首页 | 本学科首页   官方微博 | 高级检索  
相似文献
 共查询到20条相似文献,搜索用时 15 毫秒
1.
We present a family of nonrelativistic Yang–Mills gauge theories in D+1D+1 dimensions whose free-field limit exhibits quantum critical behavior with gapless excitations and dynamical critical exponent z=2z=2. The ground state wavefunction is intimately related to the partition function of relativistic Yang–Mills in D   dimensions. The gauge couplings exhibit logarithmic scaling and asymptotic freedom in the upper critical spacetime dimension, equal to 4+14+1. The theories can be deformed in the infrared by a relevant operator that restores Poincaré invariance as an accidental symmetry. In the large-N limit, our nonrelativistic gauge theories can be expected to have weakly curved gravity duals.  相似文献   

2.
We report on the presence of new axially symmetric monopoles, antimonopoles and vortex-rings solutions of the SU(2)×U(1) Weinberg–Salam model of electromagnetic and weak interactions. When the ??-winding number n=1n=1, and 2, the configurations are monopole–antimonopole pair (MAP) and monopole–antimonopole chain (MAC) with poles of alternating sign magnetic charge arranged along the zz-axis. Vortex-rings start to appear from the MAP and MAC configurations when the winding number n=3n=3. The MAP configurations possess zero net magnetic charge whereas the MAC configurations possess net magnetic charge of 4πn/e4πn/e.  相似文献   

3.
4.
The large-n expansion is applied to the calculation of thermal critical exponents describing the critical behavior of spatially anisotropic d-dimensional systems at m  -axial Lifshitz points. We derive the leading non-trivial 1/n1/n correction for the perpendicular correlation-length exponent νL2νL2 and hence several related thermal exponents to order O(1/n)O(1/n). The results are consistent with known large-n expansions for d  -dimensional critical points and isotropic Lifshitz points, as well as with the second-order epsilon expansion about the upper critical dimension d?=4+m/2d?=4+m/2 for generic m∈[0,d]m[0,d]. Analytical results are given for the special case d=4d=4, m=1m=1. For uniaxial Lifshitz points in three dimensions, 1/n1/n coefficients are calculated numerically. The estimates of critical exponents at d=3d=3, m=1m=1 and n=3n=3 are discussed.  相似文献   

5.
We study a renormalized coupling g and mass m   in four-dimensional ?4?4 theory on tori with finite size z=mLz=mL. Precise numerical values close to the continuum limit are reported for z=1,2,4z=1,2,4, based on Monte Carlo simulations performed in the equivalent all-order strong coupling reformulation. Ordinary renormalized perturbation theory is found to work marginally at z=2z=2 and to fail at z=1z=1. By exactly integrating over the constant field mode we set up a renormalized expansion in z and compute three nontrivial orders. These results reasonably agree with the numerical data at small z. In the new expansion, the universal continuum limit exists as expected from multiplicative renormalizability. The triviality scenario is corroborated with significant precision.  相似文献   

6.
We introduce a network evolution process motivated by the network of citations in the scientific literature. In each iteration of the process a node is born and directed links are created from the new node to a set of target nodes already in the network. This set includes mm “ambassador” nodes and ll of each ambassador’s descendants where mm and ll are random variables selected from any choice of distributions plpl and qmqm. The process mimics the tendency of authors to cite varying numbers of papers included in the bibliographies of the other papers they cite. We show that the degree distributions of the networks generated after a large number of iterations are scale-free and derive an expression for the power-law exponent. In a particular case of the model where the number of ambassadors is always the constant mm and the number of selected descendants from each ambassador is the constant ll, the power-law exponent is (2l+1)/l(2l+1)/l. For this example we derive expressions for the degree distribution and clustering coefficient in terms of ll and mm. We conclude that the proposed model can be tuned to have the same power law exponent and clustering coefficient of a broad range of the scale-free distributions that have been studied empirically.  相似文献   

