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| The LIGO journal club usually meets at 3:00PM on Fridays on 2nd floor of W Bridge (room 265). We meet to discuss a recent journal article from PRL, ApJ or the like. Someone is designated as a lead, to initiate the discussion, but not to present slides or give a monologue. The lead should also post a link to the article the Tuesday before meeting in the [[#Meetings and papers|Meetings and papers]] section below. | |
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| Journal club meetings are held weekly on ???days at ??:?? PM. | Preferably, selected articles won't be exceptionally long, and would relate (at least tangentially) to LIGO. You will be emailed by the journal club Tsar two weeks out from your date and again a week out. The rotating roster can be found at [[https://docs.google.com/spreadsheets/d/1TxTmFStB9jT1xCvscr5xKY5ovuA4nme58XK4IrqI6_0/edit?usp=sharing| HERE ]] == Mailing List == To send emails to everyone: ligo-journal-club@caltech.edu Click here to [[https://lists.caltech.edu/listinfo/ligo-journal-club|subscribe]] == Meetings and papers == || '''Date''' || '''Lead''' || '''Link (pre-print or other open format) and other links''' || '''Link (official DOI peer reviewed version)''' || '''Attendance ''' || || 2020 Jan 24 || Aidan || [[https://arxiv.org/abs/2001.05712]], "Multi-node optical frequency dissemination with post automatic phase correction" || || || || 2020 Jan 17 || Lilli || [[https://arxiv.org/abs/1912.04903]] || || || || 2020 Jan 10 || Koji || [[https://arxiv.org/abs/1905.06308| arxiv:nucl-ex/1905.06308]] || [[ https://doi.org/10.1038/s41586-019-1533-4 | Energy of the 229Th nuclear clock transition ]] || || || 2019 Dec 20 || Yehonathan || [[https://journals.aps.org/prx/abstract/10.1103/PhysRevX.9.041025]] || [[ https://journals.aps.org/prx/abstract/10.1103/PhysRevX.9.041025 | Nanorheology of Interfacial Water during Ice Gliding ]] || || || 2019 Dec 13 || Gabriele || [[https://arxiv.org/abs/1912.04825 | arXiv:cs-LG/1912.04825]] || [[ | Integration of Neural Network-Based Symbolic Regression in Deep Learning for Scientific Discovery ]] || || || 2019 Dec 06 || Shruti || [[https://arxiv.org/abs/quant-ph/0412078 | arXiv:quant-ph/0412078]] || [[ https://science.sciencemag.org/content/306/5700/1330 | Quantum-Enhanced Measurements: Beating the Standard Quantum Limit ]] || 8 || || 2019 Nov 22 || Anchal || [[https://arxiv.org/abs/1511.04021 | Arxiv Pre-print]] || [[ https://link.springer.com/article/10.1007/JHEP02(2016)004 | Chaos in quantum channels ]] || 5 || || 2019 Nov 15 || Rana || [[ https://doi.org/10.1038/s41586-019-1256-6 | Revsiting Cold Fusion ]] || [[https://www.nature.com/articles/d41586-019-01675-9 | Commentary]] || || || 2019 Nov 8 || Chris || [[https://doi.org/10.1038/s41467-019-11579-x | Bell's theorem for temporal order]] || || || || 2019 Oct 31 || Raymond || [[https://journals.aps.org/prl/pdf/10.1103/PhysRevLett.121.261302 | Piezoelectrically Tuned Multimode Cavity Search for Axion Dark Matter]] || || || || 2019 Oct 11 || Shreya || [[https://arxiv.org/pdf/1712.06615.pdf | Gravitational Probes of Dark Matter Physics]] || || || || 2019 Oct 4 || Jon || [[https://arxiv.org/abs/1906.06193 | Novel signatures of dark matter in laser-interferometric gravitational-wave detectors]] || || || || 2019 Sep 27 || Duo || [[https://www.pnas.org/content/115/9/1992 | https://www.pnas.org/content/115/9/1992]] || || || || 2019 Sep 13 || Aaron || [[https://www.sciencedirect.com/science/article/pii/S0264127519303491?via%3Dihub | https://www.sciencedirect.com/science/article/pii/S0264127519303491?via%3Dihub]] || || || || 2019 Aug 9 || Lilli || [[https://arxiv.org/abs/1906.10260 | arXiv 1906.10260]] || || || || 2019 Aug 2 || Koji || [[https://arxiv.org/abs/1812.03842 | arXiv 1812.03842]] || [[https://doi.org/10.1364/OPTICA.6.000240| Crystalline optical cavity at 4 K with thermal-noise-limited instability and ultralow drift ]] || || || 2019 July 26 || gautam || [[https://caltech.tind.io/record/745711?ln=en | R. Pintelon, J. Schoukens]], Ch 6: "An Intuitive Introduction to Frequency Domain Identification" || || ~8 || || 2019 July 12 || Gabriele || [[https://arxiv.org/abs/1903.07603|Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM]] [[https://link.aps.org/doi/10.1103/PhysRevLett.122.061105|Prospects