Non-coaxial rotating flow of viscous fluid with heat and mass transfer
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作者:
Mohamad, Ahmad Qushairi
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Univ Teknol Malaysia, Fac Sci, Dept Math Sci, Johor Baharu 81310, MalaysiaUniv Teknol Malaysia, Fac Sci, Dept Math Sci, Johor Baharu 81310, Malaysia
Mohamad, Ahmad Qushairi
[1
]
Khan, Ilyas
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Majmaah Univ, Coll Engn, Basic Engn Sci Dept, Majmaah 11952, Saudi ArabiaUniv Teknol Malaysia, Fac Sci, Dept Math Sci, Johor Baharu 81310, Malaysia
Khan, Ilyas
[2
]
Shafie, Sharidan
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Univ Teknol Malaysia, Fac Sci, Dept Math Sci, Johor Baharu 81310, MalaysiaUniv Teknol Malaysia, Fac Sci, Dept Math Sci, Johor Baharu 81310, Malaysia
Shafie, Sharidan
[1
]
Isa, Zaiton Mat
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Univ Teknol Malaysia, Fac Sci, Dept Math Sci, Johor Baharu 81310, MalaysiaUniv Teknol Malaysia, Fac Sci, Dept Math Sci, Johor Baharu 81310, Malaysia
Isa, Zaiton Mat
[1
]
Ismail, Zulkhibri
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Univ Malaysia Pahang, Fac Ind Sci & Technol, Kuantan 263002, Pahang, IndiaUniv Teknol Malaysia, Fac Sci, Dept Math Sci, Johor Baharu 81310, Malaysia
Ismail, Zulkhibri
[3
]
机构:
[1] Univ Teknol Malaysia, Fac Sci, Dept Math Sci, Johor Baharu 81310, Malaysia
Heat and mass transfer in unsteady non-coaxial rotating flow of viscous fluid over an infinite vertical disk is investigated. The motion in the fluid is induced due to two sources. Firstly, due to the buoyancy force which is caused because of temperature and concentration gradients. Secondly, because of non-coaxial rotation of a disk such that the disk executes cosine or since oscillation in its plane and the fluid is at infinity. The problem is modeled in terms of coupled partial differential equations with some physical boundary and initial conditions. The dimensionless form of the problem is solved via Laplace transform method for exact solutions. Expressions for velocity field, temperature and concentration distributions are obtained, satisfying all the initial and boundary conditions. Skin friction, Nusselt number and Sherwood number are also evaluated. The physical significance of the mathematical results is shown in various plots and is discussed for several embedded parameters. It is found that magnitude of primary velocity is less than secondary velocity. In limiting sense, the present solutions are found identical with published results.
机构:
COMSATS Inst Informat Technol, Dept Math, Islamabad, PakistanUniv North West, Dept Math Sci, Int Inst Symmetry Anal & Math Modelling, ZA-2735 Mmabatho, South Africa
Asghar, S.
Hanif, K.
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Quaid I Azam Univ, Dept Math, Islamabad, PakistanUniv North West, Dept Math Sci, Int Inst Symmetry Anal & Math Modelling, ZA-2735 Mmabatho, South Africa
Hanif, K.
Hayat, T.
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Quaid I Azam Univ, Dept Math, Islamabad, PakistanUniv North West, Dept Math Sci, Int Inst Symmetry Anal & Math Modelling, ZA-2735 Mmabatho, South Africa
Hayat, T.
Khalique, C. M.
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Univ North West, Dept Math Sci, Int Inst Symmetry Anal & Math Modelling, ZA-2735 Mmabatho, South AfricaUniv North West, Dept Math Sci, Int Inst Symmetry Anal & Math Modelling, ZA-2735 Mmabatho, South Africa
机构:
COMSATS Inst Informat Technol, Dept Math, Islamabad, PakistanUniv North West, Dept Math Sci, Int Inst Symmetry Anal & Math Modelling, ZA-2735 Mmabatho, South Africa
Asghar, S.
Hanif, K.
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机构:
Quaid I Azam Univ, Dept Math, Islamabad, PakistanUniv North West, Dept Math Sci, Int Inst Symmetry Anal & Math Modelling, ZA-2735 Mmabatho, South Africa
Hanif, K.
Hayat, T.
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机构:
Quaid I Azam Univ, Dept Math, Islamabad, PakistanUniv North West, Dept Math Sci, Int Inst Symmetry Anal & Math Modelling, ZA-2735 Mmabatho, South Africa
Hayat, T.
Khalique, C. M.
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Univ North West, Dept Math Sci, Int Inst Symmetry Anal & Math Modelling, ZA-2735 Mmabatho, South AfricaUniv North West, Dept Math Sci, Int Inst Symmetry Anal & Math Modelling, ZA-2735 Mmabatho, South Africa