1,869 research outputs found
Left Ventricular Outflow Tract Obstruction Defined by Active Three-Dimensional Echocardiography Using Rotational Transthoracic Acquisition
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/75675/1/j.1540-8175.1994.tb01105.x.pd
Components of Antineutrino Emission in Nuclear Reactor
New scattering experiments aimed for sensitive searches of
the magnetic moment and projects to explore small mixing angle
oscillations at reactors call for a better understanding of the reactor
antineutrino spectrum. Here we consider six components, which contribute to the
total spectrum generated in nuclear reactor. They are: beta
decay of the fission fragments of U, Pu, U and
Pu, decay of beta-emitters produced as a result of neutron capture in
U and also due to neutron capture in accumulated fission fragments
which perturbs the spectrum. For antineutrino energies less than 3.5 MeV we
tabulate evolution of spectra corresponding to each of the four
fissile isotopes vs fuel irradiation time and their decay after the irradiation
is stopped and also estimate relevant uncertainties. Small corrections to the
ILL spectra are considered.Comment: LaTex 8 pages, 2 ps figure
Neutrino magnetic moments and low-energy solar neutrino-electron scattering experiments
The scattering of solar neutrinos on electrons is sensitive to the neutrino
magnetic moments through an interference of electromagnetic and weak amplitudes
in the cross section. We show that future low-energy solar neutrino experiments
with good angular resolution can be sensitive to the resulting azimuthal
asymmetries in event number and should provide useful information on
non-standard neutrino properties such as magnetic moments. We compare
asymmetries expected at HELLAZ (mainly pp neutrinos) with those at the
Kamiokande and Super-Kamiokande experiments (Boron neutrinos), both for the
case of Dirac and Majorana neutrinos and discuss the advantages of low
energies. Potentially interesting information on the solar magnetic fields may
be accessible.Comment: 21 pages, latex, 5 PS figures, uses revtex, text improved, to be
published in Phys. Rev.
Solar neutrinos: global analysis with day and night spectra from SNO
We perform global analysis of the solar neutrino data including the day and
night spectra of events at SNO. In the context of two active neutrino mixing,
the best fit of the data is provided by the LMA MSW solution with Delta m^2 =
6.15 10^{-5} eV^2, tan^2\theta = 0.41, f_B = 1.05, where f_B is the boron
neutrino flux in units of the corresponding flux in the Standard Solar Model
(SSM). At 3 sigma level we find the following upper bounds: tan^2\theta < 0.84
and Delta m^2 < 3.6 10^{-4} eV^2. From 1 sigma-interval we expect the day-night
asymmetries of the charged current and electron scattering events to be:
A_{DN}^{CC} = 3.9 +3.6-2.9 and A_{DN}^{ES} = 2.1 +2.1-1.4. The only other
solution which appears at 3 sigma-level is the VAC solution with Delta m^2 =
4.5 10^{-10} eV^2, tan^2\theta = 2.1 and f_B=0.75. The best fit point in the
LOW region, with Delta m^2 = 0.93 10^{-7} eV^2 and tan^2\theta = 0.64, is
accepted at 99.95% (3.5 sigma) C.L. . The least chi^2 point from the SMA
solution region, with Delta m^2 = 4.6 10^{-6} eV^2 and tan^2\theta = 5 10^{-4},
could be accepted at 5.5 sigma-level only. In the three neutrino context the
influence of theta_{13} is studied. We find that with increase of theta_{13}
the LMA best fit point shifts to larger Delta m^2, mixing angle is practically
unchanged, and the quality of the fit becomes worse. The fits of LOW and SMA
slightly improve. Predictions for KamLAND experiment (total rates, spectrum
distortion) have been calculated.Comment: Typos corrected, reference adde
Neutrino spin-flips in curved space-time
The general relativistic effects on spin-flavor oscillations above the core
of type II supernovae are investigated. The evolution equation is derived and
the relative magnitudes of the terms in the Hamiltonian, which arise from the
weak, electromagnetic and gravitational interaction, are compared. The effects
on the resonance position and the adiabaticity are studied. Explicit
calculations are presented for non-rotating and slowly rotating stars.Comment: 16 pages, 1 figure, accepted by Phys. Rev.
