeordnetes Werk: |
Enthalten in: International journal of applied and computational mathematics - [New Dehli] : Springer India, 2015, 8(2022), 4 vom: 25. Juni |
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| Übergeordnetes Werk: |
volume:8 ; year:2022 ; number:4 ; day:25 ; month:06 |
| Links: |
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| DOI / URN: |
10.1007/s40819-022-01362-w |
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| Katalog-ID: |
SPR047413530 |
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| 520 | |a Abstract The presentation of the current article leads to analyze the magnetohydrodynamic flow of Williamson nanofluid past a linearly expanding sheet. Thermodynamical properties of the second law are proposed for the heat transport phenomena using the Buongiorno model with the influential properties of a binary chemical reaction. The impacts of Brownian, as well as thermophoresis, also affect the flow phenomena significantly. Adopting suitable similarity transformation, the proposed governing equations for the non-Newtonian fluid are transformed to nonlinear ordinary equations and a further numerical approach is implemented for this system combined with the shooting technique. The behavior of the characteristic parameters is shown graphically, and the simulation results of the rate coefficients are shown in the tables. However, the major outcomes are described as; the cross-diffusion effects caused by the Brownian and thermophoresis give rise to enhance the fluid temperature. Further, Eckert number due to the inclusion of dissipative heat along with thermal radiation and magnetic parameter overshoots the fluid temperature. | ||
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| 650 | 4 | |a Numerical scheme |7 (dpeaa)DE-He213 | |
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| 700 | 1 | |a Tinker, Seema |4 aut | |
| 700 | 1 | |a Kulshrestha, B. K. |4 aut | |
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10.1007/s40819-022-01362-w doi (DE-627)SPR047413530 (SPR)s40819-022-01362-w-e DE-627 ger DE-627 rakwb eng Sharma, Ram Prakash verfasserin aut Effect of Non-linear Thermal Radiation and Binary Chemical Reaction on the Williamson Nanofluid Flow Past a Linearly Stretching Sheet 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s), under exclusive licence to Springer Nature India Private Limited 2022 Abstract The presentation of the current article leads to analyze the magnetohydrodynamic flow of Williamson nanofluid past a linearly expanding sheet. Thermodynamical properties of the second law are proposed for the heat transport phenomena using the Buongiorno model with the influential properties of a binary chemical reaction. The impacts of Brownian, as well as thermophoresis, also affect the flow phenomena significantly. Adopting suitable similarity transformation, the proposed governing equations for the non-Newtonian fluid are transformed to nonlinear ordinary equations and a further numerical approach is implemented for this system combined with the shooting technique. The behavior of the characteristic parameters is shown graphically, and the simulation results of the rate coefficients are shown in the tables. However, the major outcomes are described as; the cross-diffusion effects caused by the Brownian and thermophoresis give rise to enhance the fluid temperature. Further, Eckert number due to the inclusion of dissipative heat along with thermal radiation and magnetic parameter overshoots the fluid temperature. Williamson nanofluid (dpeaa)DE-He213 Buongiorno model (dpeaa)DE-He213 Linearly expanding surface (dpeaa)DE-He213 Binary chemical reaction (dpeaa)DE-He213 Numerical scheme (dpeaa)DE-He213 Mishra, S. R. aut Tinker, Seema aut Kulshrestha, B. K. aut Enthalten in International journal of applied and computational mathematics [New Dehli] : Springer India, 2015 8(2022), 4 vom: 25. Juni (DE-627)815914253 (DE-600)2806624-8 2199-5796 nnns volume:8 year:2022 number:4 day:25 month:06 https://dx.doi.org/10.1007/s40819-022-01362-w lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OLC-PHA GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 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_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 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_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 8 2022 4 25 06 |
| spelling |
