553,350 research outputs found

    Free energy and theta dependence of SU(N) gauge theories

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    We study the dependence of the free energy on the CP violating angle theta, in four-dimensional SU(N) gauge theories with N >= 3, and in the large-N limit. Using the Wilson lattice formulation for numerical simulations, we compute the first few terms of the expansion of the ground-state energy F(theta) around theta = 0, F(theta) - F(0) = A_2 theta^2 (1 + b_2 theta^2 + ...). Our results support Witten's conjecture: F(theta) - F(0) = A theta^2 + O(1/N) for theta < pi. We verify that the topological susceptibility has a nonzero large-N limit chi_infinity = 2A with corrections of O(1/N^2), in substantial agreement with the Witten-Veneziano formula which relates chi_infinity to the eta' mass. Furthermore, higher order terms in theta are suppressed; in particular, the O(theta^4) term b_2 (related to the eta' - eta' elastic scattering amplitude) turns out to be quite small: b_2 = -0.023(7) for N=3, and its absolute value decreases with increasing N, consistently with the expectation b_2 = O(1/N^2).Comment: 3 pages, talk presented at the conference Lattice2002(topology). v2: One reference has been updated, no further change

    CAID and Design Education

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    Measuring Product Semantics with a Computer

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    Reconstruction of the Extended Gauge Structure from Zâ€ČZ' Observables at Future Colliders

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    The discovery of a new neutral gauge boson Zâ€ČZ' with a mass in the TeV region would allow for determination of gauge couplings of the Zâ€ČZ' to ordinary quarks and leptons in a model independent way. We show that these couplings in turn would allow us to determine the nature of the extended gauge structure. As a prime example we study the E6E_6 group. In this case two discrete constraints on experimentally determined couplings have to be satisfied. If so, the couplings would then uniquely determine the two parameters, tan⁥ÎČ\tan \beta and ÎŽ\delta, which fully specify the nature of the Zâ€ČZ' within E6E_6. If the Zâ€ČZ' is part of the E6E_6 gauge structure, then for MZâ€Č=1M_{Z'}=1 TeV tan⁥ÎČ\tan \beta and ÎŽ\delta could be determined to around 10%10\% at the future colliders. The NLC provides a unique determination of the two constraints as well as of tan⁥ÎČ\tan \beta and ÎŽ\delta, though with slightly larger error bars than at the LHC. On the other hand, since the LHC primarily determines three out of four normalized couplings, it provides weaker constraints for the underlying gauge structure.Comment: 14 pages LaTeX using RevTeX and psfig.sty. TeX source and 3 PS figures, tarred, compressed and uuencoded; also available via anonymous ftp to ftp://dept.physics.upenn.edu/pub/Cvetic/UPR-636-T

    Discrete regularisation of localised kinetic terms

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    We investigate the behaviour of 5d models with general brane kinetic terms by discretising the extra dimension. We show that in the continuum limit the Kaluza-Klein masses and wave functions are in general nonanalytic in the coefficients of brane terms.Comment: Presented at the 7th DESY Workshop on Elementary Particle Theory ``Loops and Legs in Quantum Field Theory'', Zinnowitz, April 25-30, 200

    Digital Vellum

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    Non Singular Origin of the Universe and the Cosmological Constant Problem (CCP)

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    We consider a non singular origin for the Universe starting from an Einstein static Universe in the framework of a theory which uses two volume elements −gd4x\sqrt{-{g}}d^{4}x and Ίd4x\Phi d^{4}x, where Ί\Phi is a metric independent density, also curvature, curvature square terms, first order formalism and for scale invariance a dilaton field ϕ\phi are considered in the action. In the Einstein frame we also add a cosmological term that parametrizes the zero point fluctuations. The resulting effective potential for the dilaton contains two flat regions, for ϕ→∞\phi \rightarrow \infty relevant for the non singular origin of the Universe and ϕ→−∞\phi \rightarrow -\infty, describing our present Universe. Surprisingly, avoidance of singularities and stability as ϕ→∞\phi \rightarrow \infty imply a positive but small vacuum energy as ϕ→−∞\phi \rightarrow -\infty. Zero vacuum energy density for the present universe is the "threshold" for universe creation.Comment: awarded an honorable mention in the Gravity Research Foundation 2011 Awards for Essays in Gravitation for 201

    Electroweak constraints on new physics

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    We briefly review the limits on new interactions implied by electroweak precision data. Special attention is payed to the bounds on the Higgs boson mass. We also comment on the required cancellation among the new contributions to precisely measured electroweak observables in any Standard Model extension, if the new particles have to evade the indirect constraints on their couplings and masses but still remain at the LHC reach.Comment: Latex 4 pages, 1 table, 2 figures. To appear in the proceedings of 10th Hellenic School and Workshops on Elementary Particle Physics and Gravity (Corfu 2010), Corfu, Greece, Aug 29 - Sep 19, 201

    The Jackiw-Pi model and its symmetries

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    The non-Abelian gauge model proposed by Jackiw and Pi, which generates an even-parity mass term in three space-time dimensions, is revisited in this letter. All the symmetries of the model are collected and established by means of BRS invariance and Slavnov-Taylor identity. The path for the perturbatively quantization of the Jackiw-Pi model, through the algebraic method of renormalization, is presented.Comment: 5 page
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