13,360 research outputs found

    An assessment of the newest magnetar-SNR associations

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    Anomalous X-ray Pulsars and Soft-Gamma Repeaters groups are magnetar candidates featuring low characteristic ages (Ï„=P2PË™\tau = {P\over{2 {\dot P}}}). At least some of them they should still be associated with the remnants of the explosive events in which they were born, giving clues to the type of events leading to their birth and the physics behind the apparent high value of the magnetar magnetic fields. To explain the high values of BB, a self-consistent picture of field growth also suggests that energy injection into the SNR is large and unavoidable, in contrast with the evolution of {\it conventional} SNR. This modified dynamics, in turn, has important implications for the proposed associations. We show that this scenario yields low ages for the new candidates CXOU J171405.7-381031/CTB 37B and XMMU J173203.3-344518/G353.6-0.7, and predicted values agree with recently found PË™{\dot P}, giving support to the overall picture.Comment: Contributed talk to the ASTRONS 2010 Conference, Cesme, Turkey, Aug. 2-6 201

    Major loop reconstruction from switching of individual particles

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    Major hysteresis loops of groups of isolated 60 mm square garnet particles of a regular two-dimensional array, have been measured magnetooptically. Individual loops for each particle were measured, and the statistics of the distribution of coercivities and interaction fields was determined. It is shown that from the measured coercivity distribution and calculated magnetostatic interaction fields the major hysteresis loop can be reconstructed. The switching sequence, and the major loop of an assembly of 535 particles were calculated numerically for two cases: first, when calculating the magnetostatic interaction, the 25 particles were assumed to be isolated; second, the major loop of the same 25 particles, embedded into a 939 square, was reconstructed taking into account the interactions among all 81 particles. The numerically simulated major hysteresis loops agree very well with the measured loops, demonstrating the reliability of numerical modeling

    The Quasi-Roche lobe overflow state in the evolution of Close Binary Systems containing a radio pulsar

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    We study the evolution of close binary systems formed by a normal (solar composition), intermediate mass donor star together with a neutron star. We consider models including irradiation feedback and evaporation. These non-standard ingredients deeply modify the mass transfer stages of these binaries. While models that neglect irradiation feedback undergo continuous, long standing mass transfer episodes, models including these effect suffer a number cycles of mass transfer and detachment. During mass transfer the systems should reveal themselves as low-mass X-ray binaries (LMXBs), whereas when detached they behave as a binary radio pulsars. We show that at these stages irradiated models are in a Roche lobe overflow (RLOF) state or in a quasi-RLOF state. Quasi-RLOF stars have a radius slightly smaller than its Roche lobe. Remarkably, these conditions are attained for orbital period and donor mass values in the range corresponding to a family of binary radio pulsars known as "redbacks". Thus, redback companions should be quasi-RLOF stars. We show that the characteristics of the redback system PSR J1723-2837 are accounted for by these models. In each mass transfer cycle these systems should switch from LMXB to binary radio pulsar states with a timescale of \sim million years. However, there is recent and fast growing evidence of systems switching on far shorter, human timescales. This should be related to instabilities in the accretion disc surrounding the neutron star and/or radio ejection, still to be included in the model having the quasi-RLOF state as a general condition.Comment: 27 pages, 7 figures. Accepted for publication in The Astrophysical Journa

    An evolutionary model for the gamma-ray system PSR J1311-3430 and its companion

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    The most recent member of the millisecond pulsar with very low-mass companions and short orbital periods class, PSR J1311-3430 (Pletsch et al. 2012) is a remarkable object in various senses. Besides being the first discovered in gamma-rays, its measured features include the very low or absent hydrogen content. We show in this Letter that this important piece of information leads to a very restricted range of initial periods for a given donor mass. For that purpose, we calculate in detail the evolution of the binary system self-consistently, including mass transfer and evaporation, finding the features of the new evolutionary path leading to the observed configuration. It is also important to remark that the detailed evolutionary history of the system naturally leads to a high final pulsar mass, as it seems to be demanded by observations.Comment: 5 pages, 5 figures, 1 table. Accepted for publication in MNRAS Letter

    Pion mass effects on axion emission from neutron stars through NN bremsstrahlung processes

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    The rates of axion emission by nucleon-nucleon bremsstrahlung are calculated with the inclusion of the full momentum contribution from a nuclear one pion exchange (OPE) potential. The contributions of the neutron-neutron (nn), proton-proton (pp) and neutron-proton (np) processes in both the nondegenerate and degenerate limits are explicitly given. We find that the finite momentum corrections to the emissivities are quantitatively significant for the non-degenerate regime and temperature-dependent, and should affect the existing axion mass bounds. The trend of these nuclear effects is to diminish the emissivities

    Critical issues in rape investigation: a UK perspective

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    This article examines a recent history of criminal justice reform to responses to the investigation of rape offences. Beginning with a selective overview of the professional development of detectives and criticisms relating to investigation of „low status‟ crimes this article points to the challenges in the professionalization of detectives in the context of investigative responses to marginalised victims. The paper goes on to outline police responses and evaluations of initiatives aimed at improving effectiveness before summarising the complexities and vulnerabilities faced by victims and how these experiences impact upon the likelihood of successful prosecution. Finally the paper summaries the main analysis and indentifies the key challenges to the criminal justice sector in improving responses to rape victims

    Critical issues in rape investigation: an overview of reform in England and Wales

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    This article examines a recent history of criminal justice reform to responses to the investigation of rape offences. Beginning with a selective overview of the professional development of detectives and criticisms relating to investigation of „low status‟ crimes this article points to the challenges in the professionalization of detectives in the context of investigative responses to marginalised victims. The paper goes on to outline police responses and evaluations of initiatives aimed at improving effectiveness before summarising the complexities and vulnerabilities faced by victims and how these experiences impact upon the likelihood of successful prosecution. Finally the paper summaries the main analysis and indentifies the key challenges to the criminal justice sector in improving responses to rape victims

    Color-flavor locked strange matter

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    We analyze how the CFL states in dense matter work in the direction of enhancing the parameter space for absolutely stable phases (strange matter). We find that the "CFL strange matter" phase can be the true ground state of hadronic matter for a much wider range of the parameters of the model (the gap of the QCD Cooper pairs Δ\Delta, the strange quark mass msm_s and the Bag Constant BB) than the state without any pairing, and derive a full equation of state and an accurate analytic approximation to the lowest order in Δ\Delta and msm_{s} which may be directly used for applications. The effects of pairing on the equation of state are found to be small (as previously expected) but not negligible and may be relevant for astrophysics.Comment: 5 pages, 2 figure
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