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Thermodynamics and dynamics of systems

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Mukamel, Ruffo, Schreiber (2005); Barre, Mukamel, Ruffo (2001) s=S/N , =E/N , m=M/N , u=U/N ... Yamaguchi, Barre, Bouchet, Dauxois, Ruffo (2004) Summary ... – PowerPoint PPT presentation

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Title: Thermodynamics and dynamics of systems


1
Thermodynamics and dynamics of systems with long
range interactions David Mukamel
2
Systems with long range interactions
two-body interaction
v(r) a 1/rs at large r with sltd, d
dimensions
examples dipolar interactions, self gravitating
systems, coulomb interactions, vortices in two
dimensions, electrons interacting with laser
field etc.
3
Thermodynamics
since
the entropy may be neglected in
the Thermodynamic limit
the equilibrium state is just the ground state
4
In order to make the energy and the entropy scale
in the same way one may rescale the
Hamiltonian (Kac prescription)
This rescaling is relevant in a number of
cases, such as
self gravitating systems ferromagnetic dipolar
systems
5
Self gravitating systems
In finite systems, although EgtgtS, if T is high
enough may be comparable to S, and the
full free energy need to be considered.
6
Self gravitating systems
e.g. in globular clusters clusters of the order
105 stars within a distance of 102 light years.
May be considered as a gas of massive objects
Thus although
since T is large
becomes comparable to S
7
Ferromagnetic dipolar systems
v 1/r3
D is the shape dependent demagnetization factor
8
Discuss features which result from the
non-additivity models with Hamiltonian
9
Some general considerations
Negative specific heat in microcanonical
ensemble of non-additive systems. Antonov (1962)
Lynden-Bell Wood (1968) Thirring (1970)
coexistence region in systems with short range
interactions
E0 xE1 (1-x)E2 S0 xS1 (1-x)S2
hence S is concave and the microcanonical specific
heat is non-negative
10
On the other hand in systems with long range
interactions (non-additive), in the region
E1ltEltE2
E0 xE1 (1-x)E2 S0
xS1 (1-x)S2
S
The entropy may thus follow the
homogeneous system curve, the entropy is not
concave. and the microcanonical specific heat
becomes negative.
compared with canonical ensemble where
11
To study this question of ensembles
inequivalence in more detail it is instructive to
consider mean-field type interactions, e.g.
in Ising models
Although the canonical thermodynamic functions
(free energy, entropy etc) are extensive, the
system is non-additive
12
Ising model with long and short range
interactions.
d1 dimensional geometry, ferromagnetic long
range interaction Jgt0
The model has been analyzed within the canonical
ensemble Nagel (1970), Kardar (1983)
13
T/J
2nd order
1st order
K/J
0
-1/2
14
Canonical (T,K) phase diagram
15
Microcanonical analysis
Mukamel, Ruffo, Schreiber (2005) Barre, Mukamel,
Ruffo (2001)
U number of broken bonds in a configuration
Number of microstates
16
sS/N , E/N , mM/N , uU/N
but
17
continuous transition
discontinuous transition
In a 1st order transition there is a
discontinuity in T, and thus there is a T region
which is not accessible.
18
m0
discontinuity in T
19
Microcanonical phase diagram
20
canonical
microcanonical
The two phase diagrams differ in the 1st order
region of the canonical diagram
21
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In general it is expected that whenever the
canonical transition is first order the
microcanonical and canonical ensembles differ
from each other.
23
Dynamics
Microcanonical Ising dynamics
Problem by making single spin flips it is
basically impossible to keep the energy fixed
for arbitrary K and J.
24
Microcanonical Ising dynamics Creutz (1983)
This is implemented by adding an auxiliary
variable, called a demon such that
systems energy demons energy
25
Creutz algorithm
  • Start with
  • Attempt to flip a spin
  • accept the move if energy decreases
  • and give the excess energy to the demon.
  • if energy increases, take the needed energy
    from the
  • demon. Reject the move if the demon does not
    have
  • the needed energy.

26
Yields the caloric curve T(E).
N400, K-0.35 E/N-0.2416
27
To second order in ED the demon distribution is
And it looks as if it is unstable for CV lt
0 (particularly near the microcanonical
tricritical point where CV vanishes). However
the distribution is stable as long as the
entropy increases with E (namely Tgt0) since the
next to leading term is of order 1/N.
28
Breaking of Ergodicity in Microcanonical
dynamics. Borgonovi, Celardo, Maianti, Pedersoli
(2004) Mukamel, Ruffo, Schreiber (2005).
Systems with short range interactions are defined
on a convex region of their extensive parameter
space.
If there are two microstates with magnetizations
M1 and M2 Then there are microstates
corresponding to any magnetization M1 lt M lt M2
.
29
This is not correct for systems with long range
interactions where the domain over which the
model is defined need not be convex.
30
Ising model with long and short range interactions
mM/N (N - N-)/N u U/N number of broken
bonds per site in a configuration
corresponding to isolated down spins -
- - -
Hence
31
K-0.4
32
Local dynamics cannot make the system cross from
one segment to another. Ergodicity is thus
broken even for a finite system.
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37
Breaking of Ergodicity at finite systems has to
do with the fact that the available range of m
dcreases as the energy is lowered.
Had it been
then the model could have moved between the right
and the left segments by lowering its energy with
a probability which is exponentially small in the
system size.
38
Time scales
Relaxation time of a state at a local maximum of
the entropy (metastable state)
s
39
critical radius above which droplet grows.
40
For systems with long range interactions the
relaxation time grows exponentially with the
system size. In this case there is no
geometry. The dynamics depends only on m. The
dynamics is that of a single particle moving in
a potential V(m)-s(m)
Griffiths et al (1966) (CE Ising) Antoni et al
(2004) (XY model) Chavanis et al (2003)
(Gravitational systems)
41
M0 is a local maximum of the entropy K-0.4
42
Relaxation of a state with a local minimum of the
entropy (thermodynamically unstable)
One would expect the relaxation time of the
m0 state to remain finite for large systems (as
is the case of systems with short range
interactions..
43
M0 is a minimum of the entropy K-0.25
44
One may understand this result by considering the
following Langevin equation for m
With D1/N
45
Fokker-Planck Equation
This is the dynamics of a particle moving in a
double well potential V(m)-s(m), with T1/N
starting at m0.
46
Taking for simplicity s(m)am2, agt0, the
problem becomes that of a particle moving in a
potential V(m) -am2 at temperature TD1/N
This equation yields at large t
47
Diverging time scales have been observed in a
number of systems with log range interactions.
The Hamiltonian Mean Field Model (HMF) (an XY
model with mean field ferromagnetic interactions)
There exists a class of quasistationary m0
states with relaxation time
Yamaguchi, Barre, Bouchet, Dauxois, Ruffo (2004)
48
Summary
Some general thermodynamic and dynamical
properties of system with long range interactions
have been considered. Negative specific heat in
microcanonical ensembles Canonical and
microcanonical ensembles need not be
equivalent whenever the canonical transition is
first order. Breaking of ergodicity in
microcanonical dynamics due to non-convexity of
the domain over which the model exists. Long
time scales, diverging with the system size. The
results were derived for mean field long range
interactions but they are expected to be valid
for algebraically decaying potentials.
49
  • S. Ruffo
  • J. Barre
  • N. Schreiber
  • Campa
  • A. Giansanti
  • K. Jain
  • F. Bouchet

50
Globular clusters are gravitationally bound
concentrations of approximately ten thousand to
one million stars, spread over a volume of
several tens to about 200 light years in
diameter.
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