Thermodynamics of abstract composition rules
description
Transcript of Thermodynamics of abstract composition rules
Thermodynamics of abstract composition rules
• Product, addition, logarithm
• Abstract composition rules, entropy formulas and
generalizations of the Boltzmann equation
• Application: Lattice SU2 with fluctuating temperature
T.S.Biró, MTA KFKI RMKI Budapest
Talk given at Zimányi School, Nov. 30. – Dec. 4. 2009, Budapest, Hungary
Thanks to: G.Purcsel, K.Ürmössy, Zs.Schram, P.Ván
Non-extensive Thermodynamics
The goal is to describe:
• statistical
• macro-equilibrium
• irreversible
properties of long-range correlated (entangled) systems
Non-extensive Thermodynamics
The goal is to describe:
• statistical
• macro-equilibrium
• irreversible
properties of long-range correlated (entangled) systems
Non-extensive Thermodynamics
Generalizations done (more or less):
• entropy formulas
• kinetic eq.-s: Boltzmann, Fokker-Planck, Langevin
• composition rules
Most important: fat tail distributions canonically
Applications (fits)
• galaxies, galaxy clusters• anomalous diffusion (Lévy flight)• turbulence, granular matter, viscous fingering• solar neutrinos, cosmic rays• plasma, glass, spin-glass• superfluid He, BE-condenstaion• hadron spectra• liquid crystals, microemulsions• finance models• tomography• lingustics, hydrology, cognitive sciences
Logarithm: Product Sum
additive extensive
Abstract Composition Rules
)y,x(hyx
EPL 84: 56003, 2008
Repeated Composition, large-N
Scaling law for large-N
)0,x(hdy
dx :N
)0,x(hyxx
)0,x(h)y,x(hxx
yy,0x),y,x(hx
2
1n2n1nn
1nn1n1nn
N
1nn0n1nn
Formal Logarithm
Asymptotic rules are associative and attractors among all rules…
Asymptotic rules are associative
).),,((
))()()((
))()(()(
)))()((,()),(,(
1
11
1
zyx
zLyLxLL
zLyLLLxLL
zLyLLxzyx
Associative rules are asymptotic
),(),(
)0(
)(
)0(
)()(
)(
)0(
))0,((
)0()0,(
)()(
)()()),((
0
2
yxhyx
xdz
zxL
xxhxh
yyhh
yxyxh
x
Scaled Formal Logarithm
xxL
axLa
xL
axLa
xL
LL
a
a
)(
)(1
)(
)(1
)(
0)0(,1)0(
0
11
Deformed logarithm
)(ln)/1(ln
))(ln()(ln 1
xx
xLx
aa
aa
Deformed exponential
)()(/1
))(exp()(
xexe
xLxe
aa
aa
Entropy formulas, distributions
Boltzmann – GibbsRényiTsallisKaniadakis …
EPJ A 40: 325, 2009
Entropy formulas from composition rules
Joint probability = marginal prob. * conditional prob.
