Opendata, web and dolomites

GWsFromEMRIs SIGNED

Gravitational waves from extreme mass-ratio inspirals

Total Cost €

0

EC-Contrib. €

0

Partnership

0

Views

0

Project "GWsFromEMRIs" data sheet

The following table provides information about the project.

Coordinator
UNIVERSITAT DE LES ILLES BALEARS 

Organization address
address: CARRETERA DE VALLDEMOSSA KM 7.5
city: PALMA DE MALLORCA
postcode: 7122
website: www.uib.es

contact info
title: n.a.
name: n.a.
surname: n.a.
function: n.a.
email: n.a.
telephone: n.a.
fax: n.a.

 Coordinator Country Spain [ES]
 Total cost 158˙121 €
 EC max contribution 158˙121 € (100%)
 Programme 1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility)
 Code Call H2020-MSCA-IF-2016
 Funding Scheme MSCA-IF-EF-ST
 Starting year 2018
 Duration (year-month-day) from 2018-02-01   to  2020-08-18

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    UNIVERSITAT DE LES ILLES BALEARS ES (PALMA DE MALLORCA) coordinator 158˙121.00

Map

 Project objective

In 2016, the Laser Interferometer Gravitational-Wave Observatory (LIGO) collaboration announced its first ground-breaking detections of gravitational waves sourced by binary black hole mergers. These observations herald the beginning of a new era in astronomy: gravitational waves are expected to shed light on many unsolved astrophysical and theoretical problems, such as finding neutron stars' equation of state, modelling the formation and evolution of compact objects and testing alternative theories of gravity. With LIGO's next observational run starting in late 2016 and the prospect of seeing the space-based interferometer eLISA fly in the near future, gravitational wave physics is set to be one of the most active and exciting fields in contemporary science. Black hole binaries are going to be key targets both for LIGO and eLISA: it is thus crucial to perfect the modelling of these systems, as this will enable us to extract the rich information encoded in the gravitational wave signals that will be detected in the years to come. This project proposes the development of a state-of-the-art code to study extreme mass-ratio inspirals into Kerr black holes, including the full gravitational self-force (i.e. both conservative and dissipative effects). The project will contribute to the construction of a template bank for eLISA. Furthermore, it will inform the calibration of effective-one-body (EOB) and phenomenological waveform models which form the basis of LIGO-Virgo data analysis.

Are you the coordinator (or a participant) of this project? Plaese send me more information about the "GWSFROMEMRIS" 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 "GWSFROMEMRIS" are provided by the European Opendata Portal: CORDIS opendata.

More projects from the same programme (H2020-EU.1.3.2.)

NPsVLCD (2019)

Natural Product-Inspired Therapies for Leishmaniasis and Chagas Disease

Read More  

NaWaTL (2020)

Narrative, Writing, and the Teotihuacan Language: Exploring Language History Through Phylogenetics, Epigraphy and Iconography

Read More  

NeuroSens (2019)

Neuromodulation of Sensory Processing

Read More