User talk:Nicole/PubMan reference integration

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@article{escidoc:39322, title = "The inner Cauchy horizon of axisymmetric and stationary black holes with surrounding matter", author = "Ansorg, Marcus and Hennig, Jörg", issn = "0264-9381", year = "2008", abstract = "We investigate the interior of regular axisymmetric and stationary black holes surrounded by matter and find that for non-vanishing angular momentum of the black hole the spacetime can always be extended regularly up to and including an inner Cauchy horizon. We provide an explicit relation for the regular metric at the inner Cauchy horizon in terms of that at the event horizon. As a consequence, we obtain the universal equality (8\piJ)2 = A+Aâˆ’ where J is the black hole's angular momentum and Aâˆ’ and A+ denote the horizon areas of inner Cauchy and event horizons, respectively. We also find that in the limit J \rightarrow 0 the inner Cauchy horizon becomes singular.", keywords = "gr-qc", journal = "Classical and quantum gravity", volume = "25", issue = "22", }

@article{escidoc:39189, title = "Boosting Nearest-Neighbour to Long-Range Integrable Spin Chains", author = "Bargheer, Till and Beisert, Niklas and Loebbert, Florian", language = "en", issn = "1742-5468", year = "2008", abstract = "We present an integrability-preserving recursion relation for the explicit construction of long-range spin chain Hamiltonians. These chains are generalizations of the Haldane-Shastry and Inozemtsev models and they play an important role in recent advances in string/gauge duality. The method is based on arbitrary nearest-neighbour integrable spin chains and it sheds light on the moduli space of deformation parameters. We also derive the closed chain asymptotic Bethe equations.", keywords = "hep-th cond-mat.stat-mech math-ph math.MP", journal = "Journal of Statistical Mechanics: Theory and Experiment", volume = "08", }

@article{escidoc:39314, title = "Probing non-Riemannian spacetime geometry", author = "Puetzfeld, Dirk and Obukhov, Yuri N.", issn = "0375-9601", year = "2008", abstract = "The equations of motion for matter in non-Riemannian spacetimes are derived via a multipole method. It is found that only test bodies with microstructure couple to the non-Riemannian spacetime geometry. Consequently it is impossible to detect spacetime torsion with the satellite experiment Gravity Probe B, contrary to some recent claims in the literature.", keywords = "gr-qc astro-ph", journal = "Physics Letters A", }

@article{escidoc:39320, title = "Neutrinos, Axions and Conformal Symmetry", author = "Meissner, Krzysztof A. and Nicolai, Hermann", language = "en", issn = "1434-6052", year = "2008", date = "2008-10-22", abstract = "We demonstrate that radiative breaking of conformal symmetry (and simultaneously electroweak symmetry) in the standard model with right-chiral neutrinos and a minimally enlarged scalar sector induces spontaneous breaking of lepton number symmetry, which naturally gives rise to an axion-like particle with some unusual features. The couplings of this â€˜axionâ€™ to standard model particles, in particular photons and gluons, are entirely determined (and computable) via the conformal anomaly, and their smallness turns out to be directly related to the smallness of the masses of the light neutrinos.", keywords = "hep-th hep-ph", journal = "European Physical Journal C", }

@article{escidoc:39265, title = "Hyperboloidal evolution with the Einstein equations", author = "Zenginoglu, Anil", language = "en", issn = "0264-9381", year = "2008", abstract = "We consider an approach to the hyperboloidal evolution problem based on the Einstein equations written for a rescaled metric. It is shown that a conformal scale factor can be freely prescribed a priori in terms of coordinates in a well-posed hyperboloidal initial value problem such that the location of null infinity is independent of the time coordinate. With an appropriate choice of a single gauge source function each of the formally singular conformal source terms in the equations attains a regular limit at null infinity. The suggested approach could be beneficial in numerical relativity for both wave extraction and outer boundary treatment.", keywords = "gr-qc", journal = "Classical and Quantum Gravity", volume = "25", issue = "19", }

