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First law of thermodynamics (fluid mechanics)

In physics, the first law of thermodynamics is an expression of the conservation of total energy of a system. The increase of the energy of a system is equal to the sum of work done on the system and the heat added to that system:

where

  • is the total energy of a system.
  • is the work done on it.
  • is the heat added to that system.

In fluid mechanics, the first law of thermodynamics takes the following form:[1][2]

where

Because it expresses conservation of total energy, this is sometimes referred to as the energy balance equation of continuous media. The first law is used to derive the non-conservation form of the Navier–Stokes equations.[3]

Note edit

 

Where

That is, pulling is positive stress and pushing is negative stress.

Compressible fluid edit

For a compressible fluid the left hand side of equation becomes:

 

because in general

 

Integral form edit

 

That is, the change in the internal energy of the substance within a volume is the negative of the amount carried out of the volume by the flow of material across the boundary plus the work done compressing the material on the boundary minus the flow of heat out through the boundary. More generally, it is possible to incorporate source terms.[2]

Alternative representation edit

 

where   is specific enthalpy,   is dissipation function and   is temperature. And where

  •  

i.e. internal energy per unit volume equals mass density times the sum of: proper energy per unit mass, kinetic energy per unit mass, and gravitational potential energy per unit mass.

  •  

i.e. change in heat per unit volume (negative divergence of heat flow) equals the divergence of heat conductivity times the gradient of the temperature.

  •  

i.e. divergence of work done against stress equals flow of material times divergence of stress plus stress times divergence of material flow.

  •  

i.e. stress times divergence of material flow equals deviatoric stress tensor times divergence of material flow minus pressure times material flow.

  •  

i.e. enthalpy per unit mass equals proper energy per unit mass plus pressure times volume per unit mass (reciprocal of mass density).

  •  
  •  

Alternative form data edit

  •   left hand side of Navier–Stokes equations minus body force (per unit volume) acting on fluid.
  •   this relation is derived using this relationship   which is alternative form of continuity equation  

See also edit

References edit

  1. ^ F. M. White (2006). Viscous fluid flow (3rd ed.). McGraw Hill. pp. 69–72.
  2. ^ a b Truesdell; Toupin (1960). "The classical field theories". In Flügge (ed.). Encyclopedia of physics: Principles of classical mechanics and field theory. Vol. III. p. 609.
  3. ^ Chung (2002). Computational fluid dynamics. Cambridge University Press. pp. 33–34.

first, thermodynamics, fluid, mechanics, physics, first, thermodynamics, expression, conservation, total, energy, system, increase, energy, system, equal, work, done, system, heat, added, that, system, displaystyle, where, displaystyle, total, energy, system, . In physics the first law of thermodynamics is an expression of the conservation of total energy of a system The increase of the energy of a system is equal to the sum of work done on the system and the heat added to that system d E t d Q d W displaystyle dE t dQ dW where E t displaystyle E t is the total energy of a system W displaystyle W is the work done on it Q displaystyle Q is the heat added to that system In fluid mechanics the first law of thermodynamics takes the following form 1 2 D E t D t D W D t D Q D t D E t D t s v q displaystyle frac DE t Dt frac DW Dt frac DQ Dt to frac DE t Dt nabla cdot mathbf sigma cdot v nabla cdot mathbf q where s displaystyle mathbf sigma is the Cauchy stress tensor v displaystyle mathbf v is the flow velocity and q displaystyle mathbf q is the heat flux vector Because it expresses conservation of total energy this is sometimes referred to as the energy balance equation of continuous media The first law is used to derive the non conservation form of the Navier Stokes equations 3 Contents 1 Note 2 Compressible fluid 3 Integral form 4 Alternative representation 5 Alternative form data 6 See also 7 ReferencesNote edits p I T displaystyle mathbf sigma p mathbf I mathbf T nbsp Where p displaystyle p nbsp is the pressure I displaystyle mathbf I nbsp is the identity matrix T displaystyle mathbf T nbsp is the deviatoric stress tensor That is pulling is positive stress and pushing is negative stress Compressible fluid editFor a compressible fluid the left hand side of equation becomes D E t D t E t E v displaystyle frac DE t Dt frac partial E partial t nabla cdot E mathbf v nbsp because in general v 0 displaystyle nabla cdot mathbf v neq 0 nbsp Integral form edit V E t d V V E v d A V s v d A V q d A displaystyle int V frac partial E partial t dV oint partial V E mathbf v cdot d mathbf A oint partial V mathbf sigma cdot v cdot d mathbf A oint partial V mathbf q cdot d mathbf A nbsp That is the change in the internal energy of the substance within a volume is the negative of the amount carried out of the volume by the flow of material across the boundary plus the work done compressing the material on the boundary minus the flow of heat out through the boundary More generally it is possible to incorporate source terms 2 Alternative representation editr D h D t D p D t k T F displaystyle rho frac Dh Dt frac Dp Dt nabla cdot k nabla T Phi nbsp where h displaystyle h nbsp is specific enthalpy F t v displaystyle Phi mathbf tau nabla mathbf v nbsp is dissipation function and T displaystyle T nbsp is temperature And where E t r e 1 2 v 2 g r displaystyle E t rho e frac 1 2 v 2 mathbf g cdot r nbsp i e internal energy per unit volume equals mass density times the sum of proper energy per unit mass kinetic energy per unit mass and gravitational potential energy per unit mass q k T displaystyle nabla cdot mathbf q nabla cdot k nabla T nbsp i e change in heat per unit volume negative divergence of heat flow equals the divergence of heat conductivity times the gradient of the temperature s v v s s v displaystyle nabla cdot mathbf sigma cdot v mathbf v cdot nabla cdot sigma sigma nabla mathbf v nbsp i e divergence of work done against stress equals flow of material times divergence of stress plus stress times divergence of material flow s v F p v displaystyle sigma nabla mathbf v Phi p nabla cdot mathbf v nbsp i e stress times divergence of material flow equals deviatoric stress tensor times divergence of material flow minus pressure times material flow h e p r displaystyle h e frac p rho nbsp i e enthalpy per unit mass equals proper energy per unit mass plus pressure times volume per unit mass reciprocal of mass density s D J D t f displaystyle nabla cdot sigma frac DJ Dt mathbf f nbsp p v D p D t r D D t p r displaystyle p nabla cdot mathbf v frac Dp Dt rho frac D Dt left frac p rho right nbsp Alternative form data edit s D J D t f displaystyle nabla cdot mathbf sigma frac D mathbf J Dt mathbf f nbsp left hand side of Navier Stokes equations minus body force per unit volume acting on fluid p v D p D t r D D t p r displaystyle p nabla cdot mathbf v frac Dp Dt rho frac D Dt left frac p rho right nbsp this relation is derived using this relationship r v D r D t displaystyle rho nabla cdot mathbf v frac D rho Dt nbsp which is alternative form of continuity equation r t J 0 displaystyle frac partial rho partial t nabla cdot mathbf J 0 nbsp See also editClausius Duhem inequality Continuum mechanics First law of thermodynamics Material derivative Incompressible flowReferences edit F M White 2006 Viscous fluid flow 3rd ed McGraw Hill pp 69 72 a b Truesdell Toupin 1960 The classical field theories In Flugge ed Encyclopedia of physics Principles of classical mechanics and field theory Vol III p 609 Chung 2002 Computational fluid dynamics Cambridge University Press pp 33 34 Retrieved from https en wikipedia org w index php title First law of thermodynamics fluid mechanics amp oldid 1082504881, wikipedia, wiki, book, books, library,

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