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Dataset results
12 results for “Numerical Relativity”
Precessing binary-black-hole numerical relativity catalogue (minimal data release)
<p>This page contains the minimal data release associated with the catalogue presented in <a href="https://dcc.ligo.org/DocDB/0186/P2300054/001/catalogue.pdf">A catalogue of precessing black-hole-binary numerical-relativity simulations</a>. This catalogue contains 80 single-spin precessing black-hole-binary configurations. </p> <p>The content of the data release is described <a href="https://data.cardiffgravity.org/bam-catalogue/">here</a>, along with instructions on how to parse the data.</p>
Precessing binary-black-hole numerical relativity catalogue (complete data release)
<p>This page contains the minimal data release associated with the catalogue presented in <a href="https://dcc.ligo.org/DocDB/0186/P2300054/001/catalogue.pdf">A catalogue of precessing black-hole-binary numerical-relativity simulations</a>. This catalogue contains 80 single-spin precessing black-hole-binary configurations. </p> <p>The content of the data release is described <a href="https://data.cardiffgravity.org/bam-catalogue/">here</a>, along with instructions on how to parse the data.</p>
Dataset related to Balazs et al. The dynamics of forearc – back-arc basin subsidence: numerical models and observations from Mediterranean subduction zones
<p>Additional model data to publication by Balazs et al. The dynamics of forearc – back-arc basin subsidence: numerical models and observations from Mediterranean subduction zones</p>
PlaSim output data from TSI-related numerical experiments
<p>Dear Visitor,<br> <br> Here you can access all the output of the PlaSim simulations in netCDF format.<br> <br> The form of the file names is as follows:<br> <br> TS_History#_m0##.nc<br> <br> , where TS abbreviates surface temperature, # refers to the particular<br> forcing history (C, B, Ta, Tb, N) and ## denotes numbers from 1 to 40.</p>
PlaSim output data from TSI-related numerical experiments
<p>Dear Visitor,</p> <p>Here you can access all the output of the PlaSim simulations in netCDF format.</p> <p>The form of the file names is as follows:</p> <p>TS_History#_m0##.nc</p> <p>, where TS abbreviates surface temperature, # refers to the particular<br> forcing history (C, B, Ta, Tb, N) and ## denotes numbers from 1 to 40.</p>
PlaSim output data from TSI-related numerical experiments
<p>Dear Visitor,</p> <p>Here you can access all the output of the PlaSim simulations in netCDF format.</p> <p>The form of the file names is as follows:</p> <p>TS_History#_m0##.nc</p> <p>, where TS abbreviates surface temperature, # refers to the particular<br> forcing history (C, B, Ta, Tb, N) and ## denotes numbers from 1 to 40.</p>
PlaSim output data from TSI-related numerical experiments
<p>Dear Visitor,<br> <br> Here you can access all the output of the PlaSim simulations in netCDF format.<br> <br> The form of the file names is as follows:<br> <br> TS_History#_m0##.nc<br> <br> , where TS abbreviates surface temperature, # refers to the particular<br> forcing history (C, B, Ta, Tb, N) and ## denotes numbers from 1 to 40</p>
PlaSim output data from TSI-related numerical experiments
<p>Dear Visitor,<br> <br> Here you can access all the output of the PlaSim simulations in netCDF format.<br> <br> The form of the file names is as follows:<br> <br> TS_History#_m0##.nc<br> <br> , where TS abbreviates surface temperature, # refers to the particular<br> forcing history (C, B, Ta, Tb, N) and ## denotes numbers from 1 to 40.</p>
Waveform data for Gravitational waveforms for high spin and high mass-ratio binary black holes: A synergistic use of numerical-relativity codes
<p>This dataset consists of binary black hole waveforms for three different configurations</p> <p>* q=3, chi1=chi2=0.9<br> * q=4, chi1=chi2=0.9<br> * q=5, chi1=chi2=0.9</p> <p>where q = m1/m2 is the ratio of the black hole masses, and chi1 and chi2 are the dimensionless spins of the black holes, oriented parallel to and in the direction of the orbital angular momentum.</p> <p>The waveforms are computed using the 3-dimensional numerical relativity simulation codes</p> <p> SpEC (SPectral Einstein Code -- https://www.black-holes.org/code/SpEC.html)<br> ET (Einstein Toolkit -- https://einsteintoolkit.org)</p> <p>SpEC is computationally efficient and accurate, and produces long waveforms, but in these cases, the simulations crash at the merger. The ET is less computationally efficient and accurate, but the simulations complete successfully. We therefore combine long SpEC inspirals with short ET mergers, blending the waveforms to produce hybrid waveforms.</p> <p>The waveform data directories are named as follows:</p> <p>q=3,chi1=chi2=0.9:<br> SpEC: q3_0.9_0.9_r200<br> ET: ceas_22_e5_2<br> Hybrid: q3_0.9_0.9_r200_hyb_ceas_22_e5_2</p> <p>q=4,chi1=chi2=0.9:<br> SpEC: q4_0.9_0.9_EccNew<br> ET: ceas_20_5_e7<br> Hybrid: q4_0.9_0.9_EccNew_hyb_ceas_20_5_e7</p> <p>q=5,chi1=chi2=0.9:<br> SpEC: q5.0_s0_0_0.9_s0_0_0.9_r200<br> ET: ceas_23_e5_2<br> Hybrid: q5.0_s0_0_0.9_s0_0_0.9_r200_hyb_ceas_23_e5_2</p> <p>The data is in the SXS simulation format (https://data.black-holes.org/waveforms/documentation.html), though only a subset of the SXS-format data is present.</p> <p>Also included is a Mathematica notebook, HybridizeWaveforms.nb, showing how the hybrid can be computed from the separate inspiral and merger waveforms using the open source SimulationTools code (https://simulationtools.org).</p> <p>See the paper</p> <p> I. Hinder, S. Ossokine, H. Pfeiffer and A. Buonanno -- Gravitational waveforms for high spin and high mass-ratio binary black holes: A synergistic use of numerical-relativity codes</p> <p>for more details.</p>
3D HDF5 data from numerical relativity simulations
<p>3D HDF5 data from numerical relativity simulations. Test data for visualization purposes.</p>
Investigating the velocity of magmatic intrusions and its relation with rock fracture toughness: insights from laboratory experiments and numerical models
<p>This repository provides compressed folders containing the velocity profiles recorded during our oil-filled crack propagation experiments and the code used to simulate those experiments. In particular, the files in compressed folders <strong>10ml</strong>, <strong>30ml</strong>, <strong>50ml</strong> and <strong>others_ml</strong> contain two columns corresponding to the tracked cracks' depth [m] and velocity [m/s]. The two folders <strong>DYKE-CODE_constant-Ef</strong> and <strong>DYKE-CODE_variable-Ef</strong> contain the Fortran90 code, the input and output files, and all the scripts needed to reproduce the simulations and the plots displayed in Figure 3 and Figure 4 of the article <em>"</em>Investigating the velocity of magmatic intrusions and its relation with rock fracture toughness: insights from laboratory experiments and numerical models<em>"</em><strong><em> </em></strong> by A. Gaete, F. Maccaferri, S. Furst, and V. Pinel.</p>
Dataset related to article "Numerical Activities of Daily Living – Financial: a short version"
<p>Il dataset contiene i seguenti dati:</p> <ul> <li>colonne B, C, D: i dati socio-demografici dei soggetti, riportati nell’articolo in Tabella 1;</li> <li>colonna E: punteggi grezzi dei soggetti al test MMSE, utilizzati nelle analisi riportate in Tabella 5;</li> <li>colonne dalla F alla CE: punteggi ottenuti al test NADL-F originale e short, utilizzati per le analisi riportate nelle tabelle 3, 4 e 5.</li> </ul>
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