for Resolving the Hubble Constant Tension with Standard Sirens]] [[https://link.aps.org/doi/10.1103/PhysRevLett.122.221301|https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.122.221301]]|| || || || 2019 June 28 || Nobody || [[https://arxiv.org/abs/1903.02017|Axion Dark Matter Search with Interferometric Gravitational Wave Detectors]] || || || || 2019 June 14 || Rana || [[https://arxiv.org/abs/1901.09045|Internal structure of white dwarfs from gravitational waves]] [[https://arxiv.org/abs/1903.04612|Understanding the evolution of close white dwarf binaries]]|| - || || || 2019 Apr 26 || Jon || [[https://arxiv.org/pdf/1812.09942.pdf|arXiv 1812.09942]] || || || || 2019 Apr 12 || Aaron || [[https://arxiv.org/abs/1605.00539v2|arXiv 1605.00539v2]] || [[https://doi.org/10.1016/j.crhy.2016.07.012|Introduction to Quantum-limited Parametric Amplification of Quantum Signals with Josephson Circuits]] || 8 || || 2019 Apr 5 || Jess || [[https://arxiv.org/abs/1903.07603|arXiv 1903.07603]] || Evidence for Physics Beyond Standard Model Cosmology || 4 || || 2019 Mar 15 || RNaana || [[https://actu.epfl.ch/news/scientists-build-the-smallest-optical-frequency--5/ || Scientists build the smallest optical frequency comb to-date]] || [[https://doi.org/10.1126/science.1193968| Microresonator-Based Optical Frequency Combs ]] || 9 || || 2019 Mar 1 || Koji || [[https://arxiv.org/abs/1810.00728|ArXiv:1810.00728]] || [[https://doi.org/10.1103/PhysRevLett.122.081104|Picometer-Stable Hexagonal Optical Bench to Verify LISA Phase Extraction Linearity and Precision]] || 6 || || 2019 Feb 22 || Aaron || [[https://iopscience.iop.org/article/10.1088/1367-2630/13/1/013017/meta|Proposal for an Optomechanical Traveling Wave Phonon-Photon Translator]] || [[https://copilot.caltech.edu/documents/512-1901_04129.pdf|Phononic bandgap nano-acoustic cavity with ultralong phonon lifetime]] || 5 || || 2019 Feb 1 || rAnA || [[https://arxiv.org/abs/1605.01060|Pair Fireball Precursors of Neutron Star Mergers]] || [[https://doi.org/10.1093/mnras/stw1800|Pair fireball precursors of neutron star mergers]] || || || 2019 Jan 18 || Gabriele Vajente || [[https://doi.org/10.1364/AO.53.001459|In situ correction of mirror surface to reduce round-trip losses in Fabry–Perot cavities]] || [[https://doi.org/10.1103/PhysRevD.87.082003 |Reduction of higher order mode generation in large scale gravitational wave interferometers by central heating residual aberration correction]] || 6 || [[Journal_Club/Past_meetings|Past meetings (archival)]] == Journal club roster 2018 == You can find an ordered list of upcoming presenters [[https://docs.google.com/spreadsheets/d/1TxTmFStB9jT1xCvscr5xKY5ovuA4nme58XK4IrqI6_0/edit#gid=0 | HERE ]]. The JCTsar script will chose people in this order. If you find you can't do a week that you are assigned to then find someone willing to trade and update that spreadsheet. === Highlighted papers pool === If we are short of a presenter we will draw something from this list of papers. If you find any papers that would be interesting to discuss at future journal club meetings, then you should add them to the list on the following page: [[Journal_Club/Interesting_papers|Interesting papers]] Older papers on this list can be found in the [[Journal_Club/Interesting_papers_archive | Interesting papers (archive) ]] page. == Chooser script (Updated python) == [[https://github.com/fincle/RoboTsar]] The python script TsarMailer.py downloads the [[https://docs.google.com/spreadsheets/d/1TxTmFStB9jT1xCvscr5xKY5ovuA4nme58XK4IrqI6_0/edit?usp=sharing| google spreadsheet list ]]. This sheet contains an ordered list of names and a list of public holidays to veto. It counts the number of days since the start of the year, vetoing public holidays and chooses presenters sequentially from the list. The scripts loops back to the beginning once the end is reached. An arbitrary phase shift is also added to the week number so that the list position can be twiddled in the event the presenter list length changes and position needs to be fixed. If a swap of names is performed leaving the list length the same there is no need to adjust the phase factor. Three other scripts exist to remind the presenter to post a paper and to remind people