Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/34964
DC Field | Value | Language |
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dc.contributor.author | Kramer, M. | en_US |
dc.contributor.author | Lorimer, D. R. | en_US |
dc.contributor.author | Lyne, A. G. | en_US |
dc.contributor.author | McLaughlin, M. | en_US |
dc.contributor.author | BURGAY, MARTA | en_US |
dc.contributor.author | D'Amico, Nicolò | en_US |
dc.contributor.author | POSSENTI, ANDREA | en_US |
dc.contributor.author | Camilo, F. | en_US |
dc.contributor.author | Freire, P. C. C. | en_US |
dc.contributor.author | Joshi, B. C. | en_US |
dc.contributor.author | Manchester, R. N. | en_US |
dc.contributor.author | Reynolds, J. | en_US |
dc.contributor.author | Sarkissian Australia Telescope National Facility, J. | en_US |
dc.contributor.author | Csiro | en_US |
dc.contributor.author | Stairs, Australia I. H. | en_US |
dc.contributor.author | Ferdman, R. D. | en_US |
dc.date.accessioned | 2024-03-14T14:23:50Z | - |
dc.date.available | 2024-03-14T14:23:50Z | - |
dc.date.issued | 2005 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/34964 | - |
dc.description.abstract | This first ever double pulsar system consists of two pulsars orbiting the common center of mass in a slightly eccentric orbit of only 2.4-hr duration. The pair of pulsars with pulse periods of 22 ms and 2.8 sec, respectively, confirms the long-proposed recycling theory for millisecond pulsars and provides an exciting opportunity to study the works of pulsar magnetospheres by a very fortunate geometrical alignment of the orbit relative to our line-of-sight. In particular, this binary system represents a truly unique laboratory for relativistic gravitational physics. This contribution serves as an update on the currently obtained results and their consequences for the test of general relativity in the strong-field regime. A complete and more up-to-date report of the timing results will be presented elsewhere shortly. | en_US |
dc.language.iso | eng | en_US |
dc.title | Testing GR with the Double Pulsar: Recent Results | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.48550/arXiv.astro-ph/0503386 | en_US |
dc.identifier.url | https://arxiv.org/abs/astro-ph/0503386 | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.firstpage | 142 | en_US |
dc.type.referee | REF_0 | en_US |
dc.description.international | sì | en_US |
dc.relation.alleditors | Chen, Pisin; Bloom, Elliott; Madejski, Greg; Patrosian,Vahe | en_US |
dc.relation.ispartofbook | The 22nd Texas Symposium on Relativistic Astrophysics | en_US |
dc.relation.conferencename | The 22nd Texas Symposium on Relativistic Astrophysics | en_US |
dc.relation.conferenceplace | Stanford, California | en_US |
dc.relation.conferencedate | December 13-17, 2004 | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.identifier.adsbibcode | 2005tsra.conf..142K | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.openairetype | Conference paper | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.orcid | 0000-0002-8265-4344 | - |
crisitem.author.orcid | 0000-0001-5902-3731 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | |
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Kramer2005-arXiv.pdf | postprint | 502.4 kB | Adobe PDF | View/Open |
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