Lecture 4 - ffn.ub.eduwebmrubi/papers/lecture_4.pdf · Lecture 4 . Heat transfer at small scales ....
Transcript of Lecture 4 - ffn.ub.eduwebmrubi/papers/lecture_4.pdf · Lecture 4 . Heat transfer at small scales ....
Lecture 4
Heat transfer at small scales
Linear laws between fluxes and forces proposed by NET are not valid: -In ’far-from-equilibrium situations’ For transport processes, the linear response regime holds even for large gradients For activated processes, linearity occurs only very close to equilibrium -At small scales: anomalous heat transfer
1 2( )q dJ G T T= − −
Thermal rectification: Resistance to the heat flow depends on the sign of the T-grad. Asymmetry in the phonon distribution.
Thermal grandient as a driving force
• Water polarization under thermal gradients: F. Bresme, A. Lervik, el al., PRL, 101, 020602 (2008).
• Thermomolecular orientation of nonpolar fluids: F. Römer et al. PRL, 108, 105901 (2008)
• Nanoscale mass conveyors: Regan et al., Nature, 428, 924 (2004)
• Traping of DNA by thermophoretic depletion: D. Braun , A. Libchaber, PRL, 89, 188103 (2002)
• To drive the flow of fluids in nanotubes, nanopores and microfluidoic devices
D. Braun , A. Libchaber, PRL, 89, 188103 (2002)
Very large thermal gradients: typically range from 10^5 K/m on the mesoscale to 10^8 K/m
on the nanoscale
A thermal gradient may induce actuation in DWCN
DWNT
Actuated by the temperature difference the outer NT moves along and/or around the inner tube
Chiral numbers: (n,m)
50-100 m/s ; 1K/nm; thermal force: pico Newtons
0.142cca nm=
0.142cca nm=
1 2hC na ma= +
out inL L<<
Quan-Wen Hou et al, Nanotechnology, 20, 495503 (2009)
Experiments and simulations
A. Barreiro et al., Science, 320, 775 (2008)
0.1I mA
AFM
Energy barrier
Mechanism: in the presence of a thermal gradient, there will be a current of phonons which transfer momentum to the mobile nanotube. - Reverse of the heat dissipation that occurs in friction
Translational motion
Joule heating
Molecular dynamics
Thermal driving force T zz
TFz
κ ∂=
∂
3
2 3
1010 10in
T KL nm∆
−
/ 40 /TF m sζ 4TF pN
3
2 3
100.01 0.1
10 10
inL nmI mA
T K−
∆ −
Observed in experiments 211.5 10 /zz J Kκ −⋅
Observed in simulations
Interwall potential
Structures depend on the chirality Darker color: lower potential energy
Model Two degrees of freedom:
: ( ): ( )
axial z tazimutal tθ
Forces: friction, van der Waals, thermal gradient, random
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1.5
1 2 10 /frictionf pN
Kg sζ −− ⋅
2.1 4.2vdWF pN−
( ) ( ) ( ) ( )1( ) ( ) ( )
vdW Rz zz z z
vdW R
mx t x t F T F t
m t t F F tr θ θ
ζ κ
θ ζθ
= − + + ∇ +
= − + +
( ) (0) 2 ( )
( ) (0) 2 ( )
R Rz z
R Rrot
F t F kT tF t F kT tθ θ
ζδ
ζ δ
< >=
< >=
Equilibrium photon gas
4eqJ Tσ=
Energy conservation # microstates
Planck distribution
Stefan-Boltzmann
1
exp 1N
kT
ω ω=
−
TdS=dE
Planck’s theory is not valid when length scales are comparable to the wave length of thermal radiation
Enhancement of the heat flux in the near-field
Heat Transfer coefficient
Hu et al., Appl. Phys. Lett. 92, 133106 (2008)
Thermal conductance
Domingues et al., Phys. Rev. Lett. 94, 085901 (2005)
Molecular dynamics
Ther
mal
con
duct
ance
Fluctuation-dissipation regime
FDT
Fluctuating electrodynamics
Domingues et al., PRL, 94, 085901 (2005)
Valid when thermalization is very fast
Mesoscopic thermodynamics
( , )x pΓ
( , )n tΓ ?nt
∂
∂
Photons, phonons, electrons,…:
Flux of particles, Heat flux, Energy flux, etc. Second law: entropy
dQ T s nδ µδ= = −
n Jt
∂= −∆
∂
1( )s n J Jt T t T T
µ µ µ∂ ∂= − = ∆ − ∆
∂ ∂
2 1( )LJT
µ µ= − −
2 1
( )
kT kT
kT kT
LJ kLe eT
J l e e
µ µ
µ µ
µ−
= − ∆ ≈ − ∆
= − −
Linear
Nonlinear (Arrhenius)
Nanosystems: fluctuations are important One has to adopt a probabilistic description
kinetics
-D. Reguera, J.M. Rubi and J.M. Vilar, J. Phys. Chem. B (2005) -J.M. Rubi, Scientific American, Nov., 40 (2008)
entropy production
ii) Mesoscopic conductors (Landauer):
iii) Photons
iv) Thermal emission, adsorption (Langmuir), electrokinetic phenomena (Butler-Volmer): Activated processes.
0 01( ) ( )n L n n
t Tµ µ
τ∂
= − − ≈ − −∂
i) Boltzmann (BGK): 0
0
1
0
ln nkTn
LTn
µ µ
τ −
= +
=
[ ]( ) ( ) ( ) ( , ) ( , )st L R R LJ D D n T n Tω ω ω ω ω= − −
( )1( , )
exp / 1n T
kTω
ω=
−
3 4 43 3 ( ) ( )
4st p st R LJ d d J T Tc
ω ω ω σπ
= Ω = −∫
LT RT
ELECTROMAGNETIC WAVES CONFINED IN A VERY NARROW GAP
Spectrum of electromagnetic energy for different detection distances above surface of silicon carbide normalized by its maximum value in far field at T= 300 K. (J.-J. Greffet and C. Henkel, 2007)
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When the distance diminishes, thermal radiation becomes a highly directional beam of coherent radiation. The narrow gap acts as a resonant cavity
Electromagnetic energy density above a plane interface separating glass (amorphous, optical phonons poorly defined) at T = 300 K from vacuum at T = 0 K
Photon Kinetics
2 1*
*
( )
( ) ( )
J n n
t n n d
τ
τ τ
= −
= Γ∫
) ;
)
;
T
T
R
i d black body
ii dx p h
h Kcp E h hd d
λ
λ
ω
>>
≤ ∆ ∆ ≥
∆ ≥ ∆ ≥ ≡
pp xxpx
xp
D D nJ DD x
∂= − ∂
A. Perez, L. Lapas, J.M. Rubi, PRL, 103, 048301 (2009)
Heat flux results from the contribution of Different modes
Input of the theory
Elastic:
Inelastic:
Lognormal DOS
-Statistical model which can describe collective motions. -Stems from the existence of a hierarchy of relaxations mechanisms in the material -The energy consists of a large number of contributions; central limit theorem
Y. V. Denisov, A.P. Rylev, JEPT Lett. 52, 411 (1990) 0: ,Fitting parameters ω σ
Heat transfer coefficient
21
A. Perez, L. Lapas, J.M. Rubi, PRL, 103, 048301 (2009)
FF
NF
30
0
H TH T
A. Perez-Madrid, L. Lapas, J.M. Rubi, Plos One, 8, e58770 (2013)
Summary
• At small scales heat transfer shows anomalous behaviour, not explained by the NET laws. New phenomena: Near-field thermodynamics, thermal rectification, ….
• The linear response regime may extend to the case of large gradients.