PTPlot: About
PTPlot is a tool for exploring the gravitational wave power spectrum from first-order phase transitions, and evaluating the likelihood of detecting a signal with the LISA mission.
- Plot single point and view the SNR and power spectra
- Plot multiple points given tabular data
- Browse and plot benchmark points for selected models
About the output
- All output figures
are Scalable
Vector Graphics (SVG) and can be downloaded and edited with
free tools such
as Inkscape. They are also
easily converted to PDF or bitmapped formats by Inkscape or
built-in OS tools, e.g.:
$ inkscape input_snr_file.svg --export-pdf=outpout_snr_file.pdf
Note that on Macos, Inkscape requires the full path to the source and destination files in order to work. - The CSV files that can be downloaded on 'single point' plotting pages contain the following columns (these are labeled on the first row): $$ f,\, h^2 \Omega_\text{sensitivity}, \, h^2 \Omega_\text{GW, sw},\, [h^2 \Omega_\text{GW, turb}, \, h^2 \Omega_\text{GW, tot} ]. $$ There is therefore no explicit dependence on the Hubble rate in the data.
Crediting PTPlot
The results plotted by this tool are based on the papers arXiv:1704.05871, Shape of the acoustic gravitational wave power spectrum from a first order phase transition (note the erratum) and arXiv:1910.13125, Detecting gravitational waves from cosmological phase transitions with LISA: an update. You are welcome to include plots from PTPlot in your own work; if you do use PTPlot, please cite at least:
- The above paper arXiv:1910.13125, as well as
- The Zenodo snapshot of the latest version, i.e. doi:10.5281/zenodo.6949107. This helps me track interest and usage of PTPlot in particular and justify its continued development.
Figures without the LISACosWG watermark are available on request; please do not remove it without permission.
Source
The source for PTPlot is available at https://bitbucket.org/dweir/ptplot. The code is provided under the Creative Commons Attribution 4.0 International license. Please see the section Crediting PTPlot, above.
Feedback, issues
Please get in touch with the author, David Weir [david.weir@helsinki.fi] or raise an issue on the issue tracker.
Recent news
- 1.8.2022 - version 1.0.2
- Relicensed under CC BY 4.0 International and made available on Zenodo with a DOI.
- Corrected value of sound wave power spectrum prefactor (per erratum of arXiv:1704.05871).
- Changes to appearance for readability.
- URLs which return SVG or CSV files now have the extension in the URL to make it a more pleasant experience when saving the file.
- Use
scipy.integrate.trapz
rather than some weird in-house code for calculating the integrated SNR.
- 5.3.2020 - version 1.0.1
- Can be installed with pip3 (for standalone use):
pip3 install --upgrade --git+https://dweir@bitbucket.org/dweir/ptplot.git
- Fixes a systematic error due to having logarithmically spaced data for the sensitivity curve, while eLISATools.py cannot cope with anything but evenly spaced points. Wrote a new replacement for the relevant commands that does numerical integration with an arbitrary interval.
- Fixed the value of $\tilde{\Omega}_\text{gw}$ from 0.12 to 0.012. This was due to a typo in arXiv:1704.05871 below Equation 45, which will be corrected in a forthcoming erratum.
- Power spectra and sensitivity data can now be downloaded as a CSV from individual point pages.
- Minor fixes due to changes in Django.
- Some improvements to the benchmark point database.
- Can be installed with pip3 (for standalone use):
- 7.11.2019 - version 1.0.0
- Coincides with release of paper [arXiv:1910.13125].
- Source data for plots now included in repo.
- Minor tick marks now shown.
- In plotting power spectra, only the sound wave curve is now shown (other curves remain available in the source code).
- Bugfixes, including: corrections to definition of $\kappa$ and a missing factor of $h^2$ in the sound wave GW power spectrum.
- 25.6.2019 - version 0.9.5
- 3- and 7- year mission durations available.
- Bugfixes to the "energy budget" calculation, which previously had some discrepancies at intermediate velocities.
- Axis labels cleaned up.
- "Theories" renamed to "Models" and another layer of granularity, "Scenarios", added to benchmark points.
- More flexibility in terms of individual points and scenarios having their own $T_*$ and $v_\mathrm{w}$.
- $\beta/H$ is now plotted (and used as a parameter) rather than $H/\beta$.
- 21.12.2018 - version 0.9.2
- The SNR curves and power spectra now use a single merged PowerSpectrum() class.
- All plots use a conservative form of the sound wave source where it has lifetime set either by the shock formation time or the Hubble time, whichever is shorter.
- All plots have a date and timestep to assist with debugging.
- Power spectrum plots have the SNR (from sound waves only) overplotted, too.
References
- arXiv:1512.06239 - Science with the space-based interferometer eLISA. II: Gravitational waves from cosmological phase transitions
- arXiv:1910.13125 - Detecting gravitational waves from cosmological phase transitions with LISA: an update
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