Effective potential for the massless KPZ equation

被引:13
作者
Hochberg, D
Molina-París, C
Pérez-Mercader, J
Visser, M
机构
[1] Lab Astrofis Espacial & Fis Fundamental, Madrid 28080, Spain
[2] INTA, Ctr Astrobiol, Madrid 28850, Spain
[3] Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA
[4] Washington Univ, Dept Phys, St Louis, MO 63130 USA
关键词
effective potential; KPZ equation; dynamical symmetry breaking;
D O I
10.1016/S0378-4371(99)00611-1
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
In previous work we have developed a general method for casting a classical field theory subject to Gaussian noise (that is, a stochastic partial differential equation (SPDE)) into a functional integral formalism that exhibits many of the properties more commonly associated with quantum field theories (QFTs). In particular, we demonstrated how to derive the one-loop effective potential. In this paper we apply the formalism to a specific field theory of considerable interest, the massless KPZ equation (massless noisy Burgers equation), and analyze its behavior in the ultraviolet (short-distance) regime. When this field theory is subject to white noise we can calculate the one-loop effective potential and show that it is one-loop ultraviolet renormalizable in 1, 2, and 3 space dimensions, and fails to be ultraviolet renormalizable in higher dimensions. We show that the one-loop effective potential for the massless KPZ equation is closely related to that for lambda phi(4) QFT. In particular, we prove that the massless KPZ equation exhibits one-loop dynamical symmetry breaking (via an analog of the Coleman-Weinberg mechanism) in 1 and 2 space dimensions, and that this behavior does not persist in 3 space dimensions. (C) 2000 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:437 / 455
页数:19
相关论文
共 23 条
[1]  
Barabasi A. L., 1995, FRACTAL CONCEPTS SUR, DOI 10.1017/CBO9780511599798
[2]   Dynamical critical phenomena and large-scale structure of the Universe: The power spectrum for density fluctuations [J].
Barbero, JF ;
Dominguez, A ;
Goldman, T ;
PerezMercader, J .
EUROPHYSICS LETTERS, 1997, 38 (08) :637-642
[3]   STOCHASTIC FLUCTUATIONS AND STRUCTURE FORMATION IN THE UNIVERSE [J].
BERERA, A ;
FANG, LZ .
PHYSICAL REVIEW LETTERS, 1994, 72 (04) :458-461
[4]   FIELD-THEORY RENORMALIZATION AND CRITICAL DYNAMICS ABOVE T - HELIUM, ANTI-FERROMAGNETS, AND LIQUID-GAS SYSTEMS [J].
DEDOMINICIS, C ;
PELITI, L .
PHYSICAL REVIEW B, 1978, 18 (01) :353-376
[5]  
Domínguez A, 1999, ASTRON ASTROPHYS, V344, P27
[6]   2-LOOP RENORMALIZATION-GROUP ANALYSIS OF THE BURGERS-KARDAR-PARISI-ZHANG EQUATION [J].
FREY, E ;
TAUBER, UC .
PHYSICAL REVIEW E, 1994, 50 (02) :1024-1045
[7]  
Frisch U., 1995, TURBULENCE LEGACY AN
[8]   RENORMALIZATION-GROUP ANALYSIS FOR A GENERAL SOFTLY BROKEN SUPERSYMMETRIC GAUGE-THEORY [J].
GATO, B ;
LEON, J ;
PEREZMERCADER, J ;
QUIROS, M .
NUCLEAR PHYSICS B, 1985, 253 (02) :285-307
[9]   The galaxy-galaxy correlation function as an indicator of critical phenomena in cosmology [J].
Goldman, T ;
Hochberg, D ;
Laflamme, R ;
PerezMercader, J .
PHYSICS LETTERS A, 1996, 222 (03) :177-181
[10]   Gravitational critical phenomena in the realm of the galaxies and Ising magnets [J].
Hochberg, D ;
PerezMercader, J .
GENERAL RELATIVITY AND GRAVITATION, 1996, 28 (12) :1427-1432