11,726 research outputs found
Additional Acceleration of Protons and Energetic Neutrino Production in a Filamentary Jet of the Blazar Markarian 501
Blazars have been regarded as one of the most powerful sources of the highest
energy cosmic rays and also their byproducts, neutrinos. Provided that a
magnetized filamentary system is established in a blazar jet as well, we could
apply the mechanism of multi-stage diffusive shock acceleration to a feasible
TeV emitter, Mrk 501 to evaluate the achievable maximum energy of protons.
Taking conceivable energy restriction into account systematically, it seems
adequate to say that EeV-protons are produced at this site by our present
model. We also estimate neutrino fluxes generated by these accelerated protons
and discuss the detectability based on an updated kilometre-scale telescope
such as IceCube.Comment: 17 pages, 3 Postscript figure
Vortex servovalve for fluidic or electrical input
Proportional-pressure control servovalve consisting of fluid amplifier bellows-driven jet-pipe and two vortex valves operating in push-pull, with a pair of bellows for pressure feedback is tolerant to comtaminant particles and meets minimum standby flow requirements for applications such as rocket thruster nozzles
An experimental investigation on the subcritical instability in plane Poieseuille flow
The relationship between the three dimensional properties of the fundamental flow of a plane Poieseuille flow and subcritical stability was studied. An S-T wave was introduced into the flow and the three dimensional development of the wave observed. Results indicate that: (1) the T-S wave has three dimensional properties which are synchronous with the fundamental flow, but there is damping at microamplitude; (2) when the amplitude reaches a certain threshold, subcritical instability and peak valley bifurcation occur simultaneously and a peak valley structure is formed; (3) this threshold depends to a great extent on the frequency; and (4) after the peak valley bifurcation there is a transition to a turbulent flow by the process of laminar flow collapse identical to that in Blasius flow
Fluidic proportional thruster for SPARCS 4
Design, development, fabrication, and acceptance test results for two fluidic proportional thrusters for use in SPARCS
Behavior of Li abundances in solar-analog stars II. Evidence of the connection with rotation and stellar activity
We previously attempted to ascertain why the Li I 6708 line-strengths of
Sun-like stars differ so significantly despite the superficial similarities of
stellar parameters. We carried out a comprehensive analysis of 118 solar
analogs and reported that a close connection exists between the Li abundance
A_Li and the line-broadening width (v_r+m; mainly contributed by rotational
effect), which led us to conclude that stellar rotation may be the primary
control of the surface Li content. To examine our claim in more detail, we
study whether the degree of stellar activity exhibits a similar correlation
with the Li abundance, which is expected because of the widely believed close
connection between rotation and activity. We measured the residual flux at the
line center of the strong Ca II 8542 line, r_0(8542), known to be a useful
index of stellar activity, for all sample stars using newly acquired spectra in
this near-IR region. The projected rotational velocity (v_e sin i) was
estimated by subtracting the macroturbulence contribution from v_r+m that we
had already established. A remarkable (positive) correlation was found in the
A_Li versus (vs.) r_0(8542) diagram as well as in both the r_0(8542) vs. v_e
sin i and A_Li vs. v_e sin i diagrams, as had been expected. With the
confirmation of rotation-dependent stellar activity, this clearly shows that
the surface Li abundances of these solar analogs progressively decrease as the
rotation rate decreases. Given this observational evidence, we conclude that
the depletion of surface Li in solar-type stars, probably caused by effective
envelope mixing, operates more efficiently as stellar rotation decelerates. It
may be promising to attribute the low-Li tendency of planet-host G dwarfs to
their different nature in the stellar angular momentum.Comment: 12 pages, 9 figures; accepted for publication in Astron. Astrophys
Effects of mirror reflection versus diffusion anisotropy on particle acceleration in oblique shocks
Cosmic ray particles are more rapidly accelerated in oblique shocks, with the
magnetic field inclined with respect to the shock normal direction, than in
parallel shocks, as a result of mirror reflection at the shock surface and
slower diffusion in the shock normal direction. We investigate quantitatively
how these effects contribute to reducing the acceleration time over the whole
range of magnetic field inclinations. It is shown that, for quasi-perpendicular
inclination, the mirror effect plays a remarkable role in reducing the
acceleration time; whereas, at relatively small inclination, the anisotropic
diffusion effect is dominant in reducing that time. These results are important
for a detailed understanding of the mechanism of particle acceleration by an
oblique shock in space and heliosphereic plasmas.Comment: 6 pages, 2 figure
Transitive X-ray spectrum and PeV gamma-ray cutoff in the M87 jet: Electron "Pevatron"
We propose a modified version of the X-ray spectral index and an intrinsic
cutoff frequency of inverse Compton radiation from the brightest knot of the
M87 jet, in conjunction with an application of the new conceptions of injection
and diffusive shock acceleration (DSA) of electrons in magnetized filamentary
plasma to the specified source. The drop of the X-ray flux density in a
transitive frequency region is associated with the interplay of ordinary
synchrotron cooling and weaker magnetic fields concomitant with the smaller
scale filaments that allow the electron injection, while the radio-optical
synchrotron continuum is dominantly established by the major electrons that are
quasi-secularly bound to larger filaments. With reference to, particularly, the
updated external Compton model, we demonstrate that in the Klein-Nishina regime
fading inverse Comptonization, the injected electrons can be stochastically
energized up to a Lorentz factor as high as in the temporal
competition with diffuse synchrotron cooling; this value is larger than that
attainable for a simple DSA scenario based on the resonant scattering diffusion
of the gyrating electrons bound to a supposed magnetic field homogeneously
pervading the entire knot. The upper limits of the photon frequency boosted via
conceivable inverse Compton processes are predicted to be of the common order
of Hz. The variability of the broadband spectrum is also
discussed in comparison to the features of a blazar light curve. The present
scenario of a peta-eV (PeV; eV) electron accelerator, the "Pevatron,"
might provide some guidance for exploring untrod hard X-ray and gamma-ray bands
in forthcoming observations.Comment: 34 pages, 6 figures, matches version published in Ap
Atmospheric neutrino flux at INO, South Pole and Pyh\"asalmi
We present the calculation of the atmospheric neutrino fluxes for the
neutrino experiments proposed at INO, South Pole and Pyh\"asalmi. Neutrino
fluxes have been obtained using ATMNC, a simulation code for cosmic ray in the
atmosphere. Even using the same primary flux model and the interaction model,
the calculated atmospheric neutrino fluxes are different for the different
sites due to the geomagnetic field. The prediction of these fluxes in the
present paper would be quite useful in the experimental analysis.Comment: 12Pages,9Fig
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