310 research outputs found
Exotic baryons from a heavy meson and a nucleon - Positive parity states -
We study heavy baryons with exotic flavor quantum numbers formed by a heavy
meson and a nucleon (DbarN and BN) with positive parity. One pion exchange
interaction, providing a tensor force, dominates as a long range force to bind
the DbarN and BN ystems. In the heavy quark mass limit, pseudoscalar meson and
vector meson are degenerate and the binding mechanism by the tensor force
analogous to that in the nuclear systems becomes important. As a result, we
obtain the DbarN and BN resonant states in the J^P=1/2^+, 3/2^+ and 5/2^+
channels with I=0
R-process viable outflows are suppressed in global alpha-viscosity models of collapsar disks
Collapsar disks have been proposed to be rich factories of heavy elements,
but the major question of whether their outflows are neutron-rich, and could
therefore represent significant sites of the rapid neutron-capture (r-)
process, or dominated by iron-group elements remains unresolved. We present the
first global models of collapsars that start from a stellar progenitor and
self-consistently describe the evolution of the disk, its composition, and its
outflows in response to the imploding stellar mantle, using energy-dependent M1
neutrino transport and an alpha-viscosity to approximate turbulent
angular-momentum transport. We find that a neutron-rich, neutrino-dominated
accretion flow (NDAF) is established only marginally--either for short times or
relatively low viscosities--because the disk tends to disintegrate into an
advective disk (ADAF) already at relatively high mass-accretion rates,
launching powerful outflows but preventing it from developing a hot, dense, and
therefore neutron-rich core. Viscous outflows disrupt the star within ~100s
with explosion energies close to that of hypernovae. If viscosity is neglected,
a stable NDAF with disk mass of about 1Msun is formed but is unable to release
neutron-rich ejecta, while it produces a relatively mild explosion powered by a
neutrino-driven wind blown off its surface. With ejecta electron fractions
close to 0.5, all models presumably produce large amounts of Ni56. Our results
suggest that collapsar models based on the alpha-viscosity are inefficient
r-process sites and that genuinely magnetohydrodynamic effects may be required
to generate neutron-rich outflows. A relatively weak effective viscosity
generated by magnetohydrodynamic turbulence would improve the prospects for
obtaining neutron-rich ejecta.Comment: 7 pages, 4 figures, 1 table, slightly revised discussion, main
results unchanged compared to v1, accepted to ApJ
Collimated Jet or Expanding Outflow: Possible Origins of GRBs and X-Ray Flashes
We investigate the dynamics of an injected outflow propagating in a
progenitor in the context of the collapsar model for gamma-ray bursts (GRBs)
through two dimensional axisymmetric relativistic hydrodynamic simulations.
Initially, we locally inject an outflow near the center of a progenitor. We
calculate 25 models, in total, by fixing its total input energy to be 10^{51}
ergs s^{-1} and radius of the injected outflow to be cm while
varying its bulk Lorentz factor, , and its specific
internal energy, . The injected outflow propagates
in the progenitor and drives a large-scale outflow or jet. We find a smooth but
dramatic transition from a collimated jet to an expanding outflow among
calculated models. The maximum Lorentz factor is, on the other hand, sensitive
to both of and ; roughly . Our finding will explain a smooth transition between the
GRBs, X-ray rich GRBs (XRRs) and X-ray Flashes (XRFs) by the same model but
with different values.Comment: Comments 51 pages, 21 figures. accepted for publication in ApJ high
resolution version is available at
http://www.mpa-garching.mpg.de/~mizuta/COLLAPSAR/collapsar.htm
High Ratio of 44Ti/56Ni in Cas A and Axisymmetric Collapse-Driven Supernova Explosion
The large abundance ratio of in Cas A is puzzling. In fact,
the ratio seems to be larger than the theoretical constraint derived by Woosley
& Hoffman (1991). However, this constraint is obtained on the assumption that
the explosion is spherically symmetric, whereas Cas A is famous for the
asymmetric form of the remnant. Recently, Nagataki et al. (1997) calculated the
explosive nucleosynthesis of axisymmetrically deformed collapse-driven
supernova. They reported that the ratio of was enhanced by
the stronger alpha-rich freezeout in the polar region. In this paper, we apply
these results to Cas A and examine whether this effect can explain the large
amount of and the large ratio of . We demonstrate
that the conventional spherically symmetric explosion model can not explain the
Ti mass produced in Cas A if its lifetime is shorter than 80
years and the intervening space is transparent to the gamma-ray line from the
decay of Ti. On the other hand, we show the axisymmetric explosion
models can solve the problem. We expect the same effect from a three
dimensionally asymmetric explosion, since the stronger alpha-rich freezeout
will also occur in that case in the region where the larger energy is
deposited.Comment: 10 pages, LaTeX text and 3 postscript figure
Optical characterization of In-flushed InAs/GaAs quantum dots emitting a broadband spectrum with multiple peaks at ~1 μm
Explosive Nucleosynthesis in Axisymmetrically Deformed Type II Supernovae
Explosive nucleosynthesis under the axisymmetric explosion in Type II
supernova has been performed by means of two dimensional hydrodynamical
calculations. We have compared the results with the observations of SN 1987A.
