6,931 research outputs found
Multimetric Supergravities
Making use of integral forms and superfield techniques we propose
supersymmetric extensions of the multimetric gravity Lagrangians in dimensions
one, two, three and four. The supersymmetric interaction potential covariantly
deforms the bosonic one, producing in particular suitable super-symmetric
polynomials generated by the Berezinian. As an additional application of our
formalism we construct supersymmetric multi-Maxwell theories in dimensions
three and four.Comment: 37 pages, Latex2e, no figure
Efficacy of first-line sodium thiosulphate administration in a case of potassium cyanide poisoning
Cyanide poisoning may occur following accidental fire-smoke inhalation or deliberate ingestion of salts. Hydroxocobalamin represents a first-line life-saving antidote. Although hydroxocobalamin represents a first-line lifesaving antidote, it is still not promptly available in the emergency department. Sodium thiosulfate can be administered in association with hydroxocobalamin whereas the delayed onset of clinical response makes sodium thiosulfate less suitable for emergency use. We describe a case of cyanide intoxication of a 43-year-old man who ingested an unknown amount of potassium cyanide, purchased via the Internet, in an attempted suicide. At admission to the emergency department, the patient presented GCS 3 with severe lactic acidosis. Orotracheal intubation, gastric lavage and oral activated charcoal were applied. Sodium thiosulfate was available in the emergency department and 10 grams were infused over a 30 minute period. Hydroxocobalamin was prescribed by the poison control centre and 5 grams were infused 2 hours after admission. Following sodium thiosulfate administration the patient was arousable and lactate concentration improved. No adverse effects were noted. Metabolic acidosis completely resolved 12 hours later. Cyanide concentration performed on blood samples collected at admission confirmed high cyanide blood levels (15 mg/L). This report highlights as the first-line administration of sodium thiosulfate, in rapid infusion, resulted effective and safe for cyanide poisoning. Our report suggests that sodium thiosulfate should be considered when hydroxocobalamin is not promptly available in an emergency settin
Formation of carbon-enhanced metal-poor stars in the presence of far ultraviolet radiation
Recent discoveries of carbon-enhanced metal-poor stars like SMSS
J031300.36-670839.3 provide increasing observational insights into the
formation conditions of the first second-generation stars in the Universe,
reflecting the chemical conditions after the first supernova explosion. Here,
we present the first cosmological simulations with a detailed chemical network
including primordial species as well as C, C, O, O, Si, Si, and
Si following the formation of carbon-enhanced metal poor stars. The
presence of background UV flux delays the collapse from to and
cool the gas down to the CMB temperature for a metallicity of
Z/Z=10. This can potentially lead to the formation of lower mass
stars. Overall, we find that the metals have a stronger effect on the collapse
than the radiation, yielding a comparable thermal structure for large
variations in the radiative background. We further find that radiative
backgrounds are not able to delay the collapse for Z/Z=10 or a
carbon abundance as in SMSS J031300.36-670839.3.Comment: submitted to ApJ
Dark-matter halo mergers as a fertile environment for low-mass Population III star formation
While Population III stars are typically thought to be massive, pathways
towards lower-mass Pop III stars may exist when the cooling of the gas is
particularly enhanced. A possible route is enhanced HD cooling during the
merging of dark-matter halos. The mergers can lead to a high ionization degree
catalysing the formation of HD molecules and may cool the gas down to the
cosmic microwave background (CMB) temperature. In this paper, we investigate
the merging of mini-halos with masses of a few 10 M and explore the
feasibility of this scenario. We have performed three-dimensional cosmological
hydrodynamics calculations with the ENZO code, solving the thermal and chemical
evolution of the gas by employing the astrochemistry package KROME. Our results
show that the HD abundance is increased by two orders of magnitude compared to
the no-merging case and the halo cools down to 60 K triggering
fragmentation. Based on Jeans estimates the expected stellar masses are about
10 M. Our findings show that the merging scenario is a potential
pathway for the formation of low-mass stars.Comment: Submitted to MNRA
The formation of massive primordial stars in the presence of moderate UV backgrounds
Radiative feedback from populations II stars played a vital role in early
structure formation. Particularly, photons below the Lyman limit can escape the
star forming regions and produce a background ultraviolet (UV) flux which
consequently may influence the pristine halos far away from the radiation
sources. These photons can quench the formation of molecular hydrogen by
photo-detachment of . In this study, we explore the impact of such
UV radiation on fragmentation in massive primordial halos of a few times ~M. To accomplish this goal, we perform high resolution
cosmological simulations for two distinct halos and vary the strength of the
impinging background UV field in units of . We further make use of
sink particles to follow the evolution for 10,000 years after reaching the
maximum refinement level. No vigorous fragmentation is observed in UV
illuminated halos while the accretion rate changes according to the thermal
properties. Our findings show that a few 100-10, 000 solar mass protostars are
formed when halos are irradiated by at and
suggest a strong relation between the strength of UV flux and mass of a
protostar. This mode of star formation is quite different from minihalos, as
higher accretion rates of about M/yr are observed by
the end of our simulations. The resulting massive stars are the potential
cradles for the formation of intermediate mass black holes at earlier cosmic
times and contribute to the formation of a global X-ray background.Comment: Submitted to APJ, comments are welcome. High resolution copy is
available at http://www.astro.physik.uni-goettingen.de/~mlatif/IMBHs_apj.pd
How realistic UV spectra and X-rays suppress the abundance of direct collapse black holes
Observations of high redshift quasars at indicate that they harbor
supermassive black holes (SMBHs) of a billion solar masses. The direct collapse
scenario has emerged as the most plausible way to assemble SMBHs. The nurseries
for the direct collapse black holes are massive primordial halos illuminated
with an intense UV flux emitted by population II (Pop II) stars. In this study,
we compute the critical value of such a flux () for
realistic spectra of Pop II stars through three-dimensional cosmological
simulations. We derive the dependence of on the radiation
spectra, on variations from halo to halo, and on the impact of X-ray
ionization. Our findings show that the value of is a few
times and only weakly depends on the adopted radiation spectra in
the range between K. For three simulated halos
of a few times ~M, varies from . The impact of X-ray ionization is almost
negligible and within the expected scatter of for
background fluxes of . The computed estimates of
have profound implications for the quasar abundance at
as it lowers the number density of black holes forming through an
isothermal direct collapse by a few orders of magnitude below the observed
black holes density. However, the sites with moderate amounts of
cooling may still form massive objects sufficient to be compatible with
observations.Comment: Accepted for publication in MNRAS, comments are welcom
Non-Critical Pure Spinor Superstrings
We construct non-critical pure spinor superstrings in two, four and six
dimensions. We find explicitly the map between the RNS variables and the pure
spinor ones in the linear dilaton background. The RNS variables map onto a
patch of the pure spinor space and the holomorphic top form on the pure spinor
space is an essential ingredient of the mapping. A basic feature of the map is
the requirement of doubling the superspace, which we analyze in detail. We
study the structure of the non-critical pure spinor space, which is different
from the ten-dimensional one, and its quantum anomalies. We compute the pure
spinor lowest lying BRST cohomology and find an agreement with the RNS spectra.
The analysis is generalized to curved backgrounds and we construct as an
example the non-critical pure spinor type IIA superstring on AdS_4 with RR
4-form flux.Comment: LaTeX2e, 76 pages, no figures, JHEP style; v2: references and
acknowledgments added, typos corrected; v3: typos corrected and minor changes
to match published versio
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