1,498 research outputs found

    Stochastic quantization and holographic Wilsonian renormalization group

    Full text link
    We study relation between stochastic quantization and holographic Wilsonian renormalization group flow. Considering stochastic quantization of the boundary on-shell actions with the Dirichlet boundary condition for certain AdSAdS bulk gravity theories, we find that the radial flows of double trace deformations in the boundary effective actions are completely captured by stochastic time evolution with identification of the AdSAdS radial coordinate `rr' with the stochastic time 'tt' as r=tr=t. More precisely, we investigate Langevin dynamics and find an exact relation between radial flow of the double trace couplings and 2-point correlation functions in stochastic quantization. We also show that the radial evolution of double trace deformations in the boundary effective action and the stochastic time evolution of the Fokker-Planck action are the same. We demonstrate this relation with a couple of examples: (minimally coupled)massless scalar fields in AdS2AdS_2 and U(1) vector fields in AdS4AdS_4.Comment: 1+30 pages, a new subsection is added, references are adde

    Comment on "Quantum mechanics of smeared particles"

    Get PDF
    In a recent article, Sastry has proposed a quantum mechanics of smeared particles. We show that the effects induced by the modification of the Heisenberg algebra, proposed to take into account the delocalization of a particle defined via its Compton wavelength, are important enough to be excluded experimentally.Comment: 2 page

    The Patterns of High-Level Magnetic Activity Occurring on the Surface of V1285 Aql: The OPEA Model of Flares and DFT Models of Stellar Spots

    Full text link
    Statistically analyzing Johnson UBVR observations of V1285 Aql during the three observing seasons, both activity level and behavior of the star are discussed in respect to obtained results. We also discuss the out-of-flare variation due to rotational modulation. Eighty-three flares were detected in the U-band observations of season 2006 . First, depending on statistical analyses using the independent samples t-test, the flares were divided into two classes as the fast and the slow flares. According to the results of the test, there is a difference of about 73 s between the flare-equivalent durations of slow and fast flares. The difference should be the difference mentioned in the theoretical models. Second, using the one-phase exponential association function, the distribution of the flare-equivalent durations versus the flare total durations was modeled. Analyzing the model, some parameters such as plateau, half-life values, mean average of the flare-equivalent durations, maximum flare rise, and total duration times are derived. The plateau value, which is an indicator of the saturation level of white-light flares, was derived as 2.421{\pm}0.058 s in this model, while half-life is computed as 201 s. Analyses showed that observed maximum value of flare total duration is 4641 s, while observed maximum flare rise time is 1817 s. According to these results, although computed energies of the flares occurring on the surface of V1285 Aql are generally lower than those of other stars, the length of its flaring loop can be higher than those of more active stars.Comment: 44 pages, 10 figures, 5 tables, 2011PASP..123..659

    A branch-point approximant for the equation of state of hard spheres

    Full text link
    Using the first seven known virial coefficients and forcing it to possess two branch-point singularities, a new equation of state for the hard-sphere fluid is proposed. This equation of state predicts accurate values of the higher virial coefficients, a radius of convergence smaller than the close-packing value, and it is as accurate as the rescaled virial expansion and better than the Pad\'e [3/3] equations of state. Consequences regarding the convergence properties of the virial series and the use of similar equations of state for hard-core fluids in dd dimensions are also pointed out.Comment: 6 pages, 4 tables, 3 figures; v2: enlarged version, extension to other dimensionalities; v3: typos in references correcte

    Duality and ontology

    Get PDF
    A ‘duality’ is a formal mapping between the spaces of solutions of two empirically equivalent theories. In recent times, dualities have been found to be pervasive in string theory and quantum field theory. Naïvely interpreted, duality-related theories appear to make very different ontological claims about the world—differing in e.g. space-time structure, fundamental ontology, and mereological structure. In light of this, duality-related theories raise questions familiar from discussions of underdetermination in the philosophy of science: in the presence of dual theories, what is one to say about the ontology of the world? In this paper, we undertake a comprehensive and non-technical survey of the landscape of possible ontological interpretations of duality-related theories. We provide a significantly enriched and clarified taxonomy of options—several of which are novel to the literature

    The Intrinsically X-ray Weak Quasar PHL 1811. II. Optical and UV Spectra and Analysis