Our chief findings are as follows: (1) is synthesized so much as to
explain the tail of the bolometric light curve of SN 1987A. We think this is
because the alpha-rich freezeout takes place more actively under the
axisymmetric explosion. (2) and tend to be overproduced
compared with the observations. However, this tendency relies strongly on the
progenitor's model.
We have also compared the abundance of each element in the mass number range
with the solar values. We have found three outstanding features. (1)
For the nuclei in the range , their abundances are insensitive to the
initial form of the shock wave. This insensitivity is favored since the
spherical calculations thus far can explain the solar system abundances in this
mass range. (2) There is an enhancement around A=45 in the axisymmetric
explosion compared with the spherical explosion fairly well. In particular,
, which is underproduced in the present spherical calculations, is
enhanced significantly. (3) In addition, there is an enhancement around A=65.
This tendency does not rely on the form of the mass cut but of the initial
shock wave. This enhancement may be the problem of the overproduction in this
mass range, although this effect would be relatively small since Type I
supernovae are chiefly responsible for this mass number range.Comment: 32 pages, 12 figures, LaTe
High Energy Neutrino Emission and Neutrino Background from Gamma-Ray Bursts in the Internal Shock Model
High energy neutrino emission from GRBs is discussed. In this paper, by using
the simulation kit GEANT4, we calculate proton cooling efficiency including
pion-multiplicity and proton-inelasticity in photomeson production. First, we
estimate the maximum energy of accelerated protons in GRBs. Using the obtained
results, neutrino flux from one burst and a diffuse neutrino background are
evaluated quantitatively. We also take account of cooling processes of pion and
muon, which are crucial for resulting neutrino spectra. We confirm the validity
of analytic approximate treatments on GRB fiducial parameter sets, but also
find that the effects of multiplicity and high-inelasticity can be important on
both proton cooling and resulting spectra in some cases. Finally, assuming that
the GRB rate traces the star formation rate, we obtain a diffuse neutrino
background spectrum from GRBs for specific parameter sets. We introduce the
nonthermal baryon-loading factor, rather than assume that GRBs are main sources
of UHECRs. We find that the obtained neutrino background can be comparable with
the prediction of Waxman & Bahcall, although our ground in estimation is
different from theirs. In this paper, we study on various parameters since
there are many parameters in the model. The detection of high energy neutrinos
from GRBs will be one of the strong evidences that protons are accelerated to
very high energy in GRBs. Furthermore, the observations of a neutrino
background has a possibility not only to test the internal shock model of GRBs
but also to give us information about parameters in the model and whether GRBs
are sources of UHECRs or not.Comment: 14 pages, 17 figures, accepted for publication in PRD, with extended
descriptions. Conclusions unchange
Optimization of the analogue-sensitive Cdc2/Cdk1 mutant by in vivo selection eliminates physiological limitations to its use in cell cycle analysis
Analogue-sensitive (as) mutants of kinases are widely used to selectively inhibit a single kinase with few off-target effects. The analogue-sensitive mutant cdc2-as of fission yeast (Schizosaccharomyces pombe) is a powerful tool to study the cell cycle, but the strain displays meiotic defects, and is sensitive to high and low temperature even in the absence of ATP-analogue inhibitors. This has limited the use of the strain for use in these settings. Here, we used in vivo selection for intragenic suppressor mutations of cdc2-as that restore full function in the absence of ATP-analogues. The cdc2-asM17 underwent meiosis and produced viable spores to a similar degree to the wild-type strain. The suppressor mutation also rescued the sensitivity of the cdc2-as strain to high and low temperature, genotoxins and an anti-microtubule drug. We have used cdc2-asM17 to show that Cdc2 activity is required to maintain the activity of the spindle assembly checkpoint. Furthermore, we also demonstrate that maintenance of the Shugoshin Sgo1 at meiotic centromeres does not require Cdc2 activity, whereas localization of the kinase aurora does. The modified cdc2-asM17 allele can be thus used to analyse many aspects of cell-cycle-related events in fission yeast
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