7.
Recently, Ho?ava has proposed a renormalizable theory of gravity with critical exponent z=3z=3 in the UV. This proposal might imply that the scale invariant primordial perturbation can be generated in any expansion of early universe with a∼tnatn and n>1/3n>1/3, which, in this Letter, will be confirmed by solving the motion equation of perturbation mode on super sound horizon scale for any background evolution of early universe. It is found that if enough efolding number of primordial perturbation suitable for observable universe is required, then n?1n?1 needs to be satisfied, unless the scale of UV regime is quite low. However, the possible UV completeness of HL gravity helps to relax this bound.  相似文献   

8.
We present a Markov-chain Monte Carlo algorithm of worm   type that correctly simulates the O(n)O(n) loop model on any (finite and connected) bipartite cubic graph, for any real n>0n>0, and any edge weight, including the fully-packed limit of infinite edge weight. Furthermore, we prove rigorously that the algorithm is ergodic and has the correct stationary distribution. We emphasize that by using known exact mappings when n=2n=2, this algorithm can be used to simulate a number of zero-temperature Potts antiferromagnets for which the Wang–Swendsen–Kotecký cluster algorithm is non-ergodic, including the 3-state model on the kagome lattice and the 4-state model on the triangular lattice. We then use this worm algorithm to perform a systematic study of the honeycomb-lattice loop model as a function of n?2n?2, on the critical line and in the densely-packed and fully-packed phases. By comparing our numerical results with Coulomb gas theory, we identify a set of exact expressions for scaling exponents governing some fundamental geometric and dynamic observables. In particular, we show that for all n?2n?2, the scaling of a certain return time in the worm dynamics is governed by the magnetic dimension of the loop model, thus providing a concrete dynamical interpretation of this exponent. The case n>2n>2 is also considered, and we confirm the existence of a phase transition in the 3-state Potts universality class that was recently observed via numerical transfer matrix calculations.  相似文献   

9.
We demonstrate the emergence of non-Abelian fusion rules for excitations of a two dimensional lattice model built out of Abelian degrees of freedom. It can be considered as an extension of the usual toric code model on a two dimensional lattice augmented with matter fields. It consists of the usual C(Zp)C(Zp) gauge degrees of freedom living on the links together with matter degrees of freedom living on the vertices. The matter part is described by a nn dimensional vector space which we call HnHn. The ZpZp gauge particles act on the vertex particles and thus HnHn can be thought of as a C(Zp)C(Zp) module. An exactly solvable model is built with operators acting in this Hilbert space. The vertex excitations for this model are studied and shown to obey non-Abelian fusion rules. We will show this for specific values of nn and pp, though we believe this feature holds for all n>pn>p. We will see that non-Abelian anyons of the quantum double of C(S3)C(S3) are obtained as part of the vertex excitations of the model with n=6n=6 and p=3p=3. Ising anyons are obtained in the model with n=4n=4 and p=2p=2. The n=3n=3 and p=2p=2 case is also worked out as this is the simplest model exhibiting non-Abelian fusion rules. Another common feature shared by these models is that the ground states have a higher symmetry than ZpZp. This makes them possible candidates for realizing quantum computation.  相似文献   

10.
A complex symplectic structure on a Lie algebra hh is an integrable complex structure JJ with a closed non-degenerate (2,0)(2,0)-form. It is determined by JJ and the real part ΩΩ of the (2,0)(2,0)-form. Suppose that hh is a semi-direct product g?Vg?V, and both gg and VV are Lagrangian with respect to ΩΩ and totally real with respect to JJ. This note shows that g?Vg?V is its own weak mirror image in the sense that the associated differential Gerstenhaber algebras controlling the extended deformations of ΩΩ and JJ are isomorphic.  相似文献   