    Full text link
    This is the second of two papers reporting observations and analysis of the unusually bright (m_b=14.4), luminous (M_B=-25.5), nearby (z=0.192) narrow-line quasar PHL 1811. The first paper reported that PHL 1811 is intrinsically X-ray weak, and presented a spectral energy distribution (SED). Here we present HST STIS optical and UV spectra, and ground-based optical spectra. The optical and UV line emission is very unusual. There is no evidence for forbidden or semiforbidden lines. The near-UV spectrum is dominated by very strong FeII and FeIII, and unusual low-ionization lines such as NaID and CaII H&K are observed. High-ionization lines are very weak; CIV has an equivalent width of 6.6A, a factor of ~5 smaller than measured from quasar composite spectra. An unusual feature near 1200A can be deblended in terms of Ly\alpha, NV, SiII, and CIII* using the blueshifted CIV profile as a template. Photoionization modeling shows that the unusual line emission can be explained qualitatively by the unusually soft SED. Principally, a low gas temperature results in inefficient emission of collisionally excited lines, including the semiforbidden lines generally used as density diagnostics. The emission resembles that of high-density gas; in both cases this is a consequence of inefficient cooling. PHL 1811 is very unusual, but we note that quasar surveys are generally biased against finding similar objects.Comment: Accepted for publication in ApJS. Full resolution figures available here: http://www.nhn.ou.edu/~leighly/phl1811_paper1.pd

    On the relation between virial coefficients and the close-packing of hard disks and hard spheres

    Full text link
    The question of whether the known virial coefficients are enough to determine the packing fraction η\eta_\infty at which the fluid equation of state of a hard-sphere fluid diverges is addressed. It is found that the information derived from the direct Pad\'e approximants to the compressibility factor constructed with the virial coefficients is inconclusive. An alternative approach is proposed which makes use of the same virial coefficients and of the equation of state in a form where the packing fraction is explicitly given as a function of the pressure. The results of this approach both for hard-disk and hard-sphere fluids, which can straightforwardly accommodate higher virial coefficients when available, lends support to the conjecture that η\eta_\infty is equal to the maximum packing fraction corresponding to an ordered crystalline structure.Comment: 10 pages, 6 figures; v2: discussion about hard-square and hard-hexagon systems on a lattice added; five new reference

    Longitudinal study of functional flexibility in olfer physically active

    Full text link
    Un importante componente de la condición física es la flexibilidad, particularmente para las personas mayores que suelen sufrir un deterioro de la misma con los años. Con el objetivo de conocer como la flexibilidad evoluciona a lo largo del tiempo en un grupo de personas mayores físicamente activas, este estudio longitudinal ha evaluado 54 sujetos mayores de 65 años (17 hombres y 37 mujeres), que participaban con regularidad en clases de mantenimiento físico global realizadas dos veces a la semana en sesiones de 60 minutos. Para la medición de la flexibilidad fueron aplicados los tests chair sit and reach y back scratch, en cuatro momentos distintos en un periodo total de 12 meses. Los resultados muestran la evolución positiva de la flexibilidad de las zonas testadas en el grupo de mayores practicantes de actividad física al final de un año. Se concluye que para los participantes previamente activos del estudio la flexibilidad fue mantenida con el tiempo e inclusive mejorada en el periodo total propuesto al conservarse un estilo de vida activo a través de la práctica regular de actividad física de mantenimiento global de la condición físicaFlexibility is an important component of physical fitness, particularly in elderly people whose flexibility tend to deteriorate with the passing of time. The purpose of this longitudinal study was to determine how flexibility of older adults’ change over time. The control group consisted of 54 physically active adults (17 men and 37 women) all of which were 65 years and older. These adults participated in a 60 minute global fitness course, led by a trained instructor, twice a week. During the 12 month study, the subjects’ flexibility was measured at four different times through chair sit and reach and back scratch tests. The results show that the subjects who took part in this yearlong study, experienced positive results in flexibility in the areas tested. The results concluded that the subjects in the study that were previously engaged in regularly physical activity maintained and in some cases, improved flexibility through regular global fitness activit

    Exact solution for the energy density inside a one-dimensional non-static cavity with an arbitrary initial field state

    Full text link
    We study the exact solution for the energy density of a real massless scalar field in a two-dimensional spacetime, inside a non-static cavity with an arbitrary initial field state, taking into account the Neumann and Dirichlet boundary conditions. This work generalizes the exact solution proposed by Cole and Schieve in the context of the Dirichlet boundary condition and vacuum as the initial state. We investigate diagonal states, examining the vacuum and thermal field as particular cases. We also study non-diagonal initial field states, taking as examples the coherent and Schrodinger cat states.Comment: 10 pages, 8 figure
    corecore