Scalable CI for Early Warning Gravitational Wave Detections
Start: 2018-10-01
End: 2021-09-30
National Science Foundation
OAC-1841480
...
Affiliations
| Physics |
Collaborations
| LIGO |

The recent multi-messenger detection of of the binary neutron star merger known as GW170817 changed astronomy overnight. The source was detected first in gravitational waves, two seconds later in gamma rays and after 10 hours in optical, ultraviolet, infrared, and much later x-ray and radio. From this single event the world learned that the progenitors of at least some short-hard gamma ray bursts are neutron star mergers, the origin of many elements in the periodic table such as gold and platinum might also be neutron star mergers, gravity and light travel at the same speed, and gravitational waves really could measure the expansion rate of the universe! Despite what was learned, GW170817 left the world with many questions. What object was formed afterward? Another neutron star? A black hole? Why was the gamma ray burst associated with GW170817 unlike anything else that had been observed? Data is required to address these questions - specifically electromagnetic data taken right when the neutron stars merged. It is possible to use gravitational wave data, which measures the neutron star before it merges, to automatically direct robotic observations of telescopes across the world and in space. Doing so requires tremendous cyber-infrastructure which is presently lacking.

Using gravitational waves to provide an early warning for robotic telescopes will significantly enhance the scientific utility of LIGO data by enabling multi-messenger astrophysics associated with measuring electromagnetic radiation across the spectrum right as the two neutron stars merge helping to answer what drives some of the brightest objects in the known universe. This project will fortify the streaming data delivery of LIGO by producing sub-second data delivery to a streaming early warning search for neutron star mergers. Substantial monitoring and feedback will be put in place to ensure that the entire system operates without human intervention from the instrument all the way to a public alert within seconds of data taking. The project will capitalize upon existing NSF investments in cyber-infrastructure for real-time gravitational wave analysis, but will augment significantly the layer which handles data delivery and automation, which is presently a bottleneck and failure mode.

Publications

  1. Benjamin Abbott, Richard Abbott, TD Abbott, S Abraham, F Acernese, K Ackley, C Adams, Rana Adhikari, Vaishali Adya, C Affeldt, others, "Low-latency gravitational-wave alerts for multimessenger astronomy during the second Advanced LIGO and virgo observing run." The Astrophysical Journal 875 2 (2019)
  2. R Abbott, TD Abbott, S Abraham, F Acernese, K Ackley, C Adams, RX Adhikari, VB Adya, C Affeldt, M Agathos, others, "GW190412: Observation of a binary-black-hole coalescence with asymmetric masses." Physical Review D 102 4 (2020)
  3. BP Abbott, R Abbott, TD Abbott, S Abraham, F Acernese, K Ackley, C Adams, RX Adhikari, VB Adya, C Affeldt, others, "GW190425: Observation of a compact binary coalescence with total mass~ 3.4 M⊙." The Astrophysical Journal Letters 892 1 (2020)
  4. Richard Abbott, TD Abbott, S Abraham, F Acernese, K Ackley, C Adams, RX Adhikari, VB Adya, C Affeldt, M Agathos, others, "GW190814: Gravitational waves from the coalescence of a 23 solar mass black hole with a 2.6 solar mass compact object." The Astrophysical Journal Letters 896 2 (2020)
  5. R Abbott, TD Abbott, S Abraham, F Acernese, K Ackley, A Adams, C Adams, RX Adhikari, VB Adya, C Affeldt, others, "Observation of gravitational waves from two neutron star--black hole coalescences." The Astrophysical Journal Letters 915 1 (2021)
  6. Kipp Cannon, Sarah Caudill, Chiwai Chan, Bryce Cousins, Jolien Creighton, Becca Ewing, Heather Fong, Patrick Godwin, Chad Hanna, Shaun Hooper, others, "GstLAL: A software framework for gravitational wave discovery." SoftwareX 14 (2021)
  7. Chad Hanna, Sarah Caudill, Cody Messick, Amit Reza, Surabhi Sachdev, Leo Tsukada, Kipp Cannon, Kent Blackburn, Jolien Creighton, Heather Fong, others, "Fast evaluation of multidetector consistency for real-time gravitational wave searches." Physical Review D 101 2 (2020)
  8. Ryan Magee, Heather Fong, Sarah Caudill, Cody Messick, Kipp Cannon, Patrick Godwin, Chad Hanna, Shasvath Kapadia, Duncan Meacher, Siddharth Mohite, others, "Sub-threshold Binary Neutron Star Search in Advanced LIGO’s First Observing Run." The Astrophysical Journal Letters 878 1 (2019)
  9. Ryan Magee, Deep Chatterjee, Leo Singer, Surabhi Sachdev, Manoj Kovalam, Geoffrey Mo, Stuart Anderson, Patrick Brady, Patrick Brockill, Kipp Cannon, others, "First demonstration of early warning gravitational-wave alerts." The Astrophysical Journal Letters 910 2 (2021)
  10. Surabhi Sachdev, Sarah Caudill, Heather Fong, Rico Lo, Cody Messick, Debnandini Mukherjee, Ryan Magee, Leo Tsukada, Kent Blackburn, Patrick Brady, others, "The GstLAL Search Analysis Methods for Compact Binary Mergers in Advanced LIGO's Second and Advanced Virgo's First Observing Runs." arXiv preprint arXiv:1901.08580 (2019)
  11. Surabhi Sachdev, Ryan Magee, Chad Hanna, Kipp Cannon, Leo Singer, Javed Sk, Debnandini Mukherjee, Sarah Caudill, Chiwai Chan, Jolien Creighton, others, "An early-warning system for electromagnetic follow-up of gravitational-wave events." The Astrophysical Journal Letters 905 2 (2020)
  12. M Saleem, Javed Rana, V Gayathri, Aditya Vijaykumar, Srashti Goyal, Surabhi Sachdev, Jishnu Suresh, S Sudhagar, Arunava Mukherjee, Gurudatt Gaur, others, "The science case for LIGO-India." Classical and Quantum Gravity 39 2 (2021)
  13. Leo Tsukada, Kipp Cannon, Chad Hanna, Drew Keppel, Duncan Meacher, Cody Messick, "Application of a zero-latency whitening filter to compact binary coalescence gravitational-wave searches." Physical Review D 97 10 (2018)


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About our wordmark
Monica The IGC wordmark was created by Monica Rincon Ramirez, while she was a graduate student at the Institute for Gravitation and the Cosmos (IGC). Monica enjoys drawing new connections between fundamental theory and observations. Her graduate work includes specialized topics in general relativity, loop quantum gravity, and quantum fields in cosmological backgrounds. In particular, her thesis work focused on finding effective quantum corrections to gravitational phenomena from spinfoams, and applications to cosmology. She received her PhD in 2024.

The wordmark symbolizes the scope and variety of research at the IGC. The base of the image represents quantum gravity, evoking the quantum geometrical picture from spinfoams and loop quantum gravity. These are among the approaches to fundamental questions studied at the Center for Fundamental Theory. The middle of the image represents the Center for Theoretical and Observational Cosmology by galaxies embedded in a smooth surface, characteristic of spacetime in general relativity and the much larger physical scales studied in cosmology. Finally, at the top, the surface curves to an extreme, representing a supermassive black hole accompanied by an energetic jet. These elements depict an active galactic nucleus, inspired by Centaurus A. Just to the right, a pair of black holes approaches merger. This top portion of the wordmark represents the Center for Multimessenger Astrophysics, which specializes in the study of high-energy phenomena in the universe.