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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/3D76J38
Repositorysid.inpe.br/mtc-m19/2012/12.11.15.55
Last Update2013:07.30.18.22.05 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19/2012/12.11.15.55.58
Metadata Last Update2021:02.12.13.48.16 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1063/1.4756990
ISSN0094-243X
Citation KeyMoraesMira:2012:CoKaGr
TitleCosmology from Kaluza-Klein gravitational model
Year2012
Access Date2024, Apr. 19
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size857 KiB
2. Context
Author1 Moraes, P. H. R. S.
2 Miranda, Oswaldo Duarte
Resume Identifier1
2 8JMKD3MGP5W/3C9JJ2G
Group1
2 DAS-CEA-INPE-MCTI-GOV-BR
Affiliation1
2 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1
2 oswaldo@das.inpe.br
e-Mail Addressmarcelo.pazos@inpe.br
JournalAIP Conference Proceedings
Volume1483
Pages435-440
Secondary MarkC_ASTRONOMIA_/_FÍSICA C_ENGENHARIAS_II C_ENGENHARIAS_III C_GEOCIÊNCIAS B2_INTERDISCIPLINAR B2_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA B5_MEDICINA_II B3_ODONTOLOGIA C_QUÍMICA
History (UTC)2013-03-25 13:09:16 :: marcelo.pazos@sid.inpe.br -> administrator :: 2012
2021-02-12 13:48:16 :: administrator -> marcelo.pazos@inpe.br :: 2012
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordscosmology
general relativity
gravitation
Kaluza-Klein theory
dark energy
extra dimensions
AbstractIn this work we present a cosmological model derived from Kaluza-Klein theory, identifying the functional form of the parameter associated to the fifth dimension in such a way that it produces a solution that mimetizes the effects of the cosmological constant in the scope of General Relativity.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Cosmology from Kaluza-Klein...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
agreement.html 11/12/2012 13:55 1.0 KiB 
4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP7W/3D76J38
zipped data URLhttp://urlib.net/zip/8JMKD3MGP7W/3D76J38
Languageen
Target FileAPC000435.pdf
User Groupadministrator
marcelo.pazos@inpe.br
Reader Groupadministrator
marcelo.pazos@inpe.br
Visibilityshown
Archiving Policyallowpublisher allowfinaldraft
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
LinkingTrabalho Vinculado à Tese/Dissertação
Mirror Repositorysid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Next Higher Units8JMKD3MGPCW/3ETR8EH
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.57.32 1
URL (untrusted data)http://dx.doi.org/10.1063/1.4756990
DisseminationWEBSCI; PORTALCAPES.
Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notes
NotesTHE SIXTH INTERNATIONAL SCHOOL ON FIELD THEORY AND GRAVITATION-2012
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn label lineage mark month nextedition number orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate session shorttitle sponsor subject tertiarytype
7. Description control
e-Mail (login)marcelo.pazos@inpe.br
update 

1. Identity statement
Reference TypeJournal Article
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/3EJ43JS
Repositorysid.inpe.br/mtc-m19/2013/08.01.19.43   (restricted access)
Last Update2015:03.20.12.06.30 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19/2013/08.01.19.43.38
Metadata Last Update2018:06.05.04.14.43 (UTC) administrator
DOI10.1088/0264-9381/29/15/155002
ISSN0264-9381
Citation KeyAasiAAAAAAAAAAAAAAAAACAAAAAAAAAAAABBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCDDDDDDDDDDDDRDDDDDDDDDDDEDDDDDDDDDDDDDEEEEEEEEEEEFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHIIIIIJJJJJJJJJJKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMNNNNNNNNNNNNNOOOOOOOOOOOOOOOPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPQQRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSTTTTTTBTTTTTTTTTTTTTTTTTTUVVBVPVVVVVVVVVVVVVVVVVVVWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWYYYYYYYYYZZZZZZZZZ:2012:ChViDa
TitleThe characterization of Virgo data and its impact on gravitational-wave searches
Year2012
MonthAUG 7
Access Date2024, Apr. 19
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size3790 KiB
2. Context
Author  1 Aasi, J.
