6,871 research outputs found

    The Fundamental Plane of Gamma-ray Globular Clusters

    Get PDF
    We have investigated the properties of a group of γ\gamma-ray emitting globular clusters (GCs) which have recently been uncovered in our Galaxy. By correlating the observed γ\gamma-ray luminosities LγL_{\gamma} with various cluster properties, we probe the origin of the high energy photons from these GCs. We report LγL_{\gamma} is positively correlated with the encounter rate Γc\Gamma_{c} and the metalicity [Fe/H]\left[{\rm Fe/H}\right] which place an intimate link between the gamma-ray emission and the millisecond pulsar population. We also find a tendency that LγL_{\gamma} increase with the energy densities of the soft photon at the cluster location. Furthermore, the two-dimensional regression analysis suggests that LγL_{\gamma}, soft photon densities, and Γc\Gamma_{c}/[Fe/H]\left[{\rm Fe/H}\right] possibly span fundamental planes which potentially provide better predictions for the γ\gamma-ray properties of GCs.Comment: 17 pages, 4 figures, 3 tables, published in Ap

    Further investigation on chaos of real digital filters

    Get PDF
    This Letter displays, via the numerical simulation of a real digital filter, that a finite-state machine may behave in a near-chaotic way even when its corresponding infinite-state machine does not exhibit chaotic behavior

    Observing two dark accelerators around the Galactic Centre with Fermi Large Area Telescope

    Get PDF
    We report the results from a detailed γ\gamma-ray investigation in the field of two "dark accelerators", HESS J1745-303 and HESS J1741-302, with 6.96.9 years of data obtained by the Fermi Large Area Telescope. For HESS J1745-303, we found that its MeV-GeV emission is mainly originated from the "Region A" of the TeV feature. Its γ\gamma-ray spectrum can be modeled with a single power-law with a photon index of Γ2.5\Gamma\sim2.5 from few hundreds MeV to TeV. Moreover, an elongated feature, which extends from "Region A" toward northwest for 1.3\sim1.3^{\circ}, is discovered for the first time. The orientation of this feature is similar to that of a large scale atomic/molecular gas distribution. For HESS J1741-302, our analysis does not yield any MeV-GeV counterpart for this unidentified TeV source. On the other hand, we have detected a new point source, Fermi J1740.1-3013, serendipitously. Its spectrum is apparently curved which resembles that of a γ\gamma-ray pulsar. This makes it possibly associated with PSR B1737-20 or PSR J1739-3023.Comment: 11 pages, 7 figures, 2 tables, accepted for publication in MNRA

    Cosmic axion thermalization

    Full text link
    Axions differ from the other cold dark matter candidates in that they form a degenerate Bose gas. It is shown that their huge quantum degeneracy and large correlation length cause cold dark matter axions to thermalize through gravitational self-interactions when the photon temperature reaches approximately 500 eV. When they thermalize, the axions form a Bose-Einstein condensate. Their thermalization occurs in a regime, herein called the `condensed regime', where the Boltzmann equation is not valid because the energy dispersion of the particles is smaller than their interaction rate. We derive analytical expressions for the thermalization rate of particles in the condensed regime, and check the validity of these expressions by numerical simulation of a toy model. We revisit axion cosmology in light of axion Bose-Einstein condensation. It is shown that axions are indistinguishable from ordinary cold dark matter on all scales of observational interest, except when they thermalize or rethermalize. The rethermalization of axions that are about to fall in a galactic potential well causes them to acquire net overall rotation as they go to the lowest energy state consistent with the total angular momentum they acquired by tidal torquing. This phenomenon explains the occurrence of caustic rings of dark matter in galactic halos. We find that photons may reach thermal contact with axions and investigate the implications of this possibility for the measurements of cosmological parameters.Comment: 38 pages, 1 figur

    Persistence in Cluster--Cluster Aggregation

    Get PDF
    Persistence is considered in diffusion--limited cluster--cluster aggregation, in one dimension and when the diffusion coefficient of a cluster depends on its size ss as D(s)sγD(s) \sim s^\gamma. The empty and filled site persistences are defined as the probabilities, that a site has been either empty or covered by a cluster all the time whereas the cluster persistence gives the probability of a cluster to remain intact. The filled site one is nonuniversal. The empty site and cluster persistences are found to be universal, as supported by analytical arguments and simulations. The empty site case decays algebraically with the exponent θE=2/(2γ)\theta_E = 2/(2 - \gamma). The cluster persistence is related to the small ss behavior of the cluster size distribution and behaves also algebraically for 0γ<20 \le \gamma < 2 while for γ<0\gamma < 0 the behavior is stretched exponential. In the scaling limit tt \to \infty and K(t)K(t) \to \infty with t/K(t)t/K(t) fixed the distribution of intervals of size kk between persistent regions scales as n(k;t)=K2f(k/K)n(k;t) = K^{-2} f(k/K), where K(t)tθK(t) \sim t^\theta is the average interval size and f(y)=eyf(y) = e^{-y}. For finite tt the scaling is poor for ktzk \ll t^z, due to the insufficient separation of the two length scales: the distances between clusters, tzt^z, and that between persistent regions, tθt^\theta. For the size distribution of persistent regions the time and size dependences separate, the latter being independent of the diffusion exponent γ\gamma but depending on the initial cluster size distribution.Comment: 14 pages, 12 figures, RevTeX, submitted to Phys. Rev.