10.1007/s40819-022-01362-w doi (DE-627)SPR047413530 (SPR)s40819-022-01362-w-e DE-627 ger DE-627 rakwb eng Sharma, Ram Prakash verfasserin aut Effect of Non-linear Thermal Radiation and Binary Chemical Reaction on the Williamson Nanofluid Flow Past a Linearly Stretching Sheet 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s), under exclusive licence to Springer Nature India Private Limited 2022 Abstract The presentation of the current article leads to analyze the magnetohydrodynamic flow of Williamson nanofluid past a linearly expanding sheet. Thermodynamical properties of the second law are proposed for the heat transport phenomena using the Buongiorno model with the influential properties of a binary chemical reaction. The impacts of Brownian, as well as thermophoresis, also affect the flow phenomena significantly. Adopting suitable similarity transformation, the proposed governing equations for the non-Newtonian fluid are transformed to nonlinear ordinary equations and a further numerical approach is implemented for this system combined with the shooting technique. The behavior of the characteristic parameters is shown graphically, and the simulation results of the rate coefficients are shown in the tables. However, the major outcomes are described as; the cross-diffusion effects caused by the Brownian and thermophoresis give rise to enhance the fluid temperature. Further, Eckert number due to the inclusion of dissipative heat along with thermal radiation and magnetic parameter overshoots the fluid temperature. Williamson nanofluid (dpeaa)DE-He213 Buongiorno model (dpeaa)DE-He213 Linearly expanding surface (dpeaa)DE-He213 Binary chemical reaction (dpeaa)DE-He213 Numerical scheme (dpeaa)DE-He213 Mishra, S. R. aut Tinker, Seema aut Kulshrestha, B. K. aut Enthalten in International journal of applied and computational mathematics [New Dehli] : Springer India, 2015 8(2022), 4 vom: 25. Juni (DE-627)815914253 (DE-600)2806624-8 2199-5796 nnns volume:8 year:2022 number:4 day:25 month:06 https://dx.doi.org/10.1007/s40819-022-01362-w lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OLC-PHA GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 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_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 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_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 8 2022 4 25 06 |
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10.1007/s40819-022-01362-w doi (DE-627)SPR047413530 (SPR)s40819-022-01362-w-e DE-627 ger DE-627 rakwb eng Sharma, Ram Prakash verfasserin aut Effect of Non-linear Thermal Radiation and Binary Chemical Reaction on the Williamson Nanofluid Flow Past a Linearly Stretching Sheet 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s), under exclusive licence to Springer Nature India Private Limited 2022 Abstract The presentation of the current article leads to analyze the magnetohydrodynamic flow of Williamson nanofluid past a linearly expanding sheet. Thermodynamical properties of the second law are proposed for the heat transport phenomena using the Buongiorno model with the influential properties of a binary chemical reaction. The impacts of Brownian, as well as thermophoresis, also affect the flow phenomena significantly. Adopting suitable similarity transformation, the proposed governing equations for the non-Newtonian fluid are transformed to nonlinear ordinary equations and a further numerical approach is implemented for this system combined with the shooting technique. The behavior of the characteristic parameters is shown graphically, and the simulation results of the rate coefficients are shown in the tables. However, the major outcomes are described as; the cross-diffusion effects caused by the Brownian and thermophoresis give rise to enhance the fluid temperature. Further, Eckert number due to the inclusion of dissipative heat along with thermal radiation and magnetic parameter overshoots the fluid temperature. Williamson nanofluid (dpeaa)DE-He213 Buongiorno model (dpeaa)DE-He213 Linearly expanding surface (dpeaa)DE-He213 Binary chemical reaction (dpeaa)DE-He213 Numerical scheme (dpeaa)DE-He213 Mishra, S. R. aut Tinker, Seema aut Kulshrestha, B. K. aut Enthalten in International journal of applied and computational mathematics [New Dehli] : Springer India, 2015 8(2022), 4 vom: 25. Juni (DE-627)815914253 (DE-600)2806624-8 2199-5796 nnns volume:8 year:2022 number:4 day:25 month:06 https://dx.doi.org/10.1007/s40819-022-01362-w lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OLC-PHA GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 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_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 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_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 8 2022 4 25 06 |