Spin-Flavour Oscillations and Neutrinos from SN1987A
The neutrino signal from SN1987A is analysed with respect to spin-flavour
oscillations between electron antineutrinos, , and muon
neutrinos, , by means of a maximum likelihood analysis.
Following Jegerlehner et al. best fit values for the total energy released in
neutrinos, , and the temperature of the electron antineutrino,
, for a range of mixing parameters and progenitor models are
calculated. In particular the dependence of the inferred quantities on the
metallicity of the supernova is investigated and the uncertainties involved in
using the neutrino signal to determine the neutrino magnetic moment are pointed
out.Comment: 14 pages, RevTeX, 4 figures, to appear in Physical Review
Do national resources have to be centrally managed? Vested interests and institutional reform in Norwegian fisheries governance
Corporatism -with its privileged access, restricted participation and centralized
structures - has a long history in Norwegian fisheries governance. Co-management –
understood as a decentralized, bottom-up and more inclusive form of fisheries
governance - has not been considered a relevant alternative.. Why does corporatism
still prevail in a context where stakeholder status in fisheries governance globally – both
in principle and practice - has been awarded environmental organizations, municipal
authorities and even consumer advocacy groups? Why then have alternatives to the
corporatist system of centralized consultation and state governance never been seriously
considered in Norway, in spite of the growing emphasis on fish as a public resource and
fisheries management as human intervention in geographically confined and complex
ecosystems? We suggest that thismay have to do with the fundamental assumptions
behind Norwegian fisheries governance that since fish is a national resource, it must be
centrally managed. We argue that this is an assumption that may be contested
Complete chloroplast genome sequence of Holoparasite Cistanche Deserticola (Orobanchaceae) reveals gene loss and horizontal gene transfer from Its host Haloxylon Ammodendron (Chenopodiaceae)
The central function of chloroplasts is to carry out photosynthesis, and its gene content and structure are highly conserved across land plants. Parasitic plants, which have reduced photosynthetic ability, suffer gene losses from the chloroplast (cp) genome accompanied by the relaxation of selective constraints. Compared with the rapid rise in the number of cp genome sequences of photosynthetic organisms, there are limited data sets from parasitic plants. The authors report the complete sequence of the cp genome of Cistanche deserticola, a holoparasitic desert species belonging to the family Orobanchaceae
Investigate a Gas Well Performance Using Nodal Analysis
Gas condensate well has unique reservoir characteristics and ups and downs in well behaviour affect the production rate significantly. A proper optimization can reduce the operating cost, maximize the hydrocarbon recovery and increase the net present value. Well level optimization can be achieved through optimizing well parameters, such as wellhead, tubing size, and skin factor. All of these factors have been investigated using a real field of Thrace Basin and PROSPER simulation program. The history matching data are validated to identify the future performance prediction for the same reservoir deliverability following the period changes. Therefore, predicted results are compared and validated with measured field data to provide the best production practices. Moreover, the results show that the skin factor has a large influence on the production rate by 45% reduction. The reduction in the reservoir pressure declines the production rate dramatically resulted in 70% decline. While manipulating the wellhead pressure shows minor decline compare to tubing size that does not show any significant change to production rate
Supernova prompt neutronization neutrinos and neutrino magnetic moments
It is shown that the combined action of spin-flavor conversions of supernova
neutrinos due to the interactions of their Majorana-type transition magnetic
moments with the supernova magnetic fields and flavor conversions due to the
mass mixing can lead to the transformation of \nu_e born in the neutronization
process into their antiparticles \bar{\nu}_e. Such an effect would have a clear
experimental signature and its observation would be a smoking gun evidence for
the neutrino transition magnetic moments. It would also signify the leptonic
mixing parameter |U_{e3}| in excess of 10^{-2}.Comment: LaTex, 25 pages, 3 figures. v4: Discussion section expanded,
references added. Matches the published versio
- …