    RNF17 blocks promiscuous activity of PIWI proteins in mouse testes

    Get PDF
    PIWI proteins and their associated piRNAs protect germ cells from the activity of mobile genetic elements. Two classes of piRNAs-primary and secondary-are defined by their mechanisms of biogenesis. Primary piRNAs are processed directly from transcripts of piRNA cluster loci, whereas secondary piRNAs are generated in an adaptive amplification loop, termed the ping-pong cycle. In mammals, piRNA populations are dynamic, shifting as male germ cells develop. Embryonic piRNAs consist of both primary and secondary species and are mainly directed toward transposons. In meiotic cells, the piRNA population is transposon-poor and largely restricted to primary piRNAs derived from pachytene piRNA clusters. The transition from the embryonic to the adult piRNA pathway is not well understood. Here we show that RNF17 shapes adult meiotic piRNA content by suppressing the production of secondary piRNAs. In the absence of RNF17, ping-pong occurs inappropriately in meiotic cells. Ping-pong initiates piRNA responses against not only transposons but also protein-coding genes and long noncoding RNAs, including genes essential for germ cell development. Thus, the sterility of Rnf17 mutants may be a manifestation of a small RNA-based autoimmune reaction

    A sandpile model with tokamak-like enhanced confinement phenomenology

    Get PDF
    Confinement phenomenology characteristic of magnetically confined plasmas emerges naturally from a simple sandpile algorithm when the parameter controlling redistribution scalelength is varied. Close analogues are found for enhanced confinement, edge pedestals, and edge localised modes (ELMs), and for the qualitative correlations between them. These results suggest that tokamak observations of avalanching transport are deeply linked to the existence of enhanced confinement and ELMs.Comment: Manuscript is revtex (latex) 1 file, 7 postscript figures Revised version is final version accepted for publication in PRL Revisions are mino

    Persistence with Partial Survival

    Full text link
    We introduce a parameter pp, called partial survival, in the persistence of stochastic processes and show that for smooth processes the persistence exponent θ(p)\theta(p) changes continuously with pp, θ(0)\theta(0) being the usual persistence exponent. We compute θ(p)\theta(p) exactly for a one-dimensional deterministic coarsening model, and approximately for the diffusion equation. Finally we develop an exact, systematic series expansion for θ(p)\theta(p), in powers of ϵ=1p\epsilon=1-p, for a general Gaussian process with finite density of zero crossings.Comment: 5 pages, 2 figures, references added, to appear in Phys.Rev.Let

    Managing aging effects on dry cask storage systems for extended long-term storage and transportation of used fuel - rev. 0

    Get PDF
    The cancellation of the Yucca Mountain repository program in the United States raises the prospect of extended long-term storage (i.e., &gt;120 years) and deferred transportation of used fuel at operating and decommissioned nuclear power plant sites. Under U.S. federal regulations contained in Title 10 of the Code of Federal Regulations (CFR) 72.42, the initial license term for an Independent Spent Fuel Storage Installation (ISFSI) must not exceed 40 years from the date of issuance. Licenses may be renewed by the U.S. Nuclear Regulatory Commission (NRC) at the expiration of the license term upon application by the licensee for a period not to exceed 40 years. Application for ISFSI license renewals must include the following: (1) Time-limited aging analyses (TLAAs) that demonstrate that structures, systems, and components (SSCs) important to safety will continue to perform their intended function for the requested period of extended operation; and (2) a description of the aging management program (AMP) for management of issues associated with aging that could adversely affect SSCs important to safety. In addition, the application must also include design bases information as documented in the most recent updated final safety analysis report as required by 10 CFR 72.70. Information contained in previous applications, statements, or reports filed with the Commission under the license may be incorporated by reference provided that those references are clear and specific. The NRC has recently issued the Standard Review Plan (SRP) for renewal of used-fuel dry cask storage system (DCSS) licenses and Certificates of Compliance (CoCs), NUREG-1927, under which NRC may renew a specific license or a CoC for a term not to exceed 40 years. Both the license and the CoC renewal applications must contain revised technical requirements and operating conditions (fuel storage, surveillance and maintenance, and other requirements) for the ISFSI and DCSS that address aging effects that could affect the safe storage of the used fuel. The information contained in the license and CoC renewal applications will require NRC review to verify that the aging effects on the SSCs in DCSSs/ ISFSIs are adequately managed for the period of extended operation. To date, all of the ISFSIs located across the United States with more than 1,500 dry casks loaded with used fuel have initial license terms of 20 years; three ISFSIs (Surry, H.B. Robinson and Oconee) have received their renewed licenses for 20 years, and two other ISFSIs (Calvert Cliffs and Prairie Island) have applied for license renewal for 40 years. This report examines issues related to managing aging effects on the SSCs in DCSSs/ISFSIs for extended long-term storage and transportation of used fuels, following an approach similar to that of the Generic Aging Lessons Learned (GALL) report, NUREG-1801, for the aging management and license renewal of nuclear power plants. The report contains five chapters and an appendix on quality assurance for aging management programs for used-fuel dry storage systems. Chapter I of the report provides an overview of the ISFSI license renewal process based on 10 CFR 72 and the guidance provided in NUREG-1927. Chapter II contains definitions and terms for structures and components in DCSSs, materials, environments, aging effects, and aging mechanisms. Chapter III and Chapter IV contain generic TLAAs and AMPs, respectively, that have been developed for managing aging effects on the SSCs important to safety in the dry cask storage system designs described in Chapter V. The summary descriptions and tabulations of evaluations of AMPs and TLAAs for the SSCs that are important to safety in Chapter V include DCSS designs (i.e., NUHOMS{reg_sign}, HI-STORM 100, Transnuclear (TN) metal cask, NAC International S/T storage cask, ventilated storage cask (VSC-24), and the Westinghouse MC-10 metal dry storage cask) that have been and continue to be used by utilities across the country for dry storage of used fuel to date. The goal of this report is to help establish the technical basis for extended long-term storage and transportation of used fuel
    corecore