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1.
We perform a new, recursive reduction of one-loop n-point rank R   tensor Feynman integrals [in short: (n,R)(n,R)-integrals] for n?6n?6 with R?nR?n by representing (n,R)(n,R)-integrals in terms of (n,R−1)(n,R1)- and (n−1,R−1)(n1,R1)-integrals. We use the known representation of tensor integrals in terms of scalar integrals in higher dimension, which are then reduced by recurrence relations to integrals in generic dimension. With a systematic application of metric tensor representations in terms of chords, and by decomposing and recombining these representations, a recursive reduction for the tensors is found. The procedure represents a compact, sequential algorithm for numerical evaluations of tensor Feynman integrals appearing in next-to-leading order contributions to massless and massive three- and four-particle production at LHC and ILC, as well as at meson factories.  相似文献   

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Based on the particular orderings introduced for the positive roots of finite-dimensional basic Lie superalgebras, we construct the explicit differential operator representations of the osp(2r|2n)osp(2r|2n) and osp(2r+1|2n)osp(2r+1|2n) superalgebras and the explicit free field realizations of the corresponding current superalgebras ospk(2r|2n)osp(2r|2n)k and ospk(2r+1|2n)osp(2r+1|2n)k at an arbitrary level k. The free field representations of the corresponding energy–momentum tensors and screening currents of the first kind are also presented.  相似文献   

3.
The η   production in the (n,n)(n,n) bottomonium transitions ?(n)→?(n?(n)?(n)η, is studied in the method used before for dipion heavy quarkonia transitions. The widths Γη(n,n)Γη(n,n) are calculated without fitting parameters for n=2,3,4,5n=2,3,4,5, n=1n=1. Resulting Γη(4,1)Γη(4,1) is found to be large in agreement with recent data. Multipole expansion method is shown to be inadequate for large size systems considered.  相似文献   

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We study two-dimensional nonlinear sigma models with target spaces being the complex super-Grassmannian manifolds, that is, coset supermanifolds G(m,p|n,q)≅U(m|n)/[U(p|q)⊗U(m−p|n−q)]G(m,p|n,q)U(m|n)/[U(p|q)U(mp|nq)] for 0?p?m0?p?m, 0?q?n0?q?n and 1?p+q1?p+q. The projective superspace CPm−1|nCPm1|n is a special case of p=1p=1, q=0q=0. For the two-dimensional Euclidean base space, a wide class of exact classical solutions (or harmonic maps) are constructed explicitly and elementarily in terms of Gramm–Schmidt orthonormalisation procedure starting from holomorphic bosonic and fermionic supervector input functions. The construction is a generalisation of the non-super-case published more than twenty years ago by one of the present authors.  相似文献   

8.
We study the six-dimensional dilaton gravity Yang black holes of Bergshoeff, Gibbons and Townsend, which carry (1,−1)(1,1) charge in SU(2)×SU(2)SU(2)×SU(2) gauge group. We find what values of the asymptotic parameters (mass and scalar charge) lead to a regular horizon, and show that there are no regular solutions with an extremal horizon.  相似文献   

9.
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   

10.
The idea that the existence of a consistent UV completion satisfying the fundamental axioms of local quantum field theory or string theory may impose positivity constraints on the couplings of the leading irrelevant operators in a low-energy effective field theory is critically discussed. Violation of these constraints implies superluminal propagation, in the sense that the low-frequency limit of the phase velocity vph(0)vph(0) exceeds c  . It is explained why causality is related not to vph(0)vph(0) but to the high-frequency limit vph(∞)vph() and how these are related by the Kramers–Kronig dispersion relation, depending on the sign of the imaginary part of the refractive index Imn(ω)Imn(ω) which is normally assumed positive. Superluminal propagation and its relation to UV completion is investigated in detail in three theories: QED in a background electromagnetic field, where the full dispersion relation for n(ω)n(ω) is evaluated numerically and the role of the null energy condition Tμνkμkν?0Tμνkμkν?0 is highlighted; QED in a background gravitational field, where examples of superluminal low-frequency phase velocities arise in violation of the positivity constraints; and light propagation in coupled laser–atom Λ  -systems exhibiting Raman gain lines with Imn(ω)<0Imn(ω)<0. The possibility that a negative Imn(ω)Imn(ω) must occur in quantum field theories involving gravity to avoid causality violation, and the implications for the relation of IR effective field theories to their UV completion, are carefully analysed.  相似文献   

