Results 11 to 20 of about 30,962 (264)

Wave dynamics and star formation in Taurus [PDF]

open access: yesSymposium - International Astronomical Union, 1991
The mechanism underlying the formation of cores and larger scale structures in molecular clouds must play a fundamental role in the physics of star formation since young stellar objects are usually found within or very near cores (Myers et al 1987, Beichman et al 1986).
Ralph E. Pudritz, Ana I. Gomez de Castro
openaire   +1 more source

Photons generated by gravitational waves in the near-zone of a neutron star

open access: yesNuclear Physics B, 2022
When a gravitational wave or a graviton travels through an electric or magnetic background, it could convert into a photon with some probability. In this paper, a dipole magnetic field is considered as this kind of background in both the Minkowski ...
Chao-Jun Feng   +3 more
doaj   +1 more source

Wave chaos in rapidly rotating stars [PDF]

open access: yesPhysical Review E, 2008
Effects of rapid stellar rotation on acoustic oscillation modes are poorly understood. We study the dynamics of acoustic rays in rotating polytropic stars and show using quantum chaos concepts that the eigenfrequency spectrum is a superposition of regular frequency patterns and an irregular frequency subset respectively associated with near-integrable ...
Lignieres, F., Georgeot, Bertrand
openaire   +4 more sources

Monster Radiative Shocks in the Perturbed Magnetospheres of Neutron Stars

open access: yesThe Astrophysical Journal, 2023
Magnetospheres of neutron stars can be perturbed by star quakes, interaction in a binary system, or sudden collapse of the star. The perturbations are typically in the kilohertz band and excite magnetohydrodynamic waves.
Andrei M. Beloborodov
doaj   +1 more source

Optical detection of the density-wave instability in the kagome metal KV3Sb5

open access: yesnpj Quantum Materials, 2022
Coexisting density-wave and superconducting states along with the large anomalous Hall effect in the absence of local magnetism remain intriguing and enigmatic features of the AV3Sb5 kagome metals (A = K, Rb, Cs).
Ece Uykur   +4 more
doaj   +1 more source

Observation of Star-Shaped Surface Gravity Waves [PDF]

open access: yesPhysical Review Letters, 2013
We report a new type of standing gravity wave of large amplitude, having alternatively the shape of a star and of a polygon. This wave is observed by means of a laboratory experiment by vertically vibrating a tank. The symmetry of the star (i.e., the number of branches) is independent of the container form and size, and can be changed according to the ...
Rajchenbach, Jean   +2 more
openaire   +4 more sources

Solution to the Dirichlet Problem of the Wave Equation on a Star Graph

open access: yesMathematics, 2023
In this paper, the solution to the Dirichlet problem for the wave equation on the star graph is constructed. To begin, we solve the boundary value problem on the interval (on one edge of the graph).
Gaukhar Arepova   +2 more
doaj   +1 more source

Detecting the Hadron-Quark Phase Transition with Gravitational Waves

open access: yesUniverse, 2019
The long-awaited detection of a gravitational wave from the merger of a binary neutron star in August 2017 (GW170817) marks the beginning of the new field of multi-messenger gravitational wave astronomy.
Matthias Hanauske   +9 more
doaj   +1 more source

Transmuted gravity wave signals from primordial black holes

open access: yesPhysics Letters B, 2018
Primordial black holes (PBHs) interacting with stars in binaries lead to a new class of gravity wave signatures that we explore. A small 10−16–10−7M⊙ PBH captured by a neutron star or a white dwarf will eventually consume the host.
Volodymyr Takhistov
doaj   +1 more source

A Brief Overview of Black Hole-Neutron Star Mergers

open access: yesFrontiers in Astronomy and Space Sciences, 2020
Of the three main types of binaries detectable through ground-based gravitational wave observations, black hole-neutron star (BHNS) mergers remain the most elusive.
Francois Foucart
doaj   +1 more source

Home - About - Disclaimer - Privacy