328 research outputs found
Evidence of Cosmic Strings by the Observation of the Alignment of Quasar Polarization Axes
The recently found alignment of the polarization axes of quasars in large quasar groups on Mpc scales, can be explained by general relativistic cosmic string networks. The emergent azimuthal-angle dependency in our model can be used to explain the aligned polarization axes in large quasar groups on Mpc scales. Spin axis direction perpendicular to the major axes of large quasar groups when the richness decreases, can be explained as a second order effect in our approximation scheme by the higher multiplicity terms. When more data of quasars of high redshift will become available, one could proof that the alignment emerged after the symmetry breaking scale and must have a cosmological origin
How early does attention modulate visual information processing? The importance of experimental protocol and data analysis approach
No Evidence that Predictions and Attention Modulate the First Feedforward Sweep of Cortical Information Processing
Exploring the role of expectations and stimulus relevance on stimulus-specific neural representations and conscious report
High-Frequency Gravitational Waves from Spinning Non-Abelian Cosmic-Strings
We investigated the SU(2) Einstein-Yang-Mills system on a time-dependent
non-diagonal cylindrical symmetric space-time. From the numerical
investigation, wave-like solutions are found, consistent with the familiar
string-like features. They possess an angle-deficit which depends on the
initial form of the magnetic component of the YM field, i.e., the number of
times it crosses the r-axis. The soliton-like behavior of the gravitational and
YM waves show significant differences from the ones found in the
Einstein-Maxwell system. The stability of the system is analyzed using the
multiple-scale method. To first order a consistent set of equations is
obtained.Comment: 26 pages in Revtex+ 10 eps figures. The other pictures can be
obtained at http://www.asfyon.nl/slagt.html/webdoc.ht
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