on the day. == Reorganization and topics == We are looking to shake up the structure of journal club by focusing attention on singular themes for month periods. The idea is to develop a deeper understanding of each topic rather than dipping into topics at random. Please edit this section with any ideas and suggestions as we figure out exactly what we are going to cover. Some suggested themes Experimental: - Thermal noise topics - Quantum mechanics in GW detectors and optimal detector design - Seismic cloaking and novel 'feed forward' reduction of seismic noise - Alternaive GW detectors (i.e. not laser interferometry) Data and astrophysics: - GW sources and astrophysics of a particular class of stars (i.e. Kilonovae, pulsars etc) - Cosmology and GW detection topic (GW CMB, early universe remnants?) - Exotic blackhole high energy physics coming out of GW detection - Glitches and detector characterization (machine learning stuff too?) - Bayesian statistics and optimal parameter extraction Other: - Effective outreach and evidence based teaching - Diversity in physics |
The LIGO journal club usually meets at 3:00PM on Fridays on 2nd floor of W Bridge (room 265). We meet to discuss a recent journal article from PRL, ApJ or the like. Someone is designated as a lead, to initiate the discussion, but not to present slides or give a monologue. The lead should also post a link to the article the Tuesday before meeting in the Meetings and papers section below.
Preferably, selected articles won't be exceptionally long, and would relate (at least tangentially) to LIGO.
You will be emailed by the journal club Tsar two weeks out from your date and again a week out. The rotating roster can be found at HERE
Mailing List
To send emails to everyone: ligo-journal-club@caltech.edu
Click here to subscribe
Meetings and papers
Journal club roster 2018
You can find an ordered list of upcoming presenters HERE. The JCTsar script will chose people in this order.
If you find you can't do a week that you are assigned to then find someone willing to trade and update that spreadsheet.
Highlighted papers pool
If we are short of a presenter we will draw something from this list of papers. If you find any papers that would be interesting to discuss at future journal club meetings, then you should add them to the list on the following page:
Older papers on this list can be found in the Interesting papers (archive) page.
Chooser script (Updated python)
https://github.com/fincle/RoboTsar
The python script TsarMailer.py downloads the google spreadsheet list. This sheet contains an ordered list of names and a list of public holidays to veto. It counts the number of days since the start of the year, vetoing public holidays and chooses presenters sequentially from the list. The scripts loops back to the beginning once the end is reached. An arbitrary phase shift is also added to the week number so that the list position can be twiddled in the event the presenter list length changes and position needs to be fixed.
If a swap of names is performed leaving the list length the same there is no need to adjust the phase factor.
Three other scripts exist to remind the presenter to post a paper and to remind people on the day.
Reorganization and topics
We are looking to shake up the structure of journal club by focusing attention on singular themes for month periods. The idea is to develop a deeper understanding of each topic rather than dipping into topics at random.
Please edit this section with any ideas and suggestions as we figure out exactly what we are going to cover.
Some suggested themes Experimental: - Thermal noise topics - Quantum mechanics in GW detectors and optimal detector design - Seismic cloaking and novel 'feed forward' reduction of seismic noise - Alternaive GW detectors (i.e. not laser interferometry)
Data and astrophysics: - GW sources and astrophysics of a particular class of stars (i.e. Kilonovae, pulsars etc) - Cosmology and GW detection topic (GW CMB, early universe remnants?) - Exotic blackhole high energy physics coming out of GW detection - Glitches and detector characterization (machine learning stuff too?) - Bayesian statistics and optimal parameter extraction
Other: - Effective outreach and evidence based teaching - Diversity in physics