3,087 research outputs found
Dynamic Aperture Studies for SPEAR 3
The Stanford Synchrotron Radiation Laboratory is investigating an accelerator
upgrade project that would replace the present 130 nm rad FODO lattice with an
18 nm rad double bend achromat (DBA) lattice: SPEAR 3. The low emittance design
yields a high brightness beam, but the stronger focusing in the DBA lattice
increases chromaticity and beam sensitivity to machine errors. To ensure
efficient injection and long Touschek lifetime, an optimization of the design
lattice and dynamic aperture has been performed. In this paper, we review the
methods used to maximize the SPEAR 3 dynamic aperture including necessary
optics modifications, choice of tune and phase advance, optimization of
sextupole and coupling correction, and modeling effects of machine errors,
wigglers and lattice periodicity.Comment: 23 page
TRIP13 is a protein-remodeling AAA+ ATPase that catalyzes MAD2 conformation switching.
The AAA+ family ATPase TRIP13 is a key regulator of meiotic recombination and the spindle assembly checkpoint, acting on signaling proteins of the conserved HORMA domain family. Here we present the structure of the Caenorhabditis elegans TRIP13 ortholog PCH-2, revealing a new family of AAA+ ATPase protein remodelers. PCH-2 possesses a substrate-recognition domain related to those of the protein remodelers NSF and p97, while its overall hexameric architecture and likely structural mechanism bear close similarities to the bacterial protein unfoldase ClpX. We find that TRIP13, aided by the adapter protein p31(comet), converts the HORMA-family spindle checkpoint protein MAD2 from a signaling-active 'closed' conformer to an inactive 'open' conformer. We propose that TRIP13 and p31(comet) collaborate to inactivate the spindle assembly checkpoint through MAD2 conformational conversion and disassembly of mitotic checkpoint complexes. A parallel HORMA protein disassembly activity likely underlies TRIP13's critical regulatory functions in meiotic chromosome structure and recombination
The effects of metallicity and cooling physics on fragmentation: implications on direct-collapse black hole formation
A promising supermassive black hole seed formation channel is that of direct
collapse from primordial gas clouds. We perform a suite of 3D hydrodynamics
simulations of an isolated turbulent gas cloud to investigate conditions
conducive to forming massive black hole seeds via direct collapse, probing the
impact of cloud metallicity, gas temperature floor and cooling physics on cloud
fragmentation. We find there is no threshold in metallicity which produces a
sharp drop in fragmentation. When molecular cooling is not present, metallicity
has little effect on fragmentation. When molecular cooling is present,
fragmentation is suppressed by at most , with the greatest
suppression seen at metallicities below solar. A gas temperature floor
K produces the largest drop in fragmentation of any parameter
choice, reducing fragmentation by . At metallicities below
solar or at temperatures K we see a reduction in fragmentation
. For a cloud of metallicity solar above and a temperature
below K, the detailed choices of temperature floor, metallicity, and
cooling physics have little impact on fragmentation.Comment: 5 pages, 4 figures, submitted to MNRA
Securing Bystander Privacy in Mixed Reality While Protecting the User Experience
The modern Mixed Reality devices that make the Metaverse viable can also
require vast information about the physical world. These devices can also
violate the privacy of unsuspecting or unwilling bystanders in their vicinity.
In this article, we explore the problem, existing solutions, and avenues for
future research.Comment: 12 pages, 2 Figure
High-energy electron-induced damage production at room temperature in aluminum-doped silicon
DLTS and EPR measurements are reported on aluminum-doped silicon that was irradiated at room temperature with high-energy electrons. Comparisons are made to comparable experiments on boron-doped silicon. Many of the same defects observed in boron-doped silicon are also observed in aluminum-doped silicon, but several others were not observed, including the aluminum interstitial and aluminum-associated defects. Damage production modeling, including the dependence on aluminum concentration, is presented
Effects of combined drug treatments on Plasmodium falciparum : in vitro assays with doxycycline, ivermectin and efflux pump inhibitors
There is great concern regarding the rapid emergence and spread of drug-resistance in Plasmodium falciparum, the parasite responsible for the most severe form of human malaria. Parasite populations resistant to some or all the currently available antimalarial treatments are present in different world regions. Considering the need for novel and integrated approaches to control malaria, combinations of drugs were tested on P. falciparum. The primary focus was on doxycycline, an antibiotic that specifically targets the apicoplast of the parasite. In combination with doxycycline, three different drugs known to inhibit efflux pumps (verapamil, elacridar and ivermectin) were tested, with the assumption that they could increase the intracellular concentration of the antibiotic and consequently its efficacy against P. falciparum. We emphasize that elacridar is a third-generation ABC transporters inhibitor, never tested before on malaria parasites. In vitro experiments were performed on asexual stages of two strains of P. falciparum, chloroquine-sensitive (D10) and chloroquineresistant (W2). Incubation times on asynchronous or synchronous cultures were 72h or 96h, respectively. The antiplasmodial effect (i.e. the IC50) was determined by measuring the activity of the parasite lactate dehydrogenase, while the interaction between drugs was determined through combination index (CI) analyses. Elacridar achieved an IC50 concentration comparable to that of ivermectin, approx. 10-fold lower than that of verapamil, the other tested ABC transporter inhibitor. CI results showed synergistic effect of verapamil plus doxycycline, which is coherent with the starting hypothesis, i.e. that ABC transporters represent potential targets, worth of further investigations, towards the development of companion molecules useful to enhance the efficacy of antimalarial drugs. At the same time, the observed antagonistic effect of doxycycline in combination with ivermectin or elacridar highlighted the importance of drug testing, to avoid the de-facto generation of a sub-dosage, a condition that facilitates the development of drug resistance
ASCA and contemporaneous ground-based observations of the BL Lacertae objects 1749+096 and 2200+420 (BL Lac)
We present ASCA observations of the radio-selected BL Lacertae objects
1749+096 (z=0.32) and 2200+420 (BL Lac, z=0.069) performed in 1995 Sept and
Nov, respectively. The ASCA spectra of both sources can be described as a first
approximation by a power law with photon index Gamma ~ 2. This is flatter than
for most X-ray-selected BL Lacs observed with ASCA, in agreement with the
predictions of current blazar unification models. While 1749+096 exhibits
tentative evidence for spectral flattening at low energies, a concave continuum
is detected for 2200+420: the steep low-energy component is consistent the
high-energy tail of the synchrotron emission responsible for the longer
wavelengths, while the harder tail at higher energies is the onset of the
Compton component. The spectral energy distributions from radio to gamma-rays
are consistent with synchrotron-self Compton emission from a single homogeneous
region shortward of the IR/optical wavelengths, with a second component in the
radio domain related to a more extended emission region. For 2200+420,
comparing the 1995 Nov state with the optical/GeV flare of 1997 July, we find
that models requiring inverse Compton scattering of external photons provide a
viable mechanism for the production of the highest (GeV) energies during the
flare. An increase of the external radiation density and of the power injected
in the jet can reproduce the flat gamma-ray continuum observed in 1997 July. A
directly testable prediction of this model is that the line luminosity in
2200+420 should vary shortly after (~1 month) a non-thermal synchrotron flare.Comment: 28 pages,6 figures, 5 tables; LaTeX document. accepted for
publication in the Astrophysical Journa
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