Close

1. Identity statement
Reference TypeJournal Article
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/3AT7RU8
Repositorysid.inpe.br/mtc-m19/2011/12.02.18.01
Last Update2011:12.02.18.27.47 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19/2011/12.02.18.01.55
Metadata Last Update2018:06.05.04.25.06 (UTC) administrator
Secondary KeyINPE--PRE/
ISSN0185-1101
Citation KeyAguiar:2011:WhNe
TitleGravitational wave detection: what is new
ProjectFAPESP (No. 2006/56041-3), CNPq (No. 303310/2009-0)
Year2011
MonthOct
Access Date2024, May 19
Secondary TypePRE PI
Number of Files1
Size6059 KiB
2. Context
AuthorAguiar, Odylio Denys de
Resume Identifier8JMKD3MGP5W/3C9JJ2A
GroupDAS-CEA-INPE-MCT-BR
AffiliationInstituto Nacional de Pesquisas Espaciais (INPE)
e-Mail Addresstereza@sid.inpe.br
JournalRevista Mexicana de Astronomía y Astrofísica
Volume2011
Pages299-304
History (UTC)2011-12-02 18:28:02 :: tereza@sid.inpe.br -> administrator :: 2011
2012-07-15 03:00:13 :: administrator -> tereza@sid.inpe.br :: 2011
2013-02-27 12:38:15 :: tereza@sid.inpe.br -> administrator :: 2011
2018-06-05 04:25:06 :: administrator -> tereza@sid.inpe.br :: 2011
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsGravitational waves
Instrumentation detectors
AbstractThe quest for gravitational wave detection has been one of the toughest technological challenges ever faced by experimental physicists and engineers. Despite the null results to date, after four decades of research, the community involved in this area is continuously growing. One of the main reasons for this is because the first gravitational wave detection and the regular observation of gravitational waves are among the most important scientific goals for the beginning of this millennium. They will test one of the foundations of physics, Einsteins theory of general relativity, and will open a new window for the observation of the universe, which certainly will cause a revolution in our knowledge of physics and astrophysics. In this talk I will give an updated report about the status of all relevant detectors (interferometers, bars, spheres, radio-telescopes, and CMB satellites), in operation, going to an upgrading, under construction, or still as projects. In particular, I will give details about the Brazilian Schenberg detector.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Gravitational wave detection:...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
agreement.html 02/12/2011 16:01 1.0 KiB 
4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP7W/3AT7RU8
zipped data URLhttp://urlib.net/zip/8JMKD3MGP7W/3AT7RU8
Languageen
Target FileAguiar-Congresso-RMxAC..40_oaguiar[1].pdf
User Groupadministrator
tereza@sid.inpe.br
Visibilityshown
Archiving Policyallowpublisher allowfinaldraft
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
Mirror Repositorysid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Next Higher Units8JMKD3MGPCW/3ETR8EH
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.57.26 2
Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi electronicmailaddress format isbn label lineage mark nextedition notes number orcid parameterlist parentrepositories previousedition previouslowerunit progress readergroup rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url
7. Description control
e-Mail (login)tereza@sid.inpe.br
update 


Close