Explore the words cloud of the FunGraW project. It provides you a very rough idea of what is the project "FunGraW" about.
The following table provides information about the project.
Coordinator |
UNIVERSITA DEGLI STUDI DI ROMA LA SAPIENZA
Organization address contact info |
Coordinator Country | Italy [IT] |
Total cost | 168˙277 € |
EC max contribution | 168˙277 € (100%) |
Programme |
1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility) |
Code Call | H2020-MSCA-IF-2017 |
Funding Scheme | MSCA-IF-EF-ST |
Starting year | 2019 |
Duration (year-month-day) | from 2019-01-01 to 2020-12-31 |
Take a look of project's partnership.
# | ||||
---|---|---|---|---|
1 | UNIVERSITA DEGLI STUDI DI ROMA LA SAPIENZA | IT (ROMA) | coordinator | 168˙277.00 |
The first gravitational wave (GW) detections by the Laser Interferometric Gravitational-wave Observatory (LIGO) are an historical landmark. These detections opened a completely new window to the Universe and officially marked the beginning of GW astronomy.
GWs travel almost unimpeded through the Universe, thus conveying clean information about their sources. This gives us a unique opportunity to test the nonlinear regime of Einstein’s theory of general relativity (GR) to unprecedented levels. Indeed, the GWs detected so far were emitted by the merger of binary black holes (BHs) which are the prototypical sources to investigate gravity in its most extreme regimes.
However, the true potential of GW observatories to discover new physics beyond of current knowledge is far from being fully explored. In fact, besides probing the nature of compact objects and testing GR, GW detectors may also revolutionize our understanding of particle physics, dark matter (DM) and even possibly quantum gravity. At small scales, with the advent of precision GW physics we will be probing regions closer to the BH horizon, potentially ruling out or confirming alternatives to BHs that predict corrections at the horizon scale. On the opposite side of the spectrum, GWs may also give us hints about the nature of large scale anomalies, such as the existence of DM. For example, light bosonic fields around compact objects, i.e. BHs and neutron stars (NSs), can trigger superradiant instabilities and emit long-lived monochromatic GWs that can be used to either probe the existence of new particles beyond the Standard Model or, in the absence of detections, impose strong constraints on their masses and couplings.
The prime goal of this proposal is to understand what GWs can tell us about fundamental questions such as the nature of compact objects and DM and ultimately to contribute to the recent theoretical efforts in developing the full scientific potential of the newborn field of GW astronomy.
year | authors and title | journal | last update |
---|---|---|---|
2019 |
Emanuele Berti, Richard Brito, Caio F. B. Macedo, Guilherme Raposo, João LuÃs Rosa Ultralight boson cloud depletion in binary systems published pages: , ISSN: 2470-0010, DOI: 10.1103/physrevd.99.104039 |
Physical Review D 99/10 | 2019-06-06 |
2019 |
Otto A. Hannuksela, Kaze W. K. Wong, Richard Brito, Emanuele Berti, Tjonnie G. F. Li Probing the existence of ultralight bosons with a single gravitational-wave measurement published pages: 447-451, ISSN: 2397-3366, DOI: 10.1038/s41550-019-0712-4 |
Nature Astronomy 3/5 | 2019-06-06 |
2019 |
Shrobana Ghosh, Emanuele Berti, Richard Brito, Mauricio Richartz Follow-up signals from superradiant instabilities of black hole merger remnants published pages: , ISSN: 2470-0010, DOI: 10.1103/physrevd.99.104030 |
Physical Review D 99/10 | 2019-06-06 |
2019 |
Taishi Ikeda, Richard Brito, Vitor Cardoso Blasts of Light from Axions published pages: , ISSN: 0031-9007, DOI: 10.1103/physrevlett.122.081101 |
Physical Review Letters 122/8 | 2019-04-18 |
2019 |
Otto A. Hannuksela, Kaze W. K. Wong, Richard Brito, Emanuele Berti, Tjonnie G. F. Li Probing the existence of ultralight bosons with a single gravitational-wave measurement published pages: , ISSN: 2397-3366, DOI: 10.1038/s41550-019-0712-4 |
Nature Astronomy | 2019-04-18 |
Are you the coordinator (or a participant) of this project? Plaese send me more information about the "FUNGRAW" project.
For instance: the website url (it has not provided by EU-opendata yet), the logo, a more detailed description of the project (in plain text as a rtf file or a word file), some pictures (as picture files, not embedded into any word file), twitter account, linkedin page, etc.
Send me an email (fabio@fabiodisconzi.com) and I put them in your project's page as son as possible.
Thanks. And then put a link of this page into your project's website.
The information about "FUNGRAW" are provided by the European Opendata Portal: CORDIS opendata.
Open data: improving transparency, reproducibility and collaboration in science
Read MoreNeural mechanisms of crossmodal activity in blind and sighted individuals
Read MoreMonitoring cancer stem cell dynamics and therapeutic response in BRCA2-deficient breast tumour cells
Read More