| 1. Identity statement | |
| Reference Type | Journal Article |
| Site | mtc-m16c.sid.inpe.br |
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identifier | 6qtX3pFwXQZ3P8SECKy/CBhJm |
| Repository | sid.inpe.br/jeferson/2004/06.29.11.23 (restricted access) |
| Last Update | 2006:06.14.04.04.06 (UTC) administrator |
| Metadata Repository | sid.inpe.br/jeferson/2004/06.29.11.23.50 |
| Metadata Last Update | 2018:06.04.04.12.52 (UTC) administrator |
| Secondary Key | INPE-10787-PRE/6244 |
| ISBN/ISSN | 0264-9381 |
| ISSN | 0264-9381 |
| Citation Key | AraujoMirCasPalAgu:2004:CaBlMA |
| Title | Can black-hole MACHO binaries be detected by the Brazilian spherical antenna?  |
| Year | 2004 |
| Secondary Date | 20040205 |
| Month | Feb. |
| Access Date | 2024, Apr. 27 |
| Secondary Type | PRE PI |
| Number of Files | 1 |
| Size | 87 KiB |
| 2. Context | |
| Author | 1 Araujo, Jose Carlos Neves de 2 Miranda, Oswaldo Duarte 3 Castro, Claudio de Souza 4 Paleo, Bruno Woltzenlogel 5 Aguiar, Odylio Denys de |
| Resume Identifier | 1 8JMKD3MGP5W/3C9JHGK 2 8JMKD3MGP5W/3C9JJ2G 3 4 5 8JMKD3MGP5W/3C9JJ2A |
| Group | 1 DAS-INPE-MCT-BR |
| Affiliation | 1 Instituto Nacional de Pesquisas Espaciais - Divisão de Astrofísica 2 Instituto Tecnológico de Aeronáutica - Departamento de Física |
| e-Mail Address | jcarlos@das.inpe.br |
| Journal | Classical and Quantum Gravity |
| Volume | 21 |
| Number | 5 Sp. Iss. |
| Pages | S521-S527 |
| History (UTC) | 2007-03-05 21:29:46 :: administrator -> marciana :: 2008-05-02 16:20:25 :: marciana -> administrator :: 2018-06-04 04:12:52 :: administrator -> marciana :: 2004 |
| 3. Content and structure | |
| Is the master or a copy? | is the master |
| Content Stage | completed |
| Transferable | 1 |
| Content Type | External Contribution |
| Keywords | cosmology halo |
| Abstract | Different studies show that dark matter of non-baryonic origin might exist. There is experimental evidence that at least one form of dark matter has been detected through microlensing effects. This form of dark matter is named MACHOs (massive astrophysical compact halo objects). The MACHO collaboration estimated that the masses of these objects are to be in the range 0.15–0.95M_, where the most probable mass is of 0.5M_. Some authors argue that MACHOs could be black holes, and that they could form binary systems, BHMACHO binaries. As is well known, binary systems are sources of gravitational waves. The Brazilian spherical antenna will operate in the frequency band of 3.0–3.4 kHz, sensitive to binaries of a pair of 0.5M_ black holes just before coalescing. In the present work we study the detectability of these putative BHMACHO binaries by the Brazilian spherical antenna Mario Schenberg. |
| Area | CEA |
| Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Can black-hole MACHO... |
| doc Directory Content | access |
| source Directory Content | there are no files |
| agreement Directory Content | there are no files |
| 4. Conditions of access and use | |
| Language | en |
| Target File | Can Black-Hole MACHOS Binaries be detected.pdf |
| User Group | administrator marciana valdirene |
| Visibility | shown |
| Copy Holder | SID/SCD |
| Archiving Policy | denypublisher denyfinaldraft12 |
| Read Permission | deny from all and allow from 150.163 |
| 5. Allied materials | |
| Next Higher Units | 8JMKD3MGPCW/3ETR8EH |
| Dissemination | WEBSCI; PORTALCAPES; COMPENDEX. |
| Host Collection | sid.inpe.br/mtc-m18@80/2008/03.17.15.17 |
| 6. Notes | |
| Empty Fields | alternatejournal archivist callnumber copyright creatorhistory descriptionlevel documentstage doi electronicmailaddress format isbn label lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype |
| 7. Description control | |
| e-Mail (login) | marciana |
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