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Economies of Scale and Merger Efficiencies: Empirical Evidence from the Chilean Pension Funds Market
(Universidad Alberto Hurtado. Facultad de Economía y Negocios, 2015)
Economies of scale and merger efficiencies in the chilean pension funds market.
Over the last twenty years there has been a significant concentration process in the pension fund manager industry in Chile (the number of firms has dropped from 21 in 1994 to only 6 in 2012). A major concern about the ...
Turbulent magnetic-field amplification in the first 10 milliseconds after a binary neutron star merger: Comparing high-resolution and large-eddy simulations
(American Physical Society, 2020-11)
The detection of binary neutron star mergers represents one of the most important and complex astrophysical discoveries of the recent years. One of the unclear aspects of the problem is the turbulent magnetic field ...
Environmental Policy, Mergers and Environmental R&D with Spillovers
(Pontificia Universidad Católica del Perú, 2020)
Environmental Policy, Mergers and Environmental R&D with Spillovers
(Pontificia Universidad Católica del Perú. Fondo EditorialPE, 2020)
'Fundamental Plane'-like relations from collisionless stellar dynamics: a comparison of mergers and collapses
(Blackwell Publishing LtdOxfordInglaterra, 2003)
Gradient subgrid-scale model for relativistic MHD large-eddy simulations
(American Physical Society, 2020-03-15)
Magnetohydrodynamics (MHD) turbulence is likely to play an important role in several astrophysical scenarios, where the magnetic Reynolds is very large. Numerically, these cases can be studied efficiently by means of ...
Sistemas peculiares de galaxias :
(2009-03)
Se presenta un estudio estadístico sobre grupos compactos y fósiles identificados en simulaciones numéricas combinadas
con diferentes modelos semianalíticos de formación de galaxias. Los resultados fueron también confrontados ...
Direct formation of supermassive black holes via multi-scale gas inflows in galaxy mergers
(2010)
Observations of distant quasars indicate that supermassive black holes of billions of solar masses already existed less than a billion years after the Big Bang1. Models in which the ‘seeds’ of such black holes form by the ...
Dissipationless collapse of spherical protogalaxies and the fundamental plane
(E D P SciencesLes Ulis CedexaFrança, 2002)