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10.1007/s40819-022-01362-w doi (DE-627)SPR047413530 (SPR)s40819-022-01362-w-e DE-627 ger DE-627 rakwb eng Sharma, Ram Prakash verfasserin aut Effect of Non-linear Thermal Radiation and Binary Chemical Reaction on the Williamson Nanofluid Flow Past a Linearly Stretching Sheet 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s), under exclusive licence to Springer Nature India Private Limited 2022 Abstract The presentation of the current article leads to analyze the magnetohydrodynamic flow of Williamson nanofluid past a linearly expanding sheet. Thermodynamical properties of the second law are proposed for the heat transport phenomena using the Buongiorno model with the influential properties of a binary chemical reaction. The impacts of Brownian, as well as thermophoresis, also affect the flow phenomena significantly. Adopting suitable similarity transformation, the proposed governing equations for the non-Newtonian fluid are transformed to nonlinear ordinary equations and a further numerical approach is implemented for this system combined with the shooting technique. The behavior of the characteristic parameters is shown graphically, and the simulation results of the rate coefficients are shown in the tables. However, the major outcomes are described as; the cross-diffusion effects caused by the Brownian and thermophoresis give rise to enhance the fluid temperature. Further, Eckert number due to the inclusion of dissipative heat along with thermal radiation and magnetic parameter overshoots the fluid temperature. Williamson nanofluid (dpeaa)DE-He213 Buongiorno model (dpeaa)DE-He213 Linearly expanding surface (dpeaa)DE-He213 Binary chemical reaction (dpeaa)DE-He213 Numerical scheme (dpeaa)DE-He213 Mishra, S. R. aut Tinker, Seema aut Kulshrestha, B. K. aut Enthalten in International journal of applied and computational mathematics [New Dehli] : Springer India, 2015 8(2022), 4 vom: 25. Juni (DE-627)815914253 (DE-600)2806624-8 2199-5796 nnns volume:8 year:2022 number:4 day:25 month:06 https://dx.doi.org/10.1007/s40819-022-01362-w lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OLC-PHA GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 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_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 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_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 8 2022 4 25 06 |
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10.1007/s40819-022-01362-w doi (DE-627)SPR047413530 (SPR)s40819-022-01362-w-e DE-627 ger DE-627 rakwb eng Sharma, Ram Prakash verfasserin aut Effect of Non-linear Thermal Radiation and Binary Chemical Reaction on the Williamson Nanofluid Flow Past a Linearly Stretching Sheet 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s), under exclusive licence to Springer Nature India Private Limited 2022 Abstract The presentation of the current article leads to analyze the magnetohydrodynamic flow of Williamson nanofluid past a linearly expanding sheet. Thermodynamical properties of the second law are proposed for the heat transport phenomena using the Buongiorno model with the influential properties of a binary chemical reaction. The impacts of Brownian, as well as thermophoresis, also affect the flow phenomena significantly. Adopting suitable similarity transformation, the proposed governing equations for the non-Newtonian fluid are transformed to nonlinear ordinary equations and a further numerical approach is implemented for this system combined with the shooting technique. The behavior of the characteristic parameters is shown graphically, and the simulation results of the rate coefficients are shown in the tables. However, the major outcomes are described as; the cross-diffusion effects caused by the Brownian and thermophoresis give rise to enhance the fluid temperature. Further, Eckert number due to the inclusion of dissipative heat along with thermal radiation and magnetic parameter overshoots the fluid temperature. Williamson nanofluid (dpeaa)DE-He213 Buongiorno model (dpeaa)DE-He213 Linearly expanding surface (dpeaa)DE-He213 Binary chemical reaction (dpeaa)DE-He213 Numerical scheme (dpeaa)DE-He213 Mishra, S. R. aut Tinker, Seema aut Kulshrestha, B. K. aut Enthalten in International journal of applied and computational mathematics [New Dehli] : Springer India, 2015 8(2022), 4 vom: 25. Juni (DE-627)815914253 (DE-600)2806624-8 2199-5796 nnns volume:8 year:2022 number:4 day:25 month:06 https://dx.doi.org/10.1007/s40819-022-01362-w lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OLC-PHA GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 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_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 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_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 8 2022 4 25 06 |
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Sharma, Ram Prakash |
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Sharma, Ram Prakash misc Williamson nanofluid misc Buongiorno model misc Linearly expanding surface misc Binary chemical reaction misc Numerical scheme Effect of Non-linear Thermal Radiation and Binary Chemical Reaction on the Williamson Nanofluid Flow Past a Linearly Stretching Sheet |
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Effect of Non-linear Thermal Radiation and Binary Chemical Reaction on the Williamson Nanofluid Flow Past a Linearly Stretching Sheet Williamson nanofluid (dpeaa)DE-He213 Buongiorno model (dpeaa)DE-He213 Linearly expanding surface (dpeaa)DE-He213 Binary chemical reaction (dpeaa)DE-He213 Numerical scheme (dpeaa)DE-He213 |
