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A. Badalyan

Publications and source records attributed to A. Badalyan.

3 recordsLinked to original sources

Physics mechanisms of fines detachment and migration during CO2-water corefloods

One of the key risks for a Carbon Capture Storage (CCS) is injectivity decline. Evaporation of the connate brine in near-wellbore region during CO2 injection may result in drying-up the rock yielding the mobilisation and migration of clay particles leading to decline rock permeability and consequent loss of well injectivity. Influx of the reservoir brine into the dried-up zone yields accumulation of precipitated salt and injectivity decline. This paper presents the results of eight coreflooding experiments aiming investigation of the effect of rock dry-out, fines migration, and salt precipitation during CO2 injection. Pressure drops across the cores, brine saturation and produced clay fines concentration versus Pore Volume Injected (PVI) have been measured. All lab tests exhibit the following features: intensive fines production at the very beginning of gas-water production period following reduced-rate fines production during overall evaporation period and continuous fines disappearance at the late stage; abrupt increase in gas permeability in the middle of evaporation, and non-monotonic evaporation rate and pressure drop. To explain these phenomena, we distinguished three sequential regimes of fines detachment during two-phase displacement: (i) moving gas-water menisci; (ii) pendular rings of residual water; (iii) dry flux, and found that for the conditions of our corefloods, detachment is possible in regime (i) only. Fines production during overall evaporation period is explained by simultaneous occurrence of three regimes during unstable displacement of water by gas in micro-heterogeneous rock.

physics.geo-ph

Search for Eccentric Black Hole Coalescences during the Third Observing Run of LIGO and Virgo

Despite the growing number of confident binary black hole coalescences observed through gravitational waves so far, the astrophysical origin of these binaries remains uncertain. Orbital eccentricity is one of the clearest tracers of binary formation channels. Identifying binary eccentricity, however, remains challenging due to the limited availability of gravitational waveforms that include effects of eccentricity. Here, we present observational results for a waveform-independent search sensitive to eccentric black hole coalescences, covering the third observing run (O3) of the LIGO and Virgo detectors. We identified no new high-significance candidates beyond those that were already identified with searches focusing on quasi-circular binaries. We determine the sensitivity of our search to high-mass (total mass $M>70$ $M_\odot$) binaries covering eccentricities up to 0.3 at 15 Hz orbital frequency, and use this to compare model predictions to search results. Assuming all detections are indeed quasi-circular, for our fiducial population model, we place an upper limit for the merger rate density of high-mass binaries with eccentricities $0 < e \leq 0.3$ at $0.33$ Gpc$^{-3}$ yr$^{-1}$ at 90\% confidence level.

astro-ph.HE

Open data from the third observing run of LIGO, Virgo, KAGRA and GEO

The global network of gravitational-wave observatories now includes five detectors, namely LIGO Hanford, LIGO Livingston, Virgo, KAGRA, and GEO 600. These detectors collected data during their third observing run, O3, composed of three phases: O3a starting in April of 2019 and lasting six months, O3b starting in November of 2019 and lasting five months, and O3GK starting in April of 2020 and lasting 2 weeks. In this paper we describe these data and various other science products that can be freely accessed through the Gravitational Wave Open Science Center at https://gwosc.org. The main dataset, consisting of the gravitational-wave strain time series that contains the astrophysical signals, is released together with supporting data useful for their analysis and documentation, tutorials, as well as analysis software packages.

gr-qc