D - Javier García de Abajo
... A.1 Electrostatic potential over extended graphene by an external point charge . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 119 C.1 Energy-level diagram of infrared absorption, Rayleigh scattering, and Raman scattering . . . . . . . . . . . . . . . . . . . . . . . . . . . . ...
... A.1 Electrostatic potential over extended graphene by an external point charge . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 119 C.1 Energy-level diagram of infrared absorption, Rayleigh scattering, and Raman scattering . . . . . . . . . . . . . . . . . . . . . . . . . . . . ...
Optical Shop Testing
... No part of this publication may be reproduced, stored in a retrieval system, or transmitted in any form or by any means, electronic, mechanical, photocopying, recording, scanning, or otherwise, except as permitted under Section 107 or 108 of the 1976 United States Copyright Act, without either the p ...
... No part of this publication may be reproduced, stored in a retrieval system, or transmitted in any form or by any means, electronic, mechanical, photocopying, recording, scanning, or otherwise, except as permitted under Section 107 or 108 of the 1976 United States Copyright Act, without either the p ...
High-mass X-ray Binaries: X-raying the winds Ángel Giménez García
... (∼ 12 keV), responsable del ∼ 80 − 90% del flujo total. Tiene una luminosidad variable en cualquier escala ponderable de tiempo (desde algunos segundos a varios minutos), con valores de ∼ 1032−33 erg/s, pero sin grandes estallidos como en las BeXB. El descubrimiento, en los últimos años, de 6 nuevas ...
... (∼ 12 keV), responsable del ∼ 80 − 90% del flujo total. Tiene una luminosidad variable en cualquier escala ponderable de tiempo (desde algunos segundos a varios minutos), con valores de ∼ 1032−33 erg/s, pero sin grandes estallidos como en las BeXB. El descubrimiento, en los últimos años, de 6 nuevas ...
The Hunt for Recoiled Black Holes in the Milky Way`s
... Double Imaging Spectrograph (DIS) on the 3.5-m telescope with a slit width of 1.5”. The grating used was the B400 with 400 lines per millimeter on the blue side and R300 with 300 lines per millimeter on the red side. These gratings were centered on wavelengths of 4398 Å in the blue and 7493 Å in t ...
... Double Imaging Spectrograph (DIS) on the 3.5-m telescope with a slit width of 1.5”. The grating used was the B400 with 400 lines per millimeter on the blue side and R300 with 300 lines per millimeter on the red side. These gratings were centered on wavelengths of 4398 Å in the blue and 7493 Å in t ...
Doctorat doc
... and minimum loss (1550nm) wavelengths of silica. Such fibers provide the backbone of modern optical telecommunication networks. Since the late 1970s these fibers has been manufactured routinely. It is possible to manufacture very long fibers with very low attenuation (0.2dB/km). Multicomponent glass ...
... and minimum loss (1550nm) wavelengths of silica. Such fibers provide the backbone of modern optical telecommunication networks. Since the late 1970s these fibers has been manufactured routinely. It is possible to manufacture very long fibers with very low attenuation (0.2dB/km). Multicomponent glass ...
Get PDF - OSA Publishing
... where ε 0 and ε 0 0 and n and k are the real and imaginary parts of the complex permittivity and complex refractive index, respectively. Permittivity and refractive index have the following relationships: pffiffiffi ñ ε; ...
... where ε 0 and ε 0 0 and n and k are the real and imaginary parts of the complex permittivity and complex refractive index, respectively. Permittivity and refractive index have the following relationships: pffiffiffi ñ ε; ...
Link - Max-Planck-Institut für Astronomie
... µm. The Fe I, Li I, and Ca I optical lines, as well as the nearinfrared CO lines, are typically double-peaked and show line broadening that is kinematically consistent with a rotating disk origin (Hartmann and Kenyon, 1996), although a wind may also be required to explain these profiles (Eisner and ...
... µm. The Fe I, Li I, and Ca I optical lines, as well as the nearinfrared CO lines, are typically double-peaked and show line broadening that is kinematically consistent with a rotating disk origin (Hartmann and Kenyon, 1996), although a wind may also be required to explain these profiles (Eisner and ...
High Harmonic Generation for Coherent Diffractive Imaging
... the sampled spectrum. Diffraction patterns of wide dynamic range can be acquired by means of a new design involving a beam stop and image stitching. Binary and non-binary periodic and non-periodic samples have been successfully reconstructed. It is noted that the employment of multiple-wavelength co ...
... the sampled spectrum. Diffraction patterns of wide dynamic range can be acquired by means of a new design involving a beam stop and image stitching. Binary and non-binary periodic and non-periodic samples have been successfully reconstructed. It is noted that the employment of multiple-wavelength co ...
thesis_draft_4
... Figure 4.2. Micrographs of lactose crystals obtained from a gelatin-gel (43 wt% lactose, 1.5 wt% gelatin) after 24 hours at 25°C(a) 4X (scale bar = 500 μm) and (b) 20X (scale bar = 50 μm) magnifications..........................................................................54 Figure 4.3. XRD patte ...
... Figure 4.2. Micrographs of lactose crystals obtained from a gelatin-gel (43 wt% lactose, 1.5 wt% gelatin) after 24 hours at 25°C(a) 4X (scale bar = 500 μm) and (b) 20X (scale bar = 50 μm) magnifications..........................................................................54 Figure 4.3. XRD patte ...
Section 2 Simple Molecular Orbital Theory
... orbitals should be of comparable size and hence of similar electron binding energy. The size (e.g., average value or expectation value of the distance from the atomic nucleus to the electron) of an atomic orbital is determined primarily by its principal quantum number n and by the strength of the po ...
... orbitals should be of comparable size and hence of similar electron binding energy. The size (e.g., average value or expectation value of the distance from the atomic nucleus to the electron) of an atomic orbital is determined primarily by its principal quantum number n and by the strength of the po ...
Numerical techniques for Fresnel diffraction in computational
... dynamic monocular cue is motion parallax; the principle through which objects that are further from you appear to have less lateral movement than closer objects. This can be accomplished in 2D by the simple rotation or translation of a scene, and by properly including the parallax effect into the re ...
... dynamic monocular cue is motion parallax; the principle through which objects that are further from you appear to have less lateral movement than closer objects. This can be accomplished in 2D by the simple rotation or translation of a scene, and by properly including the parallax effect into the re ...
Electromagnetic Properties of Neutrinos
... between the left-handed components of the three flavor neutrino fields νe , νμ , ντ and the lefthanded components of three massive neutrino fields νk with masses mk k 1, 2, 3. The 3 × 3 mixing matrix U is unitary U† U−1 . Neutrino electromagnetic properties are discussed in 4–7, and in the ...
... between the left-handed components of the three flavor neutrino fields νe , νμ , ντ and the lefthanded components of three massive neutrino fields νk with masses mk k 1, 2, 3. The 3 × 3 mixing matrix U is unitary U† U−1 . Neutrino electromagnetic properties are discussed in 4–7, and in the ...