  2 Abadie, J.
  3 Abbott, B. P.
  4 Abbott, R.
  5 Abbott, T. D.
  6 Abernathy, M.
  7 Accadia, T.
  8 Acernese, F.
  9 Adams, C.
 10 Adams, T.
 11 Addesso, P.
 12 Adhikari, R.
 13 Affeldt, C.
 14 Agathos, M.
 15 Agatsuma, K.
 16 Ajith, P.
 17 Allen, B.
 18 Allocca, A.
 19 Ceron, E. Amador
 20 Amariutei, D.
 21 Anderson, S. B.
 22 Anderson, W. G.
 23 Arai, K.
 24 Araya, M. C.
 25 Ast, S.
 26 Aston, S. M.
 27 Astone, P.
 28 Atkinson, D.
 29 Aufmuth, P.
 30 Aulbert, C.
 31 Aylott, B. E.
 32 Babak, S.
 33 Baker, P.
 34 Ballardin, G.
 35 Ballinger, T.
 36 Ballmer, S.
 37 Bao, Y.
 38 Barayoga, J. C. B.
 39 Barker, D.
 40 Barone, F.
 41 Barr, B.
 42 Barsotti, L.
 43 Barsuglia, M.
 44 Barton, M. A.
 45 Bartos, I.
 46 Bassiri, R.
 47 Bastarrika, M.
 48 Bastiab, A.
 49 Batch, J.
 50 Bauchrowitz, J.
 51 Bauera, Th S.
 52 Bebronne, M.
 53 Beck, D.
 54 Behnke, B.
 55 Bejgerc, M.
 56 Beker, M. G.
 57 Bell, A. S.
 58 Bell, C.
 59 Belopolski, I.
 60 Benacquista, M.
 61 Berliner, J. M.
 62 Bertolini, A.
 63 Betzwieser, J.
 64 Beveridge, N.
 65 Beyersdorf, P. T.
 66 Bhadbade, T.
 67 Bilenko, I. A.
 68 Billingsley, G.
 69 Birch, J.
 70 Biswas, R.
 71 Bitossi, M.
 72 Bizouard, M. A.
 73 Black, E.
 74 Blackburn, J. K.
 75 Blackburn, L.
 76 Blair, D.
 77 Bland, B.
 78 Blom, M.
 79 Bock, O.
 80 Bodiya, T. P.
 81 Bogan, C.
 82 Bond, C.
 83 Bondarescu, R.
 84 Bondu, F.
 85 Bonelli, L.
 86 Bonnand, R.
 87 Bork, R.
 88 Born, M.
 89 Boschi, V.
 90 Bose, S.
 91 Bosia, L.
 92 Bouhou, B.
 93 Braccini, S.
 94 Bradaschia, C.
 95 Brady, P. R.
 96 Braginsky, V. B.
 97 Branchesi, M.
 98 Brau, J. E.
 99 Breyer, J.
100 Briant, T.
101 Bridges, D. O.
102 Brillet, A.
103 Brinkmann, M.
104 Brisson, V.
105 Britzger, M.
106 Brooks, A. F.
107 Brown, D. A.
108 Bulik, T.
109 Bulten, H. J.
110 Buonanno, A.
111 Burguet-Castell, J.
112 Buskulic, D.
113 Buy, C.
114 Byer, R. L.
115 Cadonati, L.
116 Cagnoli, G.
117 Calloni, E.
118 Camp, J. B.
119 Campsie, P.
120 Cannon, K.
121 Canuel, B.
122 Cao, J.
123 Capano, C. D.
124 Carbognani, F.
125 Carbone, L.
126 Caride, S.
127 Caudill, S.
128 Cavaglia, M.
129 Cavalier, F.
130 Cavalieri, R.
131 Cella, G.
132 Cepeda, C.
133 Cesarini, E.
134 Chalermsongsak, T.
135 Charlton, P.
136 Chassande-Mottin, E.
137 Chen, W.
138 Chen, X.
139 Chen, Y.
140 Chincarini, A.
141 Chiummo, A.
142 Cho, H. S.
143 Chow, J.
144 Christensen, N.
145 Chua, S. S. Y.
146 Chung, C. T. Y.
147 Chung, S.
148 Ciani, G.
149 Clara, F.
150 Clark, D. E.
151 Clark, J. A.
152 Clayton, J. H.
153 Cleva, F.
154 Coccia, E.
155 Cohadon, P-F
156 Colacino, C. N.
157 Colla, A.
158 Colombini, M.
159 Conte, A.
160 Conte, R.
161 Cook, D.
162 Corbitt, T. R.
163 Cordier, M.
164 Cornish, N.
165 Corsi, A.
166 Costa, Cesar Augusto