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Effect of Non-linear Thermal Radiation and Binary Chemical Reaction on the Williamson Nanofluid Flow Past a Linearly Stretching Sheet |
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effect of non-linear thermal radiation and binary chemical reaction on the williamson nanofluid flow past a linearly stretching sheet |
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Effect of Non-linear Thermal Radiation and Binary Chemical Reaction on the Williamson Nanofluid Flow Past a Linearly Stretching Sheet |
| abstract |
Abstract The presentation of the current article leads to analyze the magnetohydrodynamic flow of Williamson nanofluid past a linearly expanding sheet. Thermodynamical properties of the second law are proposed for the heat transport phenomena using the Buongiorno model with the influential properties of a binary chemical reaction. The impacts of Brownian, as well as thermophoresis, also affect the flow phenomena significantly. Adopting suitable similarity transformation, the proposed governing equations for the non-Newtonian fluid are transformed to nonlinear ordinary equations and a further numerical approach is implemented for this system combined with the shooting technique. The behavior of the characteristic parameters is shown graphically, and the simulation results of the rate coefficients are shown in the tables. However, the major outcomes are described as; the cross-diffusion effects caused by the Brownian and thermophoresis give rise to enhance the fluid temperature. Further, Eckert number due to the inclusion of dissipative heat along with thermal radiation and magnetic parameter overshoots the fluid temperature. © The Author(s), under exclusive licence to Springer Nature India Private Limited 2022 |
| abstractGer |
Abstract The presentation of the current article leads to analyze the magnetohydrodynamic flow of Williamson nanofluid past a linearly expanding sheet. Thermodynamical properties of the second law are proposed for the heat transport phenomena using the Buongiorno model with the influential properties of a binary chemical reaction. The impacts of Brownian, as well as thermophoresis, also affect the flow phenomena significantly. Adopting suitable similarity transformation, the proposed governing equations for the non-Newtonian fluid are transformed to nonlinear ordinary equations and a further numerical approach is implemented for this system combined with the shooting technique. The behavior of the characteristic parameters is shown graphically, and the simulation results of the rate coefficients are shown in the tables. However, the major outcomes are described as; the cross-diffusion effects caused by the Brownian and thermophoresis give rise to enhance the fluid temperature. Further, Eckert number due to the inclusion of dissipative heat along with thermal radiation and magnetic parameter overshoots the fluid temperature. © The Author(s), under exclusive licence to Springer Nature India Private Limited 2022 |
| abstract_unstemmed |
Abstract The presentation of the current article leads to analyze the magnetohydrodynamic flow of Williamson nanofluid past a linearly expanding sheet. Thermodynamical properties of the second law are proposed for the heat transport phenomena using the Buongiorno model with the influential properties of a binary chemical reaction. The impacts of Brownian, as well as thermophoresis, also affect the flow phenomena significantly. Adopting suitable similarity transformation, the proposed governing equations for the non-Newtonian fluid are transformed to nonlinear ordinary equations and a further numerical approach is implemented for this system combined with the shooting technique. The behavior of the characteristic parameters is shown graphically, and the simulation results of the rate coefficients are shown in the tables. However, the major outcomes are described as; the cross-diffusion effects caused by the Brownian and thermophoresis give rise to enhance the fluid temperature. Further, Eckert number due to the inclusion of dissipative heat along with thermal radiation and magnetic parameter overshoots the fluid temperature. © The Author(s), under exclusive licence to Springer Nature India Private Limited 2022 |
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Effect of Non-linear Thermal Radiation and Binary Chemical Reaction on the Williamson Nanofluid Flow Past a Linearly Stretching Sheet |
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https://dx.doi.org/10.1007/s40819-022-01362-w |
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Mishra, S. R. Tinker, Seema Kulshrestha, B. K. |
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10.1007/s40819-022-01362-w |
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