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Galaxies, Volume 9, Issue 3

September 2021 - 23 articles

Cover Story: The suppression of displacements and angular motion of test masses by seismic isolation and control systems is one of the main challenges for the operation of gravitational-wave detectors. There was strong evidence during the last observation run of the Advanced LIGO detectors that noise associated with residual angular motion of the test masses led to sensitivity limitations below a few tens of Hertz. Angular motion of test masses is notoriously difficult to model since it gains relevance mostly through non-linear dynamics of a complex system. With Lightsaber, we present a first nonlinear, time-domain simulation of these dynamics with realistic noise inputs. Detailed comparisons between Lightsaber simulations and observations will hopefully lead to an improved understanding of this noise and help to develop methods to reduce it. View this paper
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Articles (23)

  • Article
  • Open Access
6 Citations
2,973 Views
14 Pages

15 September 2021

The prompt emission of most gamma-ray bursts (GRBs) typically exhibits a non-thermal Band component. The synchrotron radiation in the popular internal shock model is generally put forward to explain such a non-thermal component. However, the low-ener...

  • Review
  • Open Access
40 Citations
4,766 Views
30 Pages

13 September 2021

Driven by the increasingly complete observational knowledge of systems of satellite galaxies, mutual spatial alignments and relations in velocities among satellites belonging to a common host have become a productive field of research. Numerous studi...

  • Article
  • Open Access
11 Citations
3,292 Views
17 Pages

13 September 2021

Recently, microquasar jets have aroused the interest of many researchers focusing on the astrophysical plasma outflows and various jet ejections. In this work, we concentrate on the investigation of electromagnetic radiation and particle emissions fr...

  • Article
  • Open Access
35 Citations
4,699 Views
22 Pages

Regular Bardeen Black Holes in Anti-de Sitter Spacetime versus Kerr Black Holes through Particle Dynamics

  • Bakhtiyor Narzilloev,
  • Javlon Rayimbaev,
  • Ahmadjon Abdujabbarov and
  • Bobomurat Ahmedov

6 September 2021

In this work, test particle dynamics around a static regular Bardeen black hole (BH) in Anti-de Sitter spacetime has been studied. It has been shown for neutral test particles that parameters of a regular Bardeen black hole in Anti-de Sitter spacetim...

  • Article
  • Open Access
3 Citations
2,509 Views
14 Pages

6 September 2021

A theoretical investigation is carried out to study the propagation properties of ion acoustic shocks in a plasma comprising of positive inertial ions, weakly relativistic ion beam and trapped electrons in the presence of a quantizing magnetic field....

  • Article
  • Open Access
20 Citations
2,975 Views
10 Pages

Capture of Massless and Massive Particles by Parameterized Black Holes

  • Bobir Toshmatov,
  • Ozodbek Rahimov,
  • Bobomurat Ahmedov and
  • Abdumirhakim Ahmedov

6 September 2021

We study an influence of the leading coefficient of the parameterized line element of the spherically symmetric, static black hole on the capture of massless and massive particles. We have shown that negative (positive) values of ϵ decreases (increas...

  • Article
  • Open Access
6 Citations
3,602 Views
22 Pages

5 September 2021

The suspended test masses of gravitational-wave (GW) detectors require precise alignment to be able to operate the detector stably and with high sensitivity. This includes the continuous counter-acting of seismic disturbances, which, below a few Hert...

  • Article
  • Open Access
7 Citations
2,470 Views
20 Pages

5 September 2021

Polarized synchrotron emission from the radio halos of diffuse intracluster medium (ICM) in galaxy clusters are yet to be observed. To investigate the expected polarization in the ICM, we use high resolution (1 kpc) magnetohydrodynamic simulations of...

  • Review
  • Open Access
80 Citations
5,930 Views
29 Pages

31 August 2021

Not all the light in galaxy groups and clusters comes from stars that are bound to galaxies. A significant fraction of it constitutes the so-called intracluster or diffuse light (ICL), a low surface brightness component of groups/clusters generally f...

  • Article
  • Open Access
6 Citations
2,423 Views
8 Pages

30 August 2021

The Zipoy-Voorhees solution is known as the γ-metric and/or q-metric being static and axisymmetric vacuum solution of Einstein field equations which becomes strong curvature naked singularity. The metric is characterized by two parameters, namely, th...

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Galaxies - ISSN 2075-4434