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Lattice artifacts in the 2d O(n) non-linear σ  -model are expected to be of the form O(a2)O(a2), and hence it was (when first observed) disturbing that some quantities in the O(3)O(3) model with various actions show parametrically stronger cutoff dependence, apparently O(a)O(a), up to very large correlation lengths. In a previous letter Balog et al. (2009) [1] we described the solution to this puzzle. Based on the conventional framework of Symanzik's effective action, we showed that there are logarithmic corrections to the O(a2)O(a2) artifacts which are especially large (ln3aln3a) for n=3n=3 and that such artifacts are consistent with the data. In this paper we supply the technical details of this computation. Results of Monte Carlo simulations using various lattice actions for O(3)O(3) and O(4)O(4) are also presented.  相似文献   

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It is shown that the topological action for gravity in 2n  -dimensions can be obtained from the (2n+1)(2n+1)-dimensional Chern–Simons gravity genuinely invariant under the Poincaré group. The 2n  -dimensional topological gravity is described by the dynamics of the boundary of a (2n+1)(2n+1)-dimensional Chern–Simons gravity theory with suitable boundary conditions.  相似文献   

15.
A new treatment of the critical point of the two-dimensional interacting Bose gas is presented. In the lowest order approximation we obtain the critical temperature Tc≈2πn/[mlog(2π/mg)]Tc2πn/[mlog(2π/mg)], where n is the density, m the mass, and g the coupling. This result is based on a new formulation of interacting gases at finite density and temperature which is reminiscent of the thermodynamic Bethe ansatz in one dimension. In this formalism, the basic thermodynamic quantities are expressed in terms of a pseudo-energy. Consistent resummation of 2-body scattering leads to an integral equation for the pseudo-energy with a kernel based on the logarithm of the exact 2-body S-matrix.  相似文献   

16.
In this Letter, we consider lattice versions of the decomposition of the Yang–Mills field a la Cho–Faddeev–Niemi, which was extended by Kondo, Shinohara and Murakami in the continuum formulation. For the SU(N)SU(N) gauge group, we propose a set of defining equations for specifying the decomposition of the gauge link variable and solve them exactly without using the ansatz adopted in the previous studies for SU(2)SU(2) and SU(3)SU(3). As a result, we obtain the general form of the decomposition for SU(N)SU(N) gauge link variables and confirm the previous results obtained for SU(2)SU(2) and SU(3)SU(3).  相似文献   

17.
Gaussian and Chiral β  -Ensembles, which generalise well-known orthogonal (β=1β=1), unitary (β=2β=2), and symplectic (β=4β=4) ensembles of random Hermitian matrices, are considered. Averages are shown to satisfy duality relations like {β,N,n}⇔{4/β,n,N}{β,N,n}{4/β,n,N} for all β>0β>0, where N and n respectively denote the number of eigenvalues and products of characteristic polynomials. At the edge of the spectrum, matrix integrals of the Airy (Kontsevich) type are obtained. Consequences on the integral representation of the multiple orthogonal polynomials and the partition function of the formal one-matrix model are also discussed. Proofs rely on the theory of multivariate symmetric polynomials, especially Jack polynomials.  相似文献   

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Motivated by the necessity of discrete ZNZN symmetries in the MSSM to insure baryon stability, we study the origin of discrete gauge symmetries from open string sector U(1)U(1)?s in orientifolds based on rational conformal field theory. By means of an explicit construction, we find an integral basis for the couplings of axions and U(1)U(1) factors for all simple current MIPFs and orientifolds of all 168 Gepner models, a total of 32 990 distinct cases. We discuss how the presence of discrete symmetries surviving as a subgroup of broken U(1)U(1)?s can be derived using this basis. We apply this procedure to models with MSSM chiral spectrum, concretely to all known U(3)×U(2)×U(1)×U(1)U(3)×U(2)×U(1)×U(1) and U(3)×Sp(2)×U(1)×U(1)U(3)×Sp(2)×U(1)×U(1) configurations with chiral bi-fundamentals, but no chiral tensors, as well as some SU(5)SU(5) GUT models. We find examples of models with Z2Z2 (R-parity) and Z3Z3 symmetries that forbid certain B and/or L violating MSSM couplings. Their presence is however relatively rare, at the level of a few percent of all cases.  相似文献   

20.
We consider a classical toy model of a massive scalar field in 1+11+1 dimensions with a constant exponential expansion rate of space. The nonlinear theory under consideration supports approximate oscillon solutions, but they eventually decay due to their coupling to the expanding background. Although all the parameters of the theory and the oscillon energies are of order one in units of the scalar field mass m  , the oscillon lifetime is exponentially large in these natural units. For typical values of the parameters, we see oscillon lifetimes scaling approximately as τ∝exp(kE/m)/mτexp(kE/m)/m where E is the oscillon energy and the constant k   is on the order of 5 to 15 for expansion rates between H=0.02mH=0.02m and H=0.01mH=0.01m.  相似文献   

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