Post-Newtonian SPH calculations of binary neutron star coalescence. I. Method and first results

We present the first results from our Post-Newtonian (PN) Smoothed Particle Hydrodynamics (SPH) code, which has been used to study the coalescence of binary neutron star (NS) systems. The Lagrangian particle-based code incorporates consistently all lowest-order (1PN) relativistic effects, as well as gravitational radiation reaction, the lowest-order dissipative term in general relativity. We test our code on sequences of single NS models of varying compactness, and we discuss ways to make PN simulations more relevant to realistic NS models. We also present a PN SPH relaxation procedure for constructing equilibrium models of synchronized binaries, and we use these equilibrium models as initial conditions for our dynamical calculations of binary coalescence. Though unphysical, since tidal synchronization is not expected in NS binaries, these initial conditions allow us to compare our PN work with previous Newtonian results. We compare calculations with and without 1PN effects, for NS with stiff equations of state, modeled as polytropes with $\Gamma=3$. We find that 1PN effects can play a major role in the coalescence, accelerating the final inspiral and causing a significant misalignment in the binary just prior to final merging. In addition, the character of the gravitational wave signal is altered dramatically, showing strong modulation of the exponentially decaying waveform near the end of the merger. We also discuss briefly the implications of our results for models of gamma-ray bursts at cosmological distances.Comment: RevTeX, 37 pages, 17 figures, to appear in Phys. Rev. D, minor corrections onl

Accretion, Outflows, and Winds of Magnetized Stars

Many types of stars have strong magnetic fields that can dynamically influence the flow of circumstellar matter. In stars with accretion disks, the stellar magnetic field can truncate the inner disk and determine the paths that matter can take to flow onto the star. These paths are different in stars with different magnetospheres and periods of rotation. External field lines of the magnetosphere may inflate and produce favorable conditions for outflows from the disk-magnetosphere boundary. Outflows can be particularly strong in the propeller regime, wherein a star rotates more rapidly than the inner disk. Outflows may also form at the disk-magnetosphere boundary of slowly rotating stars, if the magnetosphere is compressed by the accreting matter. In isolated, strongly magnetized stars, the magnetic field can influence formation and/or propagation of stellar wind outflows. Winds from low-mass, solar-type stars may be either thermally or magnetically driven, while winds from massive, luminous O and B type stars are radiatively driven. In all of these cases, the magnetic field influences matter flow from the stars and determines many observational properties. In this chapter we review recent studies of accretion, outflows, and winds of magnetized stars with a focus on three main topics: (1) accretion onto magnetized stars; (2) outflows from the disk-magnetosphere boundary; and (3) winds from isolated massive magnetized stars. We show results obtained from global magnetohydrodynamic simulations and, in a number of cases compare global simulations with observations.Comment: 60 pages, 44 figure

Operation and performance of the ATLAS semiconductor tracker

The semiconductor tracker is a silicon microstrip detector forming part of the inner tracking system of the ATLAS experiment at the LHC. The operation and performance of the semiconductor tracker during the first years of LHC running are described. More than 99% of the detector modules were operational during this period, with an average intrinsic hit efficiency of (99.74±0.04)%. The evolution of the noise occupancy is discussed, and measurements of the Lorentz angle, δ-ray production and energy loss presented. The alignment of the detector is found to be stable at the few-micron level over long periods of time. Radiation damage measurements, which include the evolution of detector leakage currents, are found to be consistent with predictions and are used in the verification of radiation background simulations

Humor attenuates the cortisol awakening response in healthy older men

This study examined the impact of an important factor contributing to successful aging, humor, on post-awakening cortisol levels among a group of 45 older men whose ages ranged from 64 years to 86 years (mean = 73.6 years). Four saliva samples were collected from the participants for 2 days immediately after waking and every 15 min thereafter for three times. Cortisol data of the 2 days were aggregated for analysis. Two separate indices of cortisol awakening response reflecting the mean level of secretion and the rise from immediately to 45 min post-awakening, AUCG and AUCI, were computed using the trapezoid formula. The relation of these two indices to humor (operationalized as coping) was examined in a multiple regression analysis while controlling for the effect of age, socioeconomic status, and self-esteem. Results indicated that higher humor scores were associated with lower AUCG but had no relation with AUCI. Findings of the present study suggest that the hypothalamic-pituitary-adrenocortical axis is the major pathway whereby positive psychological dispositions, such as humor, exert their health effects in the aging population. Moreover, cortisol levels in the awakening period may be particularly sensitive to the influences of psychosocial factors

An updated meta-analysis to understand the variable efficacy of drotrecogin alfa (activated) in severe sepsis and septic shock

Background. Significant debate continues over the efficacy of drotrecogin alpha activated (DAA) in sepsis. This updated meta-analysis provides an updated summary effect estimate and explores the reasons for outcome heterogeneity in placebo-controlled randomized clinical trials of DAA on 28-day all-cause mortality in patients with severe sepsis or septic shock. Methods. Computer searches of MEDLINE, EMBASE, the Cochrane Library, ClinicalTrials.gov, published abstracts from major intensive care meetings and examination of reference lists were used to identify five placebo-controlled randomized clinical trials with 7260 patients. The primary endpoint was 28-day all-cause mortality. Secondary outcomes were 28-day incidence of severe bleeding and intracranial hemorrhage. Results. DAA was not associated with improved 28-day all-cause mortality in patients with severe sepsis or septic shock (pooled relative risk (RR) of 0.97 [95% CI 0.83-1.14]), and is associated with an increase in serious bleeding. The significant heterogeneity in the pooled RR for 28-day mortality (I2 value of 59.4%, \u3c72 P-value 0.043) is no longer present with exclusion of the post-study amendment portion of PROWESS (I2 value of 0%, \u3c72 P-value 0.44 without PROWESS post-amendment). Using meta-regression, the best ranked predictor of outcome heterogeneity was baseline mortality in the placebo arm, which was among the highest in PROWESS. Conclusion. DAA is not associated with improved survival in patients with severe sepsis or septic shock. Further studies should be done to determine whether changes in supportive therapy for sepsis explain the variable efficacy of DAA in randomized controlled clinical trials observed over time