2,140 research outputs found
The Challenge Of Data Analysis For Future CMB Observations
Ongoing observations of the Cosmic Microwave Background, such as the MAXIMA
and BOOMERanG projects, are providing datasets of unprecedented quality and
ever-increasing size. Exact analysis of the data they produce is a serious
computational challenge, currently scaling as the number of sky pixels squared
in memory and cubed in time. Here we discuss the origins of these scaling
relations and their implications for our efforts to extract precise
cosmological parameters from observations of the CMB.Comment: 6 pages LaTeX (using aipproc2.sty & aipproc2.cls), to appear in
proceedings of `3K Cosmology Euroconference', Roma, ed F Melchiorr
Agent-Based Modeling: The Right Mathematics for the Social Sciences?
This study provides a basic introduction to agent-based modeling (ABM) as a powerful blend of classical and constructive mathematics, with a primary focus on its applicability for social science research.ďż˝ The typical goals of ABM social science researchers are discussed along with the culture-dish nature of their computer experiments. The applicability of ABM for science more generally is also considered, with special attention to physics. Finally, two distinct types of ABM applications are summarized in order to illustrate concretely the duality of ABM: Real-world systems can not only be simulated with verisimilitude using ABM; they can also be efficiently and robustly designed and constructed on the basis of ABM principles. ďż˝
A Semi-Analytical Analysis of Texture Collapse
This study presents a simplified approach to studying the dynamics of global
texture collapse. We derive equations of motion for a spherically symmetric
field configuration using a two parameter ansatz. Then we analyse the effective
potential for the resulting theory to understand possible trajectories of the
field configuration in the parameter space of the ansatz. Numerical results are
given for critical winding and collapse time in spatially flat non-expanding,
and flat expanding universes. In addition, the open non-expanding and
open-expanding cases are studied.Comment: 12 pages, figures available from author, BROWN-HET-895, uses phyzz
Absence of Open Strings in a Lattice-Free Simulation of Cosmic String Formation
Lattice-based string formation algorithms can, at least in principle, be reduced to the study of the statistics of the corresponding aperiodic random walk. Since in three or more dimensions such walks are transient, this approach necessarily generates a population of open strings. To investigate whether open strings are an artifact of the lattice we develop an alternative lattice-free simulation of string formation. Replacing the lattice with a graph generated by a minimal dynamical model of a first-order phase transition we obtain results consistent with the hypothesis that the energy density in string is due to a scale-invariant Brownian distribution of closed loops alone
Leadership Behaviour and Upward Feedback: Findings from a Longitudinal Intervention
A sample of 48 managers and 308 staff members of a community health care organization took part in a study to investigate the influence of participating in an upward feedback program on leadership behaviour, both as indicated be self-ratings and subordinatesââŹâ˘ ratings. The research design consisted of three measurement points within one year. The intervention included managers receiving upward feedback and a management skills workshop. The results showed a negative effect of the program on leadership behaviour as rated by the staff. Furthermore, managers reduced their self-ratings in the condition where they participated in both a feedback session and an management skills workshop.Management;Leadership Behaviour;Self-rating;Upward Feedback
Beyond the Small-Angle Approximation For MBR Anisotropy from Seeds
In this paper we give a general expression for the energy shift of massless
particles travelling through the gravitational field of an arbitrary matter
distribution as calculated in the weak field limit in an asymptotically flat
space-time. It is {\it not} assumed that matter is non-relativistic. We
demonstrate the surprising result that if the matter is illuminated by a
uniform brightness background that the brightness pattern observed at a given
point in space-time (modulo a term dependent on the oberver's velocity) depends
only on the matter distribution on the observer's past light-cone. These
results apply directly to the cosmological MBR anisotropy pattern generated in
the immediate vicinity of of an object like a cosmic string or global texture.
We apply these results to cosmic strings, finding a correction to previously
published results for in the small-angle approximation. We also derive the
full-sky anisotropy pattern of a collapsing texture knot.Comment: 23 pages, FERMILAB-Pub-94/047-
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