Stellar pulsation is nowadays a widely understood subject. However, there has been no research about the effects of pulsations on the star's orbital dynamics throughout the galaxy. We investigate whether these oscillations can cause chaotic behaviour in the stellar orbit if it is immersed in background dark matter halos. We show that for a certain range of parameters of the pulsating object these effects are present in a general background matter field. However, for the typical range of parameters of realistic astrophysical scenarios, these effects are too small to be detectable.Comment: 6 pages, 4 figure
The ultra-light dark matter (ULDM) model has become a popular dark matter scenario nowadays. The mas...
Many dynamical models of the Milky Way halo require assumptions that the distribution function of a ...
Aims. The distinction between regular and chaotic motion in galaxies is undoubtedly an iss...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2019, Tutor: ...
In a previous paper based on dark matter only simulations we show that, in the approximation of an a...
In a previous paper based on dark matter only simulations we show that, in the approximation of an a...
Indexación: Web of ScienceStudies of dynamical stability (chaotic versus regular motion) in galactic...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Any: 2015, Tutor: A...
We show that diffusion due to chaotic mixing in the neighbourhood of the Sun may not be as relevant ...
We investigate the chaotic behavior of the S-star cluster in the Galactic center using precise $N$-b...
Dark matter (DM) can consist of very light bosons behaving as a classical scalar field that experien...
Using realistic cosmological simulations of Milky Way sized haloes, we study their dynamical state a...
This paper is concerned with the mathematical description of orbits that do not have a constant cent...
In this dissertation, we develop two novel methods for studying the nature of the Milky Way's dark m...
Observations show that stellar streams originating in satellite dwarf galaxies are frequent in the U...
The ultra-light dark matter (ULDM) model has become a popular dark matter scenario nowadays. The mas...
Many dynamical models of the Milky Way halo require assumptions that the distribution function of a ...
Aims. The distinction between regular and chaotic motion in galaxies is undoubtedly an iss...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2019, Tutor: ...
In a previous paper based on dark matter only simulations we show that, in the approximation of an a...
In a previous paper based on dark matter only simulations we show that, in the approximation of an a...
Indexación: Web of ScienceStudies of dynamical stability (chaotic versus regular motion) in galactic...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Any: 2015, Tutor: A...
We show that diffusion due to chaotic mixing in the neighbourhood of the Sun may not be as relevant ...
We investigate the chaotic behavior of the S-star cluster in the Galactic center using precise $N$-b...
Dark matter (DM) can consist of very light bosons behaving as a classical scalar field that experien...
Using realistic cosmological simulations of Milky Way sized haloes, we study their dynamical state a...
This paper is concerned with the mathematical description of orbits that do not have a constant cent...
In this dissertation, we develop two novel methods for studying the nature of the Milky Way's dark m...
Observations show that stellar streams originating in satellite dwarf galaxies are frequent in the U...
The ultra-light dark matter (ULDM) model has become a popular dark matter scenario nowadays. The mas...
Many dynamical models of the Milky Way halo require assumptions that the distribution function of a ...
Aims. The distinction between regular and chaotic motion in galaxies is undoubtedly an iss...