11.
The Alday–Maldacena solution, relevant to the n=4n=4 gluon amplitude in N=4N=4 SYM at strong coupling, was recently identified as a minimum of the regularized action in the moduli space of solutions of the AdS5AdS5σ  -model equations of motion. Analogous solutions of the Nambu–Goto equations for the n=4n=4 case are presented and shown to form (modulo the reparametrization group) an equally large but different moduli space, with the Alday–Maldacena solution at the intersection of the σ  -model and Nambu–Goto moduli spaces. We comment upon the possible form of the regularized action for n=5n=5. A function of moduli parameters zaza is written, whose minimum reproduces the BDDK one-loop five-gluon amplitude. This function may thus be considered as some kind of Legendre transform of the BDDK formula and has its own value independently of the Alday–Maldacena approach.  相似文献   

12.
In this study which is the continuation of the first part (Pavlos et al. 2012) [1], the nonlinear analysis of the solar flares index is embedded in the non-extensive statistical theory of Tsallis (1988) [3]. The qq-triplet of Tsallis, as well as the correlation dimension and the Lyapunov exponent spectrum were estimated for the singular value decomposition (SVD) components of the solar flares timeseries. Also the multifractal scaling exponent spectrum f(a)f(a), the generalized Renyi dimension spectrum D(q)D(q) and the spectrum J(p)J(p) of the structure function exponents were estimated experimentally and theoretically by using theqq-entropy principle included in Tsallis non-extensive statistical theory, following Arimitsu and Arimitsu (2000) [25]. Our analysis showed clearly the following: (a) a phase transition process in the solar flare dynamics from a high dimensional non-Gaussian self-organized critical (SOC) state to a low dimensional also non-Gaussian chaotic state, (b) strong intermittent solar corona turbulence and an anomalous (multifractal) diffusion solar corona process, which is strengthened as the solar corona dynamics makes a phase transition to low dimensional chaos, (c) faithful agreement of Tsallis non-equilibrium statistical theory with the experimental estimations of the functions: (i) non-Gaussian probability distribution function P(x)P(x), (ii) f(a)f(a) and D(q)D(q), and (iii) J(p)J(p) for the solar flares timeseries and its underlying non-equilibrium solar dynamics, and (d) the solar flare dynamical profile is revealed similar to the dynamical profile of the solar corona zone as far as the phase transition process from self-organized criticality (SOC) to chaos state. However the solar low corona (solar flare) dynamical characteristics can be clearly discriminated from the dynamical characteristics of the solar convection zone.  相似文献   

13.
Investigating long-range correlation by the Hurst exponent, HH, is crucial in the study of time series. Recently, empirical-mode-decomposition-based arbitrary-order Hilbert spectral analysis (EMD-HSA) has been proposed to numerically obtain without proof a scaling relationship, generated from the amplitude–frequency distribution, related to HH. We propose a formalism to empirically study EMD-HSA, to deduce its scaling exponent ξ(q)ξ(q) from the perspective of EMD-based arbitrary-order Hilbert marginal spectrum (EMD-HMS), and to numerically compare the results with the expected HH. EMD-HSA and EMD-HMS experiments show that, by incompletely removing (quasi-)periodic trends, the sunspot series should have an HH value around 0.12.  相似文献   

14.
Geometrical characterizations are given for the tensor R⋅SRS, where SS is the Ricci tensor   of a (semi-)Riemannian manifold (M,g)(M,g) and RR denotes the curvature operator   acting on SS as a derivation, and of the Ricci Tachibana tensor  g⋅SgS, where the natural metrical operator  gg also acts as a derivation on SS. As a combination, the Ricci curvatures   associated with directions on MM, of which the isotropy determines that MM is Einstein, are extended to the Ricci curvatures of Deszcz   associated with directions and planes on MM, and of which the isotropy determines that MM is Ricci pseudo-symmetric in the sense of Deszcz.  相似文献   

15.
The effects of single C-chain on the stability, structural and electronic properties of zigzag BN nanoribbons (ZBNNRs) were investigated by first-principles calculations. C-chain was expected to dope at B-edge for all the ribbon widths NzNz considered. The band gaps of C-chain doped NzNz-ZBNNR are narrower than that of perfect ZBNNR due to new localized states induced by C-chain. The band gaps of NzNz-ZBNNR-C(n  ) are direct except for the case of C-chain position n=2n=2. Band gaps of BN nanoribbons are tunable by C-chain and its position n, which may endow the potential applications of BNNR in electronics.  相似文献   

16.
The setting is an ergodic dynamical system (X,μ)(X,μ) whose points are themselves uniformly discrete point sets ΛΛ in some space RdRd and whose group action is that of translation of these point sets by the vectors of RdRd. Steven Dworkin’s argument relates the diffraction of the typical point sets comprising XX to the dynamical spectrum of XX. In this paper we look more deeply at this relationship, particularly in the context of point processes.  相似文献   

17.
The cross sections for (n,x)(n,x) reactions with Ge isotopes were measured at (dt) neutron energies around 14 MeV with the activation technique using metal discs of natural composition. Calculations of detector efficiency, incident neutron spectrum and correction factors were performed with the Monte Carlo technique (MCNP4C code). Cross sections data are presented for 70Ge(n,2nn,2n)69Ge, 74Ge(n,αn,α)71mZn, 76Ge(n,2nn,2n)75(m + g)Ge, 70Ge(n,pn,p)70Ga and 72Ge(n,2nn,2n)71gGe reactions. The cross section results for 72Ge(n,2nn,2n)71gGe reaction were reported for the first time. Some other cross sections were obtained with higher precision, including the 70Ge(n,pn,p)70Ga reaction. Theoretical calculations of excitation functions were performed with the TALYS-1.0 code and compared with the experimental cross section values. Data were included in the EXFOR database.  相似文献   

18.
In this Letter, some relations between the topological parameter d   and concurrences of the projective entangled states have been presented. It is shown that for the case with d=nd=n, all the projective entangled states of two n  -dimensional quantum systems are the maximally entangled states (i.e. C=1C=1). And for another case with d≠ndn, C   both approach 0 when d→+∞d+ for n=2n=2 and 3. Then we study the thermal entanglement and the entanglement sudden death (ESD) for a kind of Yang–Baxter Hamiltonian. It is found that the parameter d   influences not only the critical temperature TcTc but also the maximum entanglement value that the system can arrive at. And we also find that the parameter d has a great influence on the ESD.  相似文献   

19.
We present a Markov-chain Monte Carlo algorithm of worm   type that correctly simulates the fully-packed loop model with n=1n=1 on the honeycomb lattice, and we prove that it is ergodic and has uniform stationary distribution. The honeycomb-lattice fully-packed loop model with n=1n=1 is equivalent to the zero-temperature triangular-lattice antiferromagnetic Ising model, which is fully frustrated and notoriously difficult to simulate. We test this worm algorithm numerically and estimate the dynamic exponent zexp=0.515(8)zexp=0.515(8). We also measure several static quantities of interest, including loop-length and face-size moments. It appears numerically that the face-size moments are governed by the magnetic dimension for percolation.  相似文献   

20.
Suppose that the sphere SnSn has initially a homogeneous distribution of mass and let GG be the Lie group of orientation preserving projective diffeomorphisms of SnSn. A projective motion of the sphere, that is, a smooth curve in GG, is called force free if it is a critical point of the kinetic energy functional. We find explicit examples of force free projective motions of SnSn and, more generally, examples of subgroups HH of GG such that a force free motion initially tangent to HH remains in HH for all time (in contrast with the previously studied case for conformal motions, this property does not hold for H=SOn+1H=SOn+1). The main tool is a Riemannian metric on GG, which turns out to be not complete (in particular not invariant, as happens with non-rigid motions), given by the kinetic energy.  相似文献   

设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号