@article{escidoc:39277, title = "Improved search for galactic white dwarf binaries in Mock LISA Data Challenge 1B using an F-statistic template bank", author = "Whelan, John T. and Prix, Reinhard and Khurana, Deepak", issn = "0264-9381", year = "2008", abstract = "We report on our F-statistic search for white-dwarf binary signals in the Mock LISA Data Challenge 1B (MLDC1B). We focus in particular on the improvements in our search pipeline since MLDC1, namely refinements in the search pipeline and the use of a more accurate detector response (rigid adiabatic approximation). The search method employs a hierarchical template-grid based exploration of the parameter space, using a coincidence step to distinguish between primary (``true) and secondary maxima, followed by a final (multi-TDI) ``zoom stage to provide an accurate parameter estimation of the final candidates.", keywords = "gr-qc", journal = "Classical and quantum gravity", volume = "25", issue = "18", }

@article{escidoc:39328, title = "Double optical spring enhancement for gravitational wave detectors", author = "Rehbein, Henning and MÃ¼ller-Ebhardt, Helge and Somiya, Kentaro and Danilishin, Stefan L. and Schnabel, Roman and Danzmann, Karsten and Chen, Yanbei", language = "en", issn = "1089-4918", year = "2008", abstract = "Currently planned second-generation gravitational-wave laser interferometers such as Advanced LIGO exploit the extensively investigated signal-recycling technique. Candidate Advanced LIGO configurations are usually designed to have two resonances within the detection band, around which the sensitivity is enhanced: a stable optical resonance and an unstable optomechanical resonanceâ€”which is upshifted from the pendulum frequency due to the so-called optical-spring effect. As an alternative to a feedback control system, we propose an all-optical stabilization scheme, in which a second optical spring is employed, and the test mass is trapped by a stable ponderomotive potential well induced by two carrier light fields whose detunings have opposite signs. The double optical spring also brings additional flexibility in reshaping the noise spectral density and optimizing toward specific gravitational-wave sources. The presented scheme can be extended easily to a multi-optical-spring system that allows further optimization.", keywords = "gr-qc", journal = "Physical Review D.", volume = "78", issue = "6", }

@article{escidoc:37245, title = "A hyperboloidal study of tail decay rates for scalar and Yang-Mills fields", author = "Zenginoglu, Anil", language = "en", issn = "0264-9381", year = "2008", abstract = "We investigate the asymptotic behavior of spherically symmetric solutions to scalar wave and Yang-Mills equations on a Schwarzschild background. The studies demonstrate the astrophysical relevance of null infinity in predicting radiation signals for gravitational wave detectors and show how test fields on unbounded domains in black hole spacetimes can be simulated conveniently by numerically solving hyperboloidal initial value problems.", keywords = "gr-qc", journal = "Classical and Quantum Gravity", volume = "25", issue = "17", }

@article{escidoc:33005, title = "The Weinberg-Witten theorem on massless particles: an essay", author = "Loebbert, Florian", issn = "1521-3889", year = "2008", date = "2008-09", abstract = "In this essay we deal with the Weinberg-Witten theorem [1] which imposes limitations on massless particles. First we motivate a classification of massless particles given by the Poincar\acute\{\\{{\\}\}e{\\}\} group as the symmetry group of Minkowski spacetime. We then use the fundamental structure of the background in the form of Poincar\acute\{\\{{\\}\}e{\\}\} covariance to derive restrictions on charged massless particles known as the Weinberg-Witten theorem. We address possible misunderstandings in the proof of this theorem motivated by several papers on this topic. In the last section the consequences of the theorem are discussed. We treat it in the context of known particles and as a constraint for emergent theories.", keywords = "", journal = "Annalen der Physik", volume = "17", issue = "9-10", }

@article{escidoc:28174, title = "Complete Six-Gluon Disk Amplitude in Superstring Theory", author = "Stieberger, Stephan and Taylor, Tomasz R.", issn = "0550-3213", year = "2008", date = "2008-09", abstract = "We evaluate all next-to-maximal helicity violating (NMHV) six-gluon amplitudes in type I open superstring theory in four dimensions, at the disk level, to all orders in alpha'. Although the computation utilizes supersymmetric Ward identities, the result holds for all compactifications, even for those that break supersymmetry and is completely model-independent. Together with the maximally helicity violating (MHV) amplitudes presented in the previous work, our results provide the complete six-gluon disk amplitude.", keywords = "", journal = "Nuclear Physics B", volume = "801", issue = "1-2", }

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