On the roles of energy and entropy in thermodynamics by Ingo Mller - - PowerPoint PPT Presentation

on the roles of energy and entropy in thermodynamics
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On the roles of energy and entropy in thermodynamics by Ingo Mller - - PowerPoint PPT Presentation

On the roles of energy and entropy in thermodynamics by Ingo Mller & Wolf Weiss TU Berlin T q J.B. Fourier i x i v v t 2 i l ij ij x x j l G.


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SLIDE 1

On the roles of energy and entropy in thermodynamics

by Ingo Müller & Wolf Weiss TU Berlin

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SLIDE 2

Derivations did not require the knowledge of the nature of heat, let alone the concepts of energy and entropy

J.B. Fourier

i i

x T q     

ij l l j i ij

x v x v t         

 

2

C.-L. Navier

  • G. G. Stokes
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SLIDE 3

First Law:

probabilistic interpretation

===►

Minimal energy is conducive to equilibrium and so is maximal entropy. Temperature is control parameter. Competition between determinism by which energy approaches a minimum and stochasticity by which entropy approaches a maximum.

W Q dt dE     T Q dt dS  

W k S ln 

m equilibriu in Minimum    S T E A

  • R. Clausius
  • H. v. Helmholtz
  • R. J. Mayer

Second Law:

  • J. P. Joule
  • S. Carnot
  • L. Boltzmann
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SLIDE 4

Planetary Atmospheres

Energy of atmosphere is minimal when all air molecules lie on the solid surface. Who wins? Entropy is maximal when air molecules are evenly distributed throughout space..

Relevant parameter

Mercury and Moon have already lost their atmospheres Jupiter, Saturn and Uranus have kept even light gases Earth hangs on to oxygen and nitrogen – for he the time being !

T k R M    

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SLIDE 5

Osmosis

Pfeffer tube

  • W. Pfeffer
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SLIDE 6

Phase Diagrams (for alloys and solutions)

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SLIDE 7

Ammonia Synthesis (Haber-Bosch)

3 2 2

2 3 NH N H   mol kJ h h h h

NH N H

4 . 92 2 3

3 2 2

       K mol J s s s s

NH N H

6 . 178 3

3 2 2

      

  • F. Haber
  • K. Bosch
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SLIDE 8

Doctrine of Forces and Fluxes (TIP)

Gibbs equation

Entropy Inequality

Thus follows a semi systematic derivation for the laws of Fourier, Navier-Stokes and Fick by linear relations between forces and fluxes. Fully satisfactory for liquids and dense gases. But deficient when rates of change are rapid and gradients are steep as may easily happen in rarefied gases

           dt dc g dt d p dt du T dt ds

 

  

2

1

                

T J g q x dt ds

i i i    

1

3 1 1 1 1 1

1 1

                           

     

 

l l ii i i ij i i i i a n a a

x v p t T x v t T x T g J x T q g T

      

  

energy balance mass balance partial mass balance

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SLIDE 9

Extended Thermodynamics

Fields Field equation Entropy Principle

(α=1,2, ...N) Solutions: Thermodynamic processes for all thermodynamic processes and concave for all fields Change of fields Field equations

symmetric hyperbolic !!

Conclusion: Entropy Principle guarantees that the field equations are symmetric hyperbolic. Initial value problems well-posed:

  • existence and uniqueness of solutions
  • continuous dependence of solutions on initial data
  • finite characteristic speeds

u

) ( ) (

   

u x u F t u

i i

      

) ( ) (        

 

u x u h t h

i i

) (                       

i i i i

x F t u x u h t h

   

) , ( t x u

i 

 

  u

      

                    

i i

x h t h

2 2

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SLIDE 10

Extended Thermodynamics of 21 Moments (and partial systems)

Navier- Stokes Grad´s 13-moment Euler Cattaneo

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SLIDE 11

Heat conduction in the gap between two coaxial cylinders

Comparison between Fourier´s law and Grad´s 13-moment theory

A gas cannot rotate rigidly between the cylinders, if there is heat. A gas between the cylinders cannot be at rest on a turn table, if there is heat flow.           

1 2 1 2

75 56 ln 5 c p r p c c T

k

 

  • H. Grad
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SLIDE 12

Light Scattering

ET is a theory of many theories with only one parameter: The number of fields. For light scattering the theory provides results which are

  • satisfactory (because continuum theory works)
  • surprising (because theory provides its own limit of applicability)
  • disappointing (because so many moments are needed)
  • L. Onsager

ET 120, 165, 220, 286

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SLIDE 13

Literature

Müller,I., Weiss,W. Entropy and Energy, a universal competition. Springer Verlag, Heidelberg (2005) Müller,I., Ruggeri,T. Rational Extended Thermodynamics. Springer Verlag, New York (1998) Müller,I., Weiss,W. Thermodynamics of irreversible processes -- past and present. The European Physical Journal H 37, pp. 139-236 (2012)