The last line is for a subset
Entropy formulas from composition rules
Equiprobability: p = 1 / N
Nontrivial composition rule at statistical independence
Entropy formulas from composition rules
ppLp
L
bLaLabL
def
1ln)ln()(
ln
))(())(())((
1
1. Thermodynamical limit: deformed log
Entropy maximum at fixed energy
)()(
)()(
)(
)(
fixed ))()((
max))()((
22
2
2
11
1
1
1221
1
1221
1
ESEX
SYES
EX
SY
EEXEXX
SSYSYY
Generalized kinetic theory
Boltzmann algorithm: pairwise combination + separation
With additive composition rule at independence:
Such rules generate exponential distribution
Boltzmann algorithm: pairwise combination + separation
With associative composition rule at independence:
Such rules generate ‘exponential of the formal logarithm’ distribution
Generalized Stoßzahlansatz
)(ln)(ln
)(
0
234123412341
jaiaaijffeG
Fp
GGwfDF
General H theorem
function rising monotonica
)(G iff 0
))((4
1
)()(
))((
ij
1234341243211234
11
0
jiS
GGw
fDFFS
fFp
pS
General H theorem: entropy density formula
df)f(ln)f(F)f(
)f(ln))f(F(
2)G(ln)G(
a
a
a
Detailed balance: G = G 12 34
Examples for composition rules
Example: Gibbs-Boltzmann
WlnkSW/1ffor
flnfS
)E(eZ
1f
x)x(L
1)0,x(h,yx)y,x(h
eq
2
Example: Rényi, Tsallis
ényi Rln1
1)(
Tsallis )(1
)1(1
),1ln(1
)(
1)0,(,),(
11
/
2
q
nona
aqa
non
a
eqa
fq
SL
ffa
S
aEZ
faxa
xL
axxhaxyyxyxh
Example: Einstein
),(),(
)tanh()(
)tanh(Ar)(
1)0,(
1),(
1
22
2
2
yxhyxc
zczL
c
xcxL
cxxh
cxy
yxyxh
c
c
Important example: product class
axyyxyxa
ezL
axa
xL
axxGxh
xyGyxyxh
az
c
c
),(
1)(
)1ln(1
)(
1)0(1)0,(
)(),(
1
2
Important example: product class
axyyxyxa
ezL
axa
xL
axxGxh
xyGyxyxh
az
c
c
),(
1)(
)1ln(1
)(
1)0(1)0,(
)(),(
1
2
QCD is
like
this
!
Relativistic energy composition
Relativistic energy composition
)cos1(EE2Q
)EE()pp(Q
)Q(UEE)E,E(h
21
2
2
21
2
21
2
2
2121
( high-energy limit: mass ≈ 0 )
Asymptotic rule for m=0
)0(U2/
eq
2
E)0(U21Z
1f
xy)0(U2yx)y,x(
)0(Ux21)0,x(h
Physics background:
q > 1
q < 1
Q²
α
Simulation using non-additive rule
Non-extensive Boltzmann Equation
(NEBE) :
• Rényi-Tsallis energy addition rule
• random momenta accordingly
• pairwise collisions repeated
• momentum distribution collected
with Gábor PurcselPRL 95: 162302, 2005
Evolution in NEBE phase space
Stationary energy distributions in NEBE program
x + y x + y + 2 x y
Thermal equilibration in NEBE program
Scaling variable E or X(E)?Károly Ürmössy
Scaling variable E or X(E)?Károly Ürmössy
Microscopic theory in non-extensive approach: questions, projects, ...
• Ideal gas with deformed exponentials
• Boltzmann and Bose distribution
• Fermi distribution: ptl – hole effect
• Thermal field theory with stohastic temperature
• Lattice SU(2) with Gamma * Metropolis method
As if temperature fluctuated…
• EulerGamma Boltzmann = Tsallis
• EulerGamma Poisson = Negative Binomial
max: 1 – 1/c, mean: 1, spread: 1 / √ c
Euler - Gamma distribution
Tsallis lattice EOS
Tamás S. Bíró (KFKI RMKI Budapest) and
Zsolt Schram (DTP ATOMKI Debrecen)
• Lattice action with
superstatistics
• Ideal gas with power-law tails
• Numerical results on EOS
Lattice theory
A =
DU dt w (t) e t A(U) -S(t,U)c
DU dt w (t) e -S(t,U)c
v
Expectation values of observables:
t = a / a asymmetry parametert s
Action: S(t,U) = a(U) t + b(U) / t
Su2 Yang-Mills eos on the lattice with Euler-Gamma distributed inverse temperature: Effective action method
preliminary
with Zsolt Schram (work in progress)
Method: EulerGamma * Metropolis
• asymmetry thrown from Euler-Gamma
• at each Monte Carlo step / only after a while
• at each link update / only for the whole lattice
• meaning local / global fluctuation in space
• c = 1024 for checking usual su2
• c = 5.5 for genuine quark matter
Ratio
e / T4
(e-3p) / T4
Ideal Tsallis-Bose gas
For c = 5.5 we have 1 / a = 4.5 and e ≈ 4 e_0
Summary
• Non-extensive thermodynamics is not only
derivable from composition rules, but it is
realized by QCD interactions in the high-
energy limit and can be seen in heavy-ion
collisions!
Topical Review Issue of EPJ A