1,393 research outputs found
Frequency scaling of photo-induced tunneling
The DC current-voltage characteristics, induced by a driving electric field
with frequency Omega, of a one dimensional electron channel with a tunnel
barrier is calculated. Electron-electron interaction of finite-range is taken
into account. For intermediate interaction strengths, the non-linear
differential conductance shows cusp-like minima at bias voltages integer
multiples of hbar Omega / e that are a consequence of the finite non-zero range
of the interaction but are independent of the shape of the driving electric
field. However, the frequency-scaling of the photo-induced current shows a
cross-over between Omega^{-1} and Omega^{-2}, and depends on the spatial shape
of the driving field and the range of the interaction.Comment: 7 pages, EURO-TeX, 3 figures, to appear in Europhysics Letter
Magnetophononics: ultrafast spin control through the lattice
Using a combination of first-principles and magnetization-dynamics
calculations, we study the effect of the intense optical excitation of phonons
on the magnetic behavior in insulating magnetic materials. Taking the
prototypical magnetoelectric \CrO\ as our model system, we show that excitation
of a polar mode at 17 THz causes a pronounced modification of the magnetic
exchange interactions through a change in the average Cr-Cr distance. In
particular, the quasi-static deformation induced by nonlinear phononic coupling
yields a structure with a modified magnetic state, which persists for the
duration of the phonon excitation. In addition, our time-dependent
magnetization dynamics computations show that systematic modulation of the
magnetic exchange interaction by the phonon excitation modifies the
magnetization dynamics. This temporal modulation of the magnetic exchange
interaction strengths using phonons provides a new route to creating
non-equilibrium magnetic states and suggests new avenues for fast manipulation
of spin arrangements and dynamics.Comment: 11 pages with 7 figure
Spectral shape of the UV ionizing background and HeII absorption at redshifts 1.8 < z < 2.9
The shape of the UV ionizing background is reconstructed from optically thin
metal absorption-line systems identified in spectra of HE2347-4342, Q1157+3143,
and HS1700+6416 in the redshift interval 1.8 < z < 2.9. The systems are
analyzed by means of the Monte Carlo Inversion method completed with the
spectral shape recovering procedure. The UVB spectral shape fluctuates at 2.4 <
z < 2.9 mostly due to radiative transfer processes in the clumpy IGM. At z <
1.8, the IGM becomes almost transparent both in the HI and HeII Lyman continua
and the variability of the spectral shape comes from diversity of spectral
indices describing the QSO/AGN intrinsic radiation. At z > 2.4, the recovered
spectral shapes show intensity depression between 3 and 4 Ryd due to HeII
Ly-alpha absorption in the IGM clouds (line blanketing) and continuous medium
(true Gunn-Petersen effect). The mean HeII Ly-alpha opacity estimated from the
depth of this depression corresponds within 1-2sigma to the values directly
measured from the HI/HeII Ly-alpha forest towards the quasars studied. The
observed scatter in eta = N(HeII)/N(HI) and anti-correlation between N(HI) and
eta can be explained by the combined action of variable spectral softness and
differences in the mean gas density between the absorbing clouds. Neither of
the recovered spectral shapes show features which can be attributed to the
putative input of radiation from soft sources like starburst galaxies.Comment: 20 pages, 20 figures. Accepted for publication in A&
Reconstruction of neutrino energy in a large water Cerenkov detector using lepton information
In this note we study the reconstruction of neutrino energy from the knowledge of the beam direction and the energy and angle of the reconstructed lepton in quasi elastic electron and muon neutrino CC interactions. As a practical example, we consider the case of a prospective CERN-Frejus experiment based on the SPL and a Super Kamiokande-like water Cerenkov detector
An HST/COS legacy survey of intervening SiIII absorption in the extended gaseous halos of low-redshift galaxies
Doubly ionized silicon (SiIII) is a powerful tracer of diffuse ionized gas
inside and outside of galaxies. It can be observed in the local Universe in
ultraviolet (UV) absorption against bright extragalactic background sources. We
here present an extensive study of intervening SiIII-selected absorbers and
their relation to the circumgalactic medium (CGM) of galaxies at low redshift
(z<=0.1), based on the analysis of UV absorption spectra along 303
extragalactic lines of sight obtained with the Cosmic Origins Spectrograph
(COS) on board the Hubble Space Telescope (HST). Along a total redshift path of
Dz=24 we identify 69 intervening SiIII systems that all show associated
absorption from other low and high ions. We derive a bias-corrected number
density of dN/dz(SiIII)=2.5 for absorbers with column densities log
N(SiIII)>12.2. We develop a geometrical model for the absorption-cross section
of the CGM around the local galaxy population and find excellent agreement
between the model predictions and the observations. We further compare
redshifts and positions of the absorbers with that of ~64,000 galaxies using
archival galaxy-survey data. For the majority of the absorbers we identify
possible host galaxies within 300 km/s of the absorbers and derive impact
parameters rho<200 kpc, demonstrating that the spatial distributions of SiIII
absorbers and galaxies are highly correlated. Our study indicates that the
majority of SiIII-selected absorbers in our sample trace the CGM of nearby
galaxies within their virial radii at a typical covering fraction of ~70 per
cent. From a detailed ionization model we estimate that diffuse gas in the CGM
around galaxies, as traced by SiIII, contains substantially more baryonic mass
than their neutral interstellar medium.Comment: 32 pages, 17 figures; final version accepted for publication in A&
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