167 Coughlin, M.
168 Coulon, J-P
169 Couvares, P.
170 Coward, D. M.
171 Cowart, M.
172 Coyne, D. C.
173 Creighton, J. D. E.
174 Creighton, T. D.
175 Cruise, A. M.
176 Cumming, A.
177 Cunningham, L.
178 Cuoco, E.
179 Cutler, R. M.
180 Dahl, K.
181 Damjanic, M.
182 Danilishin, S. L.
183 D'Antonio, S.
184 Danzmann, K.
185 Dattilo, V.
186 Daudert, B.
187 Daveloza, H.
188 Davier, M.
189 Daw, E. J.
190 Day, R.
191 Dayanga, T.
192 De Rosa, R.
193 DeBbra, D.
194 Debreczeni, G.
195 Degallaix, J.
196 Del Pozzo, W.
197 Dent, T.
198 Dergachev, V.
199 DeRosa, R.
200 Dhurandhar, S.
201 Di Fiore, L.
202 Di Lieto, A.
203 Di Palma, I.
204 Emilio, M. Di Paolo
205 Di Virgilio, A.
206 Diaz, M.
207 Dietz, A.
208 Donovan, F.
209 Dooley, K. L.
210 Doravari, S.
211 Dorsher, S.
212 Drago, M.
213 Drever, R. W. P.
214 Driggers, J. C.
215 Du, Z.
216 Dumas, J-C
217 Dwyer, S.
218 Eberle, T.
219 Edgar, M.
220 Edwards, M.
221 Effler, A.
222 Ehrens, P.
223 Endroczi, G.
224 Engel, R.
225 Etzel, T.
226 Evans, K.
227 Evans, M.
228 Evans, T.
229 Factourovich, M.
230 Fafone, V.
231 Fairhurst, S.
232 Farr, B. F.
233 Favata, M.
234 Fazi, D.
235 Fehrmann, H.
236 Feldbaum, D.
237 Ferrante, I.
238 Ferrini, F.
239 Fidecaro, F.
240 Finn, L. S.
241 Fiori, I.
242 Fisher, R. P.
243 Flaminio, R.
244 Foley, S.
245 Forsi, E.
246 Forte, L. A.
247 Fotopoulos, N.
248 Fournier, J-D
249 Franc, J.
250 Franco, S.
251 Frasca, S.
252 Frasconi, F.
253 Frede, M.
254 Frei, M. A.
255 Frei, Z.
256 Freise, A.
257 Frey, R.
258 Fricke, T. T.
259 Friedrich, D.
260 Fritschel, P.
261 Frolov, V. V.
262 Fujimoto, M-K
263 Fulda, P. J.
264 Fyffe, M.
265 Gair, J.
266 Galimberti, M.
267 Gammaitoni, L.
268 Garcia, J.
269 Garufi, F.
270 Gaspar, M. E.
271 Gelencser, G.
272 Gemme, G.
273 Genin, E.
274 Gennai, A.
275 Gergely, L. A.
276 Ghosh, S.
277 Giaime, J. A.
278 Giampanis, S.
279 Giardina, K. D.
280 Giazotto, A.
281 Gil-Casanova, S.
282 Gill, C.
283 Gleason, J.
284 Goetz, E.
285 Gonzalez, G.
286 Gorodetsky, M. L.
287 Gossler, S.
288 Gouaty, R.
289 Graef, C.
290 Graff, P. B.
291 Granata, M.
292 Grant, A.
293 Gray, C.
294 Greenhalgh, R. J. S.
295 Gretarsson, A. M.
296 Griffo, C.
297 Grote, H.
298 Grover, K.
299 Grunewald, S.
300 Guidi, G. M.
301 Guido, C.
302 Gupta, R.
303 Gustafson, E. K.
304 Gustafson, R.
305 Hallam, J. M.
306 Hammer, D.
307 Hammond, G.
308 Hanks, J.
309 Hanna, C.
310 Hanson, J.
311 Hardt, A.
312 Harms, J.
313 Harry, G. M.
314 Harry, I. W.
315 Harstad, E. D.
316 Hartman, M. T.
317 Haughian, K.
318 Hayama, K.
319 Hayau, J-F
320 Heefner, J.
321 Heidmann, A.
322 Heintze, M. C.
323 Heitmann, H.
324 Hello, P.
325 Hemming, G.
326 Hendry, M. A.
327 Heng, I. S.
328 Heptonstall, A. W.
329 Herrera, V.
330 Heurs, M.
331 Hewitson, M.
332 Hild, S.
333 Hoak, D.
334 Hodge, K. A.
335 Holt, K.
336 Holtrop, M.
337 Hong, T.
338 Hooper, S.
339 Hough, J.
340 Howell, E. J.
341 Hughey, B.
342 Husa, S.
343 Huttner, S. H.
344 Huynh-Dinh, T.
345 Ingram, D. R.
346 Inta, R.
347 Isogai, T.
348 Ivanov, A.
349 Izumi, K.
350 Jacobson, M.
351 James, E.
352 Jang, Y. J.
353 Jaranowski, P.
354 Jesse, E.
355 Johnson, W. W.
356 Jones, D. I.
357 Jones, R.
358 Jonker, R. J. G.
359 Ju, L.
360 Kalmus, P.
361 Kalogera, V.
362 Kandhasamy, S.
363 Kang, G.
364 Kanner, J. B.
365 Kasprzack, M.
366 Kasturi, R.
367 Katsavounidis, E.
368 Katzman, W.
369 Kaufer, H.
370 Kaufman, K.
371 Kawabe, K.
372 Kawamura, S.
373 Kawazoe, F.
374 Keitel, D.
375 Kelley, D.
376 Kells, W.
377 Keppel, D. G.
378 Keresztes, Z.
379 Khalaidovski, A.
380 Khalili, F. Y.
381 Khazanov, E. A.
382 Kim, B. K.
383 Kim, C.
384 Kim, H.
385 Kim, K.
386 Kim, N.
387 Kim, Y. M.
388 King, P. J.
389 Kinzel, D. L.
390 Kissel, J. S.
391 Klimenko, S.
392 Kline, J.
393 Kokeyama, K.
394 Kondrashov, V.
395 Koranda, S.
396 Korth, W. Z.
397 Kowalska, I.
398 Kozak, D.
399 Kringel, V.
400 Krishnan, B.
401 Krolak, A.
402 Kuehn, G.
403 Kumar, P.
404 Kumar, R.
405 Kurdyumov, R.
406 Kwee, P.
407 Lam, P. K.
408 Landry, M.
409 Langley, A.
410 Lantz, B.
411 Lastzka, N.
412 Lawrie, C.
413 Lazzarini, A.
414 Le Roux, A.
415 Leaci, P.
416 Lee, C. H.
417 Lee, H. K.
418 Lee, H. M.
419 Leong, J. R.
420 Leonor, I.
421 Leroya, N.
422 Letendre, N.
423 Lhuillier, V.
424 Li, J.
425 Li, T. G. F.
426 Lindquist, P. E.
427 Litvine, V.
428 Liu, Y.
429 Liu, Z.
430 Lockerbie, N. A.
431 Lodhia, D.
432 Logue, J.
433 Lorenzini, M.
434 Loriette, V.
435 Lormand, M.
436 Losurdoa, G.
437 Lough, J.
438 Lubinski, M.
439 Lueck, H.
440 Lundgren, A. P.
441 Macarthur, J.
442 Macdonald, E.
443 Machenschalk, B.
444 MacInnis, M.
445 Macleod, D. M.
446 Mageswaran, M.
447 Mailand, K.
448 Majorana, E.
449 Maksimovic, I.
450 Malvezzi, V.
451 Man, N.
452 Mandel, I.
453 Mandic, V.
454 Mantovani, M.
455 Marchesoni, F.
456 Marion, F.
457 Marka, S.
458 Marka, Z.
459 Markosyan, A.
460 Maros, E.
461 Marque, J.
462 Martelli, F.
463 Martin, I. W.
464 Martin, R. M.
465 Marx, J. N.
466 Mason, K.
467 Masserot, A.
468 Matichard, F.
469 Matone, L.
470 Matzner, R. A.
471 Mavalvala, N.
472 Mazzolo, G.
473 McCarthy, R.
474 McClelland, D. E.
475 McGuire, S. C.
476 McIntyre, G.
477 McIver, J.
478 Meadors, G. D.
479 Mehmet, M.
480 Meier, T.
481 Melatos, A.
482 Melissinos, A. C.
483 Mendell, G.
484 Menendez, D. F.
485 Mercer, R. A.
486 Meshkov, S.
487 Messenger, C.
488 Meyer, M. S.
489 Miao, H.
490 Michel, C.
491 Milano, L.
492 Miller, J.
493 Minenkov, Y.
494 Mingarelli, C. M. F.
495 Mitrofanov, V. P.
496 Mitselmakher, G.
497 Mittleman, R.
498 Moe, B.
499 Mohan, M.
500 Mohapatra, S. R. P.
501 Moraru, D.
502 Moreno, G.
503 Morgado, N.
504 Morgia, A.
505 Mori, T.
506 Morriss, S. R.
507 Mosca, S.
508 Mossavi, K.
509 Mours, B.
510 Mow-Lowry, C. M.
511 Mueller, C. L.
512 Mueller, G.
513 Mukherjee, S.
514 Mullavey, A.
515 Mueller-Ebhardt, H.
516 Munch, J.
517 Murphy, D.
518 Murray, P. G.
519 Mytidis, A.
520 Nash, T.
521 Naticchioni, L.
522 Necula, V.
523 Nelson, J.
524 Neri, I.
525 Newton, G.
526 Nguyen, T.
527 Nishizawa, A.
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529 Nocera, F.
530 Nolting, D.
531 Normandin, M. E.
532 Nuttall, L.
533 Ochsner, E.
534 O'Dell, J.
535 Oelker, E.
536 Ogin, G. H.
537 Oh, J. J.
538 Oh, S. H.
539 Oldenberg, R. G.
540 O'Reilly, B.
541 O'Shaughnessy, R.
542 Osthelder, C.
543 Ott, C. D.
544 Ottaway, D. J.
545 Ottens, R. S.
546 Overmier, H.
547 Owen, B. J.
548 Page, A.
549 Palladino, L.
550 Palomba, C.
551 Pan, Y.
552 Pankow, C.
553 Paoletti, F.
554 Paoletti, R.
555 Papa, M. A.
556 Parisi, M.
557 Pasqualetti, A.
558 Passaquieti, R.
559 Passuello, D.
560 Pedraza, M.
561 Penn, S.
562 Perreca, A.
563 Persichetti, G.
564 Phelps, M.
565 Pichot, M.
566 Pickenpack, M.
567 Piergiovanni, F.
568 Pierro, V.
569 Pihlaja, M.
570 Pinard, L.
571 Pinto, I. M.
572 Pitkin, M.
573 Pletsch, H. J.
574 Plissi, M. V.
575 Poggiani, R.
576 Poeld, J.
577 Postiglione, F.
578 Poux, C.
579 Prato, M.
580 Predoi, V.
581 Prestegard, T.
582 Price, L. R.
583 Prijatelj, M.
584 Principe, M.
585 Privitera, S.
586 Prix, R.
587 Prodi, G. A.
588 Prokhorov, L. G.
589 Puncken, O.
590 Punturo, M.
591 Puppo, P.
592 Quetschke, V.
593 Quitzow-James, R.
594 Raab, F. J.
595 Rabeling, D. S.
596 Racz, I.
597 Radkins, H.
598 Raffai, P.
599 Rakhmanov, M.
600 Ramet, C.
601 Rankins, B.
602 Rapagnani, P.
603 Raymond, V.
604 Re, V.
605 Reed, C. M.
606 Reed, T.
607 Regimbaua, T.
608 Reed, S.
609 Reitze, D. H.
610 Ricci, F.
611 Riesen, R.
612 Riles, K.
613 Roberts, M.
614 Robertson, N. A.
615 Robinet, F.
616 Robinson, C.
617 Robinson, E. L.
618 Rocchi, A.
619 Roddy, S.
620 Rodriguez, C.
621 Rodruck, M.
622 Rolland, L.
623 Rollins, J. G.
624 Romano, J. D.
625 Romano, R.
626 Romie, J. H.
627 Rosinska, D.
628 Roever, C.
629 Rowan, S.
630 Ruediger, A.
631 Ruggi, P.
632 Ryan, K.
633 Salemi, F.
634 Sammut, L.
635 Sandberg, V.
636 Sankar, S.
637 Sannibale, V.
638 Santamaria, L.
639 Santiago-Prieto, I.
640 Santostasi, G.
641 Saracco, E.
642 Sassolas, B.
643 Sathyaprakash, B. S.
644 Saulson, P. R.
645 Savage, R. L.
646 Schilling, R.
647 Schnabel, R.
648 Schofield, R. M. S.
649 Schulz, B.
650 Schutz, B. F.
651 Schwinberg, P.
652 Scott, J.
653 Scott, S. M.
654 Seifert, F.
655 Sellers, D.
656 Sentenac, D.
657 Sergeev, A.
658 Shaddock, D. A