52,434 research outputs found
In What Sense Is the Early Universe Fine-Tuned?
It is commonplace in discussions of modern cosmology to assert that the early
universe began in a special state. Conventionally, cosmologists characterize
this fine-tuning in terms of the horizon and flatness problems. I argue that
the fine-tuning is real, but these problems aren't the best way to think about
it: causal disconnection of separated regions isn't the real problem, and
flatness isn't a problem at all. Fine-tuning is better understood in terms of a
measure on the space of trajectories: given reasonable conditions in the late
universe, the fraction of cosmological histories that were smooth at early
times is incredibly tiny. This discussion helps clarify what is required by a
complete theory of cosmological initial conditions.Comment: 28 pages. Prepared for a volume of essays commemorating David
Albert's Time and Chance, B. Loewer, E. Winsberg and B. Weslake, ed
Spoken word classification in children and adults
Purpose: Preschool children often have difficulties in word classification, despite good
speech perception and production. Some researchers suggest they represent words
using phonetic features rather than phonemes. We examine whether there is a
progression from feature based to phoneme based processing across age groups, and
whether responses are consistent across tasks and stimuli.
Method: In Study 1, 120 3 to 5 year old children completed three tasks assessing use of
phonetic features in classification, with an additional 58 older children completing
one of the three tasks. In Study 2, all of the children, together with an additional
adult sample, completed a nonword learning task.
Results: In all four tasks, children classified words sharing phonemes as similar. In
addition, children regarded words as similar if they shared manner of articulation,
particularly word-finally. Adults also showed this sensitivity to manner, but across
the tasks there was a pattern of increasing use of phonemic information with age.
Conclusions: Children tend to classify words as similar if they share phonemes or
share manner of articulation word finally. Use of phonemic information becomes
more common with age. These findings are in line with the theory that phonological
representations become more detailed in the preschool years
Aether compactification
We propose a new way to hide large extra dimensions without invoking branes, based on Lorentz-violating tensor fields with expectation values along the extra directions. We investigate the case of a single vector aether field on a compact circle. In such a background, interactions of other fields with the aether can lead to modified dispersion relations, increasing the mass of the Kaluza-Klein excitations. The mass scale characterizing each Kaluza-Klein tower can be chosen independently for each species of scalar, fermion, or gauge boson. No small-scale deviations from the inverse square law for gravity are predicted, although light graviton modes may exist
Bulk Entanglement Gravity without a Boundary: Towards Finding Einstein's Equation in Hilbert Space
We consider the emergence from quantum entanglement of spacetime geometry in
a bulk region. For certain classes of quantum states in an appropriately
factorized Hilbert space, a spatial geometry can be defined by associating
areas along codimension-one surfaces with the entanglement entropy between
either side. We show how Radon transforms can be used to convert this data into
a spatial metric. Under a particular set of assumptions, the time evolution of
such a state traces out a four-dimensional spacetime geometry, and we argue
using a modified version of Jacobson's "entanglement equilibrium" that the
geometry should obey Einstein's equation in the weak-field limit. We also
discuss how entanglement equilibrium is related to a generalization of the
Ryu-Takayanagi formula in more general settings, and how quantum error
correction can help specify the emergence map between the full quantum-gravity
Hilbert space and the semiclassical limit of quantum fields propagating on a
classical spacetime.Comment: 29 pages, 2 figure
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