1. Identity statement | |
Reference Type | Journal Article |
Site | mtc-m21c.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 8JMKD3MGP3W34R/3R3EK22 |
Repository | sid.inpe.br/mtc-m21c/2018/05.04.19.03 (restricted access) |
Last Update | 2018:05.04.19.03.15 (UTC) simone |
Metadata Repository | sid.inpe.br/mtc-m21c/2018/05.04.19.03.15 |
Metadata Last Update | 2020:12.07.21.11.36 (UTC) administrator |
DOI | 10.1088/1742-6596/957/1/012013 |
ISSN | 1742-6588 |
Citation Key | BortoliFrajAgui:2018:ScMiCa |
Title | Schenberg microwave cabling seismic isolation |
Year | 2018 |
Month | mar. |
Access Date | 2024, May 19 |
Type of Work | conference paper |
Secondary Type | PRE PI |
Number of Files | 1 |
Size | 669 KiB |
|
2. Context | |
Author | 1 Bortoli, F. S. 2 Frajuca, C. 3 Aguiar, Odylio Denys de |
Resume Identifier | 1 2 3 8JMKD3MGP5W/3C9JJ2A |
Group | 1 2 3 DIDAS-CGCEA-INPE-MCTIC-GOV-BR |
Affiliation | 1 Instituto Federal de São Paulo (IFSP) 2 Instituto Federal de São Paulo (IFSP) 3 Instituto Nacional de Pesquisas Espaciais (INPE) |
Author e-Mail Address | 1 2 frajuca@gmail.com 3 odylio.aguiar@inpe.br |
Journal | Journal of Physics: Conference Series |
Volume | 957 |
Number | 1 |
Pages | e012013 |
Secondary Mark | B2_INTERDISCIPLINAR B2_ENGENHARIAS_III B3_MEDICINA_II B3_GEOCIÊNCIAS B4_MATERIAIS B4_ENGENHARIAS_II B4_BIOTECNOLOGIA C_QUÍMICA C_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA C_ENGENHARIAS_IV C_ECONOMIA C_ASTRONOMIA_/_FÍSICA |
History (UTC) | 2018-05-04 19:03:15 :: simone -> administrator :: 2018-05-04 19:03:15 :: administrator -> simone :: 2018 2018-05-04 19:03:36 :: simone -> administrator :: 2018 2020-12-07 21:11:36 :: administrator -> simone :: 2018 |
|
3. Content and structure | |
Is the master or a copy? | is the master |
Content Stage | completed |
Transferable | 1 |
Content Type | External Contribution |
Version Type | publisher |
Abstract | SCHENBERG is a resonant-mass gravitational wave detector with a frequency about 3.2 kHz. Its spherical antenna, weighing 1.15 metric ton, is connected to the external world by a system which must attenuate seismic noise. When a gravitational wave passes the antenna vibrates, its motion is monitored by transducers. These parametric transducers uses microwaves carried by coaxial cables that are also connected to the external world, they also carry seismic noise. In this analysis the system was modeled using finite element method. This work shows that the addition of masses along these cables can decrease this noise, so that this noise is below the thermal noise of the detector when operating at 50 mK. |
Area | CEA |
Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Schenberg microwave cabling... |
doc Directory Content | access |
source Directory Content | there are no files |
agreement Directory Content | |
|
4. Conditions of access and use | |
Language | en |
Target File | bortoli_schenberg.pdf |
User Group | simone |
Reader Group | administrator simone |
Visibility | shown |
Archiving Policy | denypublisher denyfinaldraft12 |
Read Permission | deny from all and allow from 150.163 |
Update Permission | not transferred |
|
5. Allied materials | |
Next Higher Units | 8JMKD3MGPCW/3ETR8EH |
Citing Item List | sid.inpe.br/mtc-m21/2012/07.13.14.57.26 2 sid.inpe.br/bibdigital/2013/10.01.00.07 1 |
Dissemination | WEBSCI; PORTALCAPES; SCOPUS. |
Host Collection | urlib.net/www/2017/11.22.19.04 |
|
6. Notes | |
Notes | 12th Edoardo Amaldi Conference on Gravitational Waves (AMALDI 12) |
Empty Fields | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn keywords label lineage mark mirrorrepository nextedition orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url |
|
7. Description control | |
e-Mail (login) | simone |
update | |
|