52,614 research outputs found
The human and mammalian cerebrum scale by computational power and information resistance
The cerebrum of mammals spans a vast range of sizes and yet has a very
regular structure. The amount of folding of the cortical surface and the
proportion of white matter gradually increase with size, but the underlying
mechanisms remain elusive. Here, two laws are derived to fully explain these
cerebral scaling relations. The first law holds that the long-range information
flow in the cerebrum is determined by the total cortical surface (i.e., the
number of neurons) and the increasing information resistance of long-range
connections. Despite having just one free parameter, the first law fits the
mammalian cerebrum better than any existing function, both across species and
within humans. According to the second law, the white matter volume scales,
with a few minor corrections, to the cortical surface area. It follows from the
first law that large cerebrums have much local processing and little global
information flow. Moreover, paradoxically, a further increase in long-range
connections would decrease the efficiency of information flow.Comment: 15 pages, 2 figures; 3 supplement
Detection of Gravitational Waves from Inflation
Recent measurements of temperature fluctuations in the cosmic microwave
background (CMB) indicate that the Universe is flat and that large-scale
structure grew via gravitational infall from primordial adiabatic
perturbations. Both of these observations seem to indicate that we are on the
right track with inflation. But what is the new physics responsible for
inflation? This question can be answered with observations of the polarization
of the CMB. Inflation predicts robustly the existence of a stochastic
background of cosmological gravitational waves with an amplitude proportional
to the square of the energy scale of inflation. This gravitational-wave
background induces a unique signature in the polarization of the CMB. If
inflation took place at an energy scale much smaller than that of grand
unification, then the signal will be too small to be detectable. However, if
inflation had something to do with grand unification or Planck-scale physics,
then the signal is conceivably detectable in the optimistic case by the Planck
satellite, or if not, then by a dedicated post-Planck CMB polarization
experiment. Realistic developments in detector technology as well as a proper
scan strategy could produce such a post-Planck experiment that would improve on
Planck's sensitivity to the gravitational-wave background by several orders of
magnitude in a decade timescale.Comment: 13 page, 4 figures. To appear in the proceedings of DPF2000,
Columbus, 9-12 August 2000 and (with slight revisions) in the proceedings of,
"Gravitational Waves: A Challenge to Theoretical Astrophysics," Trieste, 5-9
June 200
Home biased? : A spatial analysis of the domestic merging behavior of US firms
Using data of US domestic mergers and acquisitions transactions, this paper shows that acquirers have a preference for geographically proximate target companies. We measure the ‘home bias’ against benchmark portfolios of hypothetical deals where the potential targets consist of firms of similar size in the same four-digit SIC code that have been targets in other transactions at about the same time or firms that have been listed at a stock exchange at that time. There is a strong and consistent home bias for M&A transactions in the US, which is significantly declining during the observation period, i.e. between 1990 and 2004. At the same time, the average distances between target and acquirer increase articulately. The home bias is stronger for small and relatively opaque target companies suggesting that local information is the decisive factor in explaining the results. Acquirers that diversify into new business lines also display a stronger preference for more proximate targets. With an event study we show that investors react relatively better to proximate acquisitions than to distant ones. That reaction is more important and becomes significant in times when the average distance between target and acquirer becomes larger, but never becomes economically significant. We interpret this as evidence for the familiarity hypothesis brought forward by Huberman (2001): Acquirers know about the existence of proximate targets and are more likely to merge with them without necessarily being better informed. However, when comparing the best and the worst deals, we are able to show a dramatic difference in distances and home bias: The most successful deals display on average a much stronger home bias and distinctively smaller distance between acquirer and target than the least successful deals. Proximity in M&A transactions therefore is a necessary but not sufficient condition for success. The paper contributes to the growing literature on the role of distance in financial decisions
Reproductive biology of carpenter seabream (Argyrozona argyrozona) (Pisces: Sparidae) in a marine protected area
The carpenter seabream (Argyrozona argyrozona) is an
endemic South African sparid that comprises an important part of the handline fishery. A three-year study (1998−2000) into its reproductive biology within the Tsitsikamma National Park revealed that these fishes are
serial spawning late gonochorists. The size at 50% maturity (L50) was estimated at 292 and 297 mm FL for both females and males, respectively. A likelihood ratio test revealed that there was no significant difference between male and female L50 (P>0.5). Both monthly gonadosomatic indices
and macroscopically determined ovarian stages strongly indicate that A. argyrozona within the Tsitsikamma
National Park spawn in the astral summer between November and April. The presence of postovulatory follicles (POFs) confirmed a six-month spawning season, and monthly proportions of early (0−6 hour old) POFs showed that spawning frequency was highest (once every 1−2 days) from December to March. Although spawning season was more highly correlated to photoperiod (r = 0.859) than temperature
(r = −0.161), the daily proportion of spawning fish was strongly correlated (r= 0.93) to ambient temperature over
the range 9−22oC. These results indicate that short-term upwelling events, a strong feature in the Tsitsikamma
National Park during summer, may negatively affect carpenter fecundity. Both spawning frequency and duration
(i.e., length of spawning season) increased with fish length. As a result of the allometric relationship between
annual fecundity and fish mass a 3-kg fish was calculated to produce fivefold more eggs per kilogram of body weight
than a fish of 1 kg. In addition to producing more eggs per unit of weight each year, larger fish also produce
significantly larger eggs
Simple model for the Darwinian transition in early evolution
It has been hypothesized that in the era just before the last universal
common ancestor emerged, life on earth was fundamentally collective. Ancient
life forms shared their genetic material freely through massive horizontal gene
transfer (HGT). At a certain point, however, life made a transition to the
modern era of individuality and vertical descent. Here we present a minimal
model for this hypothesized "Darwinian transition." The model suggests that
HGT-dominated dynamics may have been intermittently interrupted by
selection-driven processes during which genotypes became fitter and decreased
their inclination toward HGT. Stochastic switching in the population dynamics
with three-point (hypernetwork) interactions may have destabilized the
HGT-dominated collective state and led to the emergence of vertical descent and
the first well-defined species in early evolution. A nonlinear analysis of a
stochastic model dynamics covering key features of evolutionary processes (such
as selection, mutation, drift and HGT) supports this view. Our findings thus
suggest a viable route from early collective evolution to the start of
individuality and vertical Darwinian evolution, enabling the emergence of the
first species.Comment: 9 pages, 5 figures, under review at Physical Review
Examples of scalar-flat hypersurfaces in
Given a hypersurface of null scalar curvature in the unit sphere
, , such that its second fundamental form has rank
greater than 2, we construct a singular scalar-flat hypersurface in \Rr^{n+1}
as a normal graph over a truncated cone generated by . Furthermore, this
graph is 1-stable if the cone is strictly 1-stable.Comment: Paper accepted to publication in Manuscripta Mathematic
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