CaltechAUTHORS
  A Caltech Library Service

The future is now

Kasliwal, Mansi M. (2020) The future is now. Nature Reviews Physics, 2 (9). pp. 452-454. ISSN 2522-5820. https://resolver.caltech.edu/CaltechAUTHORS:20200814-150343488

Full text is not posted in this repository. Consult Related URLs below.

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20200814-150343488

Abstract

We are living the twenty-first century gold rush: astronomers and physicists have been working together to identify the sites of heavy element production in the Universe (gold included). The theory was clear decades ago: the rapid capture of free neutrons (r-process nucleosynthesis) synthesizes heavy elements (atomic mass range between 70 and 200 amu) and neutron star mergers are a promising site for this process to take place. However, the direct detection of gravitational waves (GWs) was needed to catch neutron stars in the act of merging, and telescopes were needed to pinpoint the location and characterize the electromagnetic (EM) emission. This is not an easy feat. As an example, I describe some lessons learned with a team comprised of 16 institutions around the world: the Global Relay of Observatories Watching Transients Happen (GROWTH) collaboration (Fig. 1).


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1038/s42254-020-0227-zDOIArticle
https://rdcu.be/b6goBPublisherFree ReadCube access
http://growth.caltech.edu/Related ItemGROWTH Collaboration
ORCID:
AuthorORCID
Kasliwal, Mansi M.0000-0002-5619-4938
Additional Information:© 2020 Springer Nature Limited. Published 13 August 2020; Issue Date September 2020. GROWTH is a National Science Foundation Partnership in International Research and Education programme that comprises 16 institutions around the world: California Institute of Technology (USA), University of Maryland College Park (USA), University of Wisconsin Milwaukee (USA), Texas Tech University (USA), San Diego State University (USA), University of Washington Seattle (USA), Los Alamos National Laboratory (USA), Tokyo Institute of Technology (Japan), National Central University (Taiwan), Indian Institute of Astrophysics (India), Indian Institute of Technology Bombay (India), Weizmann Institute of Science (Israel), The Oskar Klein Centre at Stockholm University (Sweden), Humboldt University (Germany), Liverpool John Moores University (UK) and University of Sydney (Australia). The authors declare no competing interests.
Issue or Number:9
Record Number:CaltechAUTHORS:20200814-150343488
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20200814-150343488
Official Citation:Kasliwal, M.M. The future is now. Nat Rev Phys 2, 452–454 (2020). https://doi.org/10.1038/s42254-020-0227-z
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:104967
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:17 Aug 2020 14:04
Last Modified:08 Sep 2020 17:30

Repository Staff Only: item control page