3,128 research outputs found
The Overshoot Problem and Giant Structures
Models of small-field inflation often suffer from the overshoot problem. A
particularly efficient resolution to the problem was proposed recently in the
context of string theory. We show that this resolution predicts the existence
of giant spherically symmetric overdense regions with radius of at least 110
Mpc. We argue that if such structures will be found they could offer an
experimental window into string theory.Comment: 19 pages, 1 figure, comments and refs. adde
D6+D0 and Five Dimensional Spinning Black Hole
We study the system of D6+D0 branes at sub-stringy scale. We show that the
proper description of the system, for large background field associated with
the D0-branes, is via spinning chargeless black holes in five dimensions. The
repulsive force between the D6-branes and the D0-branes is understood through
the centrifugal barrier. We discuss the implication on the stability of the
D6+D0 solution.Comment: 8 page
Parity in the CMB: Space Oddity
We search for a direction in the sky that exhibits parity symmetry under
reflections through a plane. We use the natural estimator, which compares the
power in even and odd multipoles, and apply minimal blind masking of
outliers to the ILC map in order to avoid large errors in the reconstruction of
multipoles. The multipoles of the cut sky are calculated both naively and by
using the covariance inversion method and we estimate the significance of our
results using CDM simulations. Focusing on low multipoles, with or even 7, we find two perpendicular
directions of even and odd parity in the map. While the even parity direction
does not appear significant, the odd direction is quite significant -- at least
a effect.Comment: 6 pages, 7 figures. Accepted for publication in The Astrophysical
Journa
A stringy glimpse into the black hole horizon
We elaborate on the recent claim [arXiv:1702.03583] that non-perturbative
effects in , which are at the core of the FZZ duality, render the
region just behind the horizon of the black hole
singular already at the classical level (). We argue that the 2D
classical black hole could shed some light on quantum
black holes in higher dimensions including large black holes in
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