59 research outputs found
Hydrodynamic Models of Type I X-Ray Bursts: Metallicity Effects
Type I X-ray bursts are thermonuclear stellar explosions driven by
charged-particle reactions. In the regime for combined H/He-ignition, the main
nuclear flow is dominated by the rp-process (rapid proton-captures and beta+
decays), the 3 alpha-reaction, and the alpha-p-process (a suite of (alpha,p)
and (p,gamma) reactions). The main flow is expected to proceed away from the
valley of stability, eventually reaching the proton drip-line beyond A = 38.
Detailed analysis of the relevant reactions along the main path has only been
scarcely addressed, mainly in the context of parameterized one-zone models. In
this paper, we present a detailed study of the nucleosynthesis and nuclear
processes powering type I X-ray bursts. The reported 11 bursts have been
computed by means of a spherically symmetric (1D), Lagrangian, hydrodynamic
code, linked to a nuclear reaction network that contains 325 isotopes (from 1H
to 107Te), and 1392 nuclear processes. These evolutionary sequences, followed
from the onset of accretion up to the explosion and expansion stages, have been
performed for 2 different metallicities to explore the dependence between the
extension of the main nuclear flow and the initial metal content. We carefully
analyze the dominant reactions and the products of nucleosynthesis, together
with the the physical parameters that determine the light curve (including
recurrence times, ratios between persistent and burst luminosities, or the
extent of the envelope expansion). Results are in qualitative agreement with
the observed properties of some well-studied bursting sources. Leakage from the
predicted SbSnTe-cycle cannot be discarded in some of our models. Production of
12C (and implications for the mechanism that powers superbursts), light
p-nuclei, and the amount of H left over after the bursting episodes will also
be discussed.Comment: 78 pages (pdf), including 34 figures. Accepted for publication in The
Astrophysical Journal Suppl. Serie
The Sensitivity of Nucleosynthesis in Type I X-ray Bursts to Thermonuclear Reaction-Rate Variations
We examine the sensitivity of nucleosynthesis in Type I X-ray bursts to
variations in nuclear rates. As a large number of nuclear processes are
involved in these phenomena -with the vast majority of reaction rates only
determined theoretically due to the lack of any experimental information- our
results can provide a means for determining which rates play significant roles
in the thermonuclear runaway. These results may then motivate new experiments.
For our studies, we have performed a comprehensive series of one-zone
post-processing calculations in conjunction with various representative X-ray
burst thermodynamic histories. We present those reactions whose rate variations
have the largest effects on yields in our studies.Comment: 8 pages, accepted for publication in New Astronomy Reviews, Special
Issue on "Astronomy with Radioactivities VI" workshop, Ringberg Castle,
Germany, Jan. 200
The effects of vitamin A supplementation with measles vaccine on leucocyte counts and in vitro cytokine production
Host-parasite interactio
Desmoplastic fibroma of the mandible - review of the literature and presentation of a rare case
Desmoplastic fibroma (DF) is a rare, benign but locally aggressive, intraosseous lesion with a high tendency of local recurrence. In this report the actual literature is reviewed regarding epidemiological data, pathology, clinical diagnostic criterias, therapy and prognosis. Moreover, a report of an interesting case is included localized in the mandibular corpus
Nuclear astrophysics: the unfinished quest for the origin of the elements
Half a century has passed since the foundation of nuclear astrophysics. Since
then, this discipline has reached its maturity. Today, nuclear astrophysics
constitutes a multidisciplinary crucible of knowledge that combines the
achievements in theoretical astrophysics, observational astronomy,
cosmochemistry and nuclear physics. New tools and developments have
revolutionized our understanding of the origin of the elements: supercomputers
have provided astrophysicists with the required computational capabilities to
study the evolution of stars in a multidimensional framework; the emergence of
high-energy astrophysics with space-borne observatories has opened new windows
to observe the Universe, from a novel panchromatic perspective; cosmochemists
have isolated tiny pieces of stardust embedded in primitive meteorites, giving
clues on the processes operating in stars as well as on the way matter
condenses to form solids; and nuclear physicists have measured reactions near
stellar energies, through the combined efforts using stable and radioactive ion
beam facilities. This review provides comprehensive insight into the nuclear
history of the Universe and related topics: starting from the Big Bang, when
the ashes from the primordial explosion were transformed to hydrogen, helium,
and few trace elements, to the rich variety of nucleosynthesis mechanisms and
sites in the Universe. Particular attention is paid to the hydrostatic
processes governing the evolution of low-mass stars, red giants and asymptotic
giant-branch stars, as well as to the explosive nucleosynthesis occurring in
core-collapse and thermonuclear supernovae, gamma-ray bursts, classical novae,
X-ray bursts, superbursts, and stellar mergers.Comment: Invited Review. Accepted for publication in "Reports on Progress in
Physics" (version with low-resolution figures
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