Modified Friedmann equations via conformal Bohm -- De Broglie gravity

We use an alternative interpretation of quantum mechanics, based on the Bohmian trajectory approach, and show that the quantum effects can be included in the classical equation of motion via a conformal transformation on the background metric. We apply this method to the Robertson-Walker metric to derive a modified version of Friedmann's equations for a Universe consisting of scalar, spin-zero, massive particles. These modified equations include additional terms that result from the non-local nature of matter and appear as an acceleration in the expansion of the Universe. We see that the same effect may also be present in the case of an inhomogeneous expansion.Comment: Accepted for publication in Ap

On the Cosmic Ray Driven Firehose Instability

The role of the non-resonant firehose instability in conditions relevant to the precursors of supernova remnant shocks is considered. Using a second order tensor expansion of the Vlasov-Fokker-Planck equation we illustrate the necessary conditions for the firehose to operate. It is found that for very fast shocks, the diffusion approximation predicts that the linear firehose growth rate is marginally faster than its resonant counterpart. Preliminary hybrid MHD-Vlasov-Fokker-Planck simulation results using young supernova relevant parameters are presented.Comment: Contribution to the 6th International Symposium on High Energy Gamma-Ray Astronomy (Gamma2016), Heidelberg, Germany. To be published in the AIP Conference Proceeding

Education and referral criteria: impact on oncology referrals to palliative care.

OBJECTIVE: To describe a quality improvement project involving education and referral criteria to influence oncology provider referrals to a palliative care service. METHODS: A single group post-test only quasi-experimental design was used to evaluate palliative care service (PCS) referrals following an intervention consisting of a didactic presentation, education outreach visits (EOV) to key providers, and referral criteria. Data on patient demographics, cancer types, consult volume, reasons for referral, pre-consult length of stay, overall hospital stay, and discharge disposition were collected pre-intervention, then post-intervention for 7.5 months and compared. SETTING AND SAMPLE: Attending oncologists, nurse practitioner, and house staff from the solid tumor division at a 700-bed urban teaching hospital participated in the project. Two geriatricians, a palliative care nurse practitioner, and rotating geriatric fellows staffed the PCS. RESULTS: The percentage of oncology referrals to PCS increased significantly following the intervention (χ(2) = 6.108, p = .013). 24.9% (390) patients were referred in the 4.6 years pre-intervention and 31.5% (106) patients were referred during 7.5 months post-intervention. The proportion of consults for pain management was significantly greater post-intervention (χ(2) = 5.378, p = .02), compared to pre-intervention, when most referrals were related to end-of-life issues. Lung, pancreatic, and colon were the most common cancer types at both periods, and there were no significant differences in patient demographics, pre-referral length of hospitalization or overall hospital days. There was a trend toward more patients being discharged alive following the intervention. CONCLUSION: A quality improvement project supported the use of education and referral criteria to influence both the frequency and reasons for palliative care referral by oncology providers

Inverse Compton emission from heavy WIMP annihilations in the Galactic Centre

A thermal relic WIMP remains a prime candidate for the nature of Dark Matter,particularly for the more poorly constrained case of a heavy ($\gtrsim$ 1 TeV)WIMP. The highest fluxes from WIMP annihilations are expected in the region ofthe Galactic Centre (GC) where current and near future gamma-ray observatoriescan be exploited to place tight limits on the WIMP paradigm. It is regularlynoted that the annihilation flux of gammas will be accompanied by chargedsecondary particles which can produce 'delayed' inverse Compton (IC) gamma-rayemission, but this component is often neglected in indirect Dark Mattersearches. In this work the inverse Compton emission is studied for the specificconditions of heavy WIMP annihilation in the GC. Using models for the magneticand radiation fields of the region, and taking into consideration the transportof secondary particles, we find that for TeV WIMPs the IC component cannot beneglected in the GC, with the particles produced cooling within the regionrather than propagating out in to the Galaxy. This effect changes the predictedspectral shape substantially and thus boosts the detection prospects for heavyWIMPs.<br

Time evolution and asymmetry of a laser produced blast wave

Studies of a blast wave produced from carbon rods and plastic spheres in an argon background gas have been conducted using the Vulcan laser at the Rutherford Appleton Laboratory. A laser of 1500 J was focused onto these targets, and rear-side observations of an emission front were recorded using a fast-framing camera. The emission front is asymmetrical in shape and tends to a more symmetrical shape as it progresses due to the production of a second shock wave later in time, which pushes out the front of the blast wave. Plastic spheres produce faster blast waves, and the breakthrough of the second shock is visible before the shock stalls. The results are presented to demonstrate this trend, and similar evolution dynamics of experimental and simulation data from the FLASH radiation-hydrodynamics code are observed

The theory of pulsar winds and nebulae

We review current theoretical ideas on pulsar winds and their surrounding nebulae. Relativistic MHD models of the wind of the aligned rotator, and of the striped wind, together with models of magnetic dissipation are discussed. It is shown that the observational signature of this dissipation is likely to be point-like, rather than extended, and that pulsed emission may be produced. The possible pulse shapes and polarisation properties are described. Particle acceleration at the termination shock of the wind is discussed, and it is argued that two distinct mechanisms must be operating, with the first-order Fermi mechanism producing the high-energy electrons (above 1 TeV) and either magnetic annihilation or resonant absorption of ion cyclotron waves responsible for the 100 MeV to 1 TeV electrons. Finally, MHD models of the morphology of the nebula are discussed and compared with observation.Comment: 33 pages, to appear in Springer Lecture Notes on "Neutron stars and pulsars, 40 years after the discovery", ed W.Becke

X-ray spectral analysis of the jet termination shock in pictor A on subarcsecond scales with Chandra

Hot spots observed at the edges of extended radio lobes in high-power radio galaxies and quasars mark the position of mildly relativistic termination shock, where the jet bulk kinetic energy is converted to the internal energy of the jet particles. These are the only astrophysical systems where mildly relativistic shocks can be directly resolved at various wavelengths of the electromagnetic spectrum. The western hot spot in the radio galaxy Pictor A is an exceptionally good target in this respect, due to the combination of its angular size and high surface brightness. In our previous work, after a careful Chandra image deconvolution, we resolved this hot spot into a disk-like feature perpendicular to the jet axis, and identified it as the front of the jet termination shock. We argued for a synchrotron origin of the observed X-ray photons, which implied electron energies reaching at least 10–100 TeV at the shock front. Here, we present a follow-up on that analysis, proposing, in particular, a novel method for constraining the shape of the X-ray continuum emission with subarcsecond resolution. The method is based on a Chandra hardness map analysis, using separately deconvolved maps in the soft and hard X-ray bands. In this way, we have found there is a systematic, yet statistically significant gradient in the hardness ratio across the shock, such that the implied electron energy index ranges from s $\leq$ 2.2 at the shock front to s > 2.7 in the near downstream. We discuss the implications of the obtained results for a general understanding of particle acceleration at mildly relativistic shocks