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We present a detailed analysis of the X-ray/IR fast variability of the Black-Hole Transient GX 339-4 during its low/hard state in August 2008. Thanks to simultaneous high time-resolution observations made with the VLT and RXTE, we performed…

High Energy Astrophysical Phenomena · Physics 2018-03-28 F. M. Vincentelli , P. Casella , T. J. Maccarone , P. Uttley , P. Gandhi , T. Belloni , B. De Marco , D. M. Russell , L. Stella , K. O'Brien

We present a new release of the RELTRANS model to fit the complex cross-spectrum of accreting black holes as a function of energy. The model accounts for continuum lags and reverberation lags self-consistently in order to consider the…

QPOs are a common feature in the X-ray power density spectrum of black hole binaries and a potentially powerful tool to probe the spacetime geometry around these objects. Here we discuss their constraining power to test the Kerr black hole…

General Relativity and Quantum Cosmology · Physics 2016-12-22 Cosimo Bambi , Sourabh Nampalliwar

In some models of quantum gravity, space-time is thought to have a foamy structure with non-trivial optical properties. We probe the possibility that photons propagating in vacuum may exhibit a non-trivial refractive index, by analyzing the…

Astrophysics · Physics 2008-11-26 J. Ellis , N. E. Mavromatos , D. V. Nanopoulos , A. S. Sakharov

We study the influence of different kinds of gaps in a quasiparticle spectrum on longitudinal and transverse optical conductivities of bilayer graphene. An exact analytical expression for magneto-optical conductivity is derived using a…

Strongly Correlated Electrons · Physics 2012-08-08 E. V. Gorbar , V. P. Gusynin , A. B. Kuzmenko , S. G. Sharapov

In this paper, we examine the motion of test particles and relativistic accretion mechanisms within the spacetime of a rotating and embedded BH. In this case, the geometric properties of the metric and their dynamical consequences for…

High Energy Astrophysical Phenomena · Physics 2026-02-06 Asifa Ashraf , Orhan Donmez , Abdelmalek Bouzenada , Chengxun Yuan , Aylin Caliskan , Gulzoda Rakhimova , Ahmadjon Abdujabbarov

Symmetry is a cornerstone of condensed matter physics, fundamentally shaping the behavior of electronic systems and inducing the emergence of novel phenomena. The Hall effect, a key concept in this field, demonstrates how symmetry breaking,…

Mesoscale and Nanoscale Physics · Physics 2025-04-29 Shuo Wang , Wei Niu , Yue-Wen Fang

We have started a long-term reverberation mapping project using the Wyoming Infrared Observatory 2.3 meter telescope titled "Monitoring AGNs with H\beta\ Asymmetry" (MAHA). The motivations of the project are to explore the geometry and…

We conduct X-ray reverberation mapping and spectral analysis of the radio galaxy Centaurus A to uncover its central structure. We compare the light curve of the hard X-ray continuum from Swift Burst Alert Telescope observations with that of…

High Energy Astrophysical Phenomena · Physics 2025-02-12 Toshiya Iwata , Atsushi Tanimoto , Hirokazu Odaka , Aya Bamba , Yoshiyuki Inoue , Kouichi Hagino

In this article we introduce a technique for finding resonance radii in a disk galaxy. We use a two-dimensional velocity field in H{\alpha} emission obtained with Fabry-Perot interferometry, derive the classical rotation curve, and subtract…

Astrophysics of Galaxies · Physics 2015-05-30 Joan Font , John E. Beckman , Benoît Epinat , Kambiz Fathi , Leonel Gutiérrez , Olivier Hernandez

The improvement of the calibration relation for determining the size of the broad-line region from the observed optical luminosity of active galactic nuclei (AGN) is a necessary task to study fundamental parameters of distant AGNs such as…

We have explored spectral line profiles due to spiral patterns in accretion discs around black holes. A parametrization was employed for the shape and emissivity of spiral waves, which can be produced by non-axisymmetric perturbations…

Astrophysics · Physics 2015-06-24 V. Karas , A. Martocchia , L. Subr

We present that the broad feature usually observed in X-ray spectra can be explained by a ray-traced emission from a two-slab system containing a dissipative, warm corona on top of an accretion disk in an AGN. Such an accretion flow is…

High Energy Astrophysical Phenomena · Physics 2026-03-11 P. P. Biswas , A. Różańska , F. H. Vincent , D. Lančová , P. T. Zycki

We present results from infrared spectroscopic projects that aim to test the relation between the mass of a black hole, M_BH, and the velocity dispersion of the stars in its host-galaxy bulge. We demonstrate that near-infrared,…

Cosmology and Nongalactic Astrophysics · Physics 2010-01-26 K. M. Dasyra , B. M. Peterson , L. J. Tacconi , H. Netzer , L. C. Ho , G. Helou , L. Armus , D. Lutz , R. Davies , L. Watson

Understanding the geometry and kinematics of the broad line region (BLR) of active galactic nuclei (AGN) is important to estimate black hole masses in AGN and study the accretion process. The technique of reverberation mapping (RM) has…

Astrophysics of Galaxies · Physics 2021-01-13 Amit Kumar Mandal , Suvendu Rakshit , C. S. Stalin , R. G. Petrov , Blesson Mathew , Ram Sagar

We explore the observational implications of a large systematic study of high-resolution three dimensional simulations of radio galaxies driven by supersonic jets. For this fiducial study, we employ non-relativistic hydrodynamic adiabatic…

Astrophysics of Galaxies · Physics 2019-09-10 Michael D. Smith , Justin Donohoe

Patterning and defect engineering are key methods to tune 2D materials' properties. However, generating 2D periodic patterns of point defects in 2D materials has been elusive until now, despite the well-established methods for creating…

We study the time reversal and space inversion symmetry properties of those transfer matrices mostly used in the calculation of energy spectra and transport-process. We study the time reversal and space inversion symmetry properties of…

Mesoscale and Nanoscale Physics · Physics 2007-05-23 L. Diago-Cisneros , H. Rodriguez-Coppola , R. Perez-Alvarez , P. Pereyra

Ultrashort laser pulse filaments in dispersive nonlinear Kerr media induce a moving refractive index perturbation which modifies the space-time geometry as seen by co-propagating light rays. We study the analogue geometry induced by the…

General Relativity and Quantum Cosmology · Physics 2010-02-23 D. Faccio , S. Cacciatori , V. Gorini , V. G. Sala , A. Averchi , A. Lotti , M. Kolesik , J. V. Moloney

Optical observations cannot resolve the structure of active galactic nuclei (AGN), and a unified model for AGN was inferred mostly from indirect methods. Optical reverberation mapping allowed us to constrain the spatial dimension of the…

High Energy Astrophysical Phenomena · Physics 2017-12-05 P. A. Rojas Lobos , R. W. Goosmann , F. Marin , D. Savić