123 research outputs found
The Pairing Mechanism in HTSC investigated by Electronic Raman Scattering
By means of electronic Raman scattering we investigated the symmetry of the
energy gap Delta(k), its temperature dependence and its variation with doping
of well characterized Bi2Sr2CaCu2O8+delta single crystals. The oxygen content
delta was varied between the under- and the overdoped regime by subsequently
annealing the same single crystal in Ar and O2, respectively. The symmetry
analysis of the polarized electronic Raman scattering is consistent with a
d_x^2-y^2-wave symmetry of the energy gap in both regimes. The gap ratio
2Delta_max/k_BT_c and its temperature dependence changes with doping similar to
predictions of theories based on paramagnon coupling.Comment: 3 pages, LaTeX, 2 ps figures available on request to
[email protected]
De onderwijsenquête van 1799:Overzicht van de toestand van scholen en onderwijs in Nederland
Het eerste landelijke overzicht van de toestand van het onderwijs stamt uit 1799. Enige jaren daarvoor had de Bataafse Republiek een einde aan het gewestelijk en stedelijk particularisme van de Republiek van de Verenigde Nederlanden gemaakt en de eenheidsstaat uitgeroepen. Van de inwoners werd verwacht dat zij hun oude bindingen opgaven en zich zouden identificeren met de cultuur van de nieuwe staat. Om de eenheidsgedachte te stimuleren nam de overheid diverse maatregelen. Het onderwijs werd als hét middel om een bijdrage aan de fundering van de nationale staat te leveren, gezien. Van staatswege zou aan de herinrichting een reorganisatie van het gehele onderwijs leiding worden gegeven. In 1798 belastte de overheid een Agent van Nationale Opvoeding met deze taak
Symmetry dependence of phonon lineshapes in superconductors with anisotropic gaps
The temperature dependence below of the lineshape of optical phonons
of different symmetry as seen in Raman scattering is investigated for
superconductors with anisotropic energy gaps. It is shown that the symmetry of
the electron-phonon vertex produces non-trivial couplings to an anisotropic
energy gap which leads to unique changes in the phonon lineshape for phonons of
different symmetry. The phonon lineshape is calculated in detail for
and phonons in a superconductor with pairing
symmetry. The role of satellite peaks generated by the electron-phonon coupling
are also addressed. The theory accounts for the substantial phonon narrowing of
the phonon, while narrowing of the phonon which is
indistinguishable from the normal state is shown, in agreement with recent
measurements on BSCCO.Comment: 15 pages (3 Figures available upon request), Revtex, 1
Formation of SMBH seeds in Pop III star clusters through collisions : the importance of mass loss
Runaway collisions in dense clusters may lead to the formation of
supermassive black hole (SMBH) seeds, and this process can be further enhanced
by accretion, as recent models of SMBH seed formation in Population III star
clusters have shown. This may explain the presence of supermassive black holes
already at high redshift, . However, in this context, mass loss during
collisions was not considered and could play an important role for the
formation of the SMBH seed. Here, we study the effect of mass loss, due to
collisions of protostars, in the formation and evolution of a massive object in
a dense primordial cluster. We consider both constant mass loss fractions as
well as analytic models based on the stellar structure of the collision
components. Our calculations indicate that mass loss can significantly affect
the final mass of the possible SMBH seed. Considering a constant mass loss of
5% for every collision, we can lose between 60-80% of the total mass that is
obtained if mass loss were not considered. Using instead analytical
prescriptions for mass loss, the mass of the final object is reduced by 15-40%,
depending on the accretion model for the cluster we study. Altogether, we
obtain masses of the order of , which are still massive enough
to be SMBH seeds.Comment: 12 pages, 9 figures, accepted by MNRA
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