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Rotating and Oscillating Neutron Stars

1996
Since neutron stars are extremely compact objects with strong gravity, general relativity must be employed in modelling their properties. The structure and gravitational fields of spherically symmetric, nonrotating stars are governed by the Tolman-Oppenheimer-Volkoff equations, a set of ordinary differential equations.
openaire   +1 more source

Bifurcations in Non Oscillating Stars

1990
The equations of a polytropic gas sphere are studied from the point of view of similarity solutions and Quasi-Invariance transformations. Ordinary differential equations are obtained that generalize Emden’s equations. Critical points are seen to exist in most cases and lead to bifurcations in the density space.
openaire   +1 more source

Haematopoietic stem cell release is regulated by circadian oscillations

Nature, 2008
Simón Nm Méndez-Ferrer   +2 more
exaly  

Nonradial oscillations of stars

Astronomy Quarterly, 1979
openaire   +1 more source

Sub-cycle control of terahertz high-harmonic generation by dynamical Bloch oscillations

Nature Photonics, 2014
Christoph Lange   +2 more
exaly  

Metabolic co-dependence gives rise to collective oscillations within biofilms

Nature, 2015
Jintao Liu   +2 more
exaly  

Abnormal neural oscillations and synchrony in schizophrenia

Nature Reviews Neuroscience, 2010
Peter J Uhlhaas, Wolf Singer
exaly  

Oscillations, travelling fronts and patterns in a supramolecular system

Nature Nanotechnology, 2018
Jorge Leira-Iglesias   +2 more
exaly  

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