Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/24386
DC Field | Value | Language |
---|---|---|
dc.contributor.author | POSSENTI, ANDREA | en_US |
dc.contributor.author | BURGAY, MARTA | en_US |
dc.date.accessioned | 2020-04-30T15:26:45Z | - |
dc.date.available | 2020-04-30T15:26:45Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.isbn | 978-3-319-20223-5 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/24386 | - |
dc.description.abstract | Radio pulsars are neutron stars (NSs) which emit collimated beams of radio waves, observed as pulses, once per rotation of the NS. A subgroup of the radio pulsars behave as highly stable clocks and monitoring the times of arrival of their radio pulses can provide an accurate determination of their positional, rotational, and orbital parameters, as well as indications on the properties of their space-time environment. In this chapter, we focus on the so-called relativistic binary pulsars, recycled NSs orbiting around a compact companion star. Some of them can be used as unique tools to test general relativity and other gravitational theories. The methodology for exploiting these sources as laboratories for gravity theories is first explained and then some of the most relevant recent results are reviewed. <P /> | en_US |
dc.language.iso | eng | en_US |
dc.title | The Role of Binary Pulsars in Testing Gravity Theories | en_US |
dc.type | Book part | - |
dc.identifier.doi | 10.1007/978-3-319-20224-2_8 | en_US |
dc.identifier.scopus | 2-s2.0-85016815741 | en_US |
dc.identifier.url | https://link.springer.com/chapter/10.1007%2F978-3-319-20224-2_8 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.firstpage | 279 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 2 | en_US |
dc.description.international | no | en_US |
dc.contributor.country | ITA | en_US |
dc.relation.allauthors | Peron, Roberto; Colpi, Monica; Gorini, Vittorio; Moschella, Ugo | en_US |
dc.relation.ispartofbook | Gravity: Where Do We Stand? | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.type.miur | 268 Contributo in volume (Capitolo o Saggio) | - |
dc.identifier.adsbibcode | 2016gwdw.book..279P | en_US |
dc.relation.ercsector | Scienze Fisiche Settori ERC (ERC) di riferimento::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation::PE9_11 Relativistic astrophysics | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegherò il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Book part | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.orcid | 0000-0001-5902-3731 | - |
crisitem.author.orcid | 0000-0002-8265-4344 | - |
Appears in Collections: | 2.01 Capitoli o saggi in libro |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
Possenti-Burgay_chapter-aam.pdf | postprint | 792.75 kB | Adobe PDF | View/Open |
Possenti-Burgay2016_Chapter_TheRoleOfBinaryPulsarsInTestin.pdf | [administrators only] | 1.23 MB | Adobe PDF |
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Items in DSpace are published in Open Access, unless otherwise indicated.