32,870 research outputs found
Tracking Quintessence Would Require Two Cosmic Coincidences
Good tracking requires that the quintessence energy fraction slowly increase
while the roll slowly decreases, but is
not yet truly slow-rolling. The supernova bound on the present quintessence
equation of state requires either (1) a cosmological constant or other
fine-tuned "crawling quintessence" or (2) "roll-over quintessence" that tracked
until recently, but now became slow rolling, because of a sharp increase in
potential curvature. Thus, fine-tuning is required by constant equation of
state and inverse power potentials, but can be avoided by the SUGRA and
Skordis-Albrecht potentials and other good trackers, provided quintessence
energy domination and slow roll {\em both} began only recently. This makes the
time in which we live special in {\em two} respects.Comment: 10 pages, including 2 figures, 3 table
\u3cem\u3ePainting the Map Red: Canada and the South African War, 1899–1902\u3c/em\u3e by Carmen Miller [Review]
Review of Carman Miller, Painting the Map Red: Canada and the South African War, 1899-1902. Montreal: McGill-Queen\u27s University Press, 1993
Knowing the Soviet Union: the ideological dimension
This repository item contains a single article of the Publication Series, papers in areas of particular scholarly interest published from 1989 to 1996 by the Boston University Institute for the Study of Conflict, Ideology, and Policy. The volume this article belongs to is titled "The USSR: what do we know and how do we know it?"
An Authority in Action—An Account of the Port of New York Authority and Its Recent Activities
Observed Smooth Energy is Anthropically Even More Likely As Quintessence Than As Cosmological Constant
For a universe presently dominated by static or dynamic vacuum energy,
cosmological constant (LCDM) or quintessence (QCDM), we calculate the
asymptotic collapsed mass fraction as function of the present ratio of vacuum
energy to clustered mass, \Omega_{Q0}/\Omega_{m0}. Identifying these collapsed
fractions as anthropic probabilities, we find the value \Omega_{Q0}/\Omega_{m0}
\sim 2 to be reasonably likely in LCDM, and very likely in QCDM.Comment: 4 pages, 2 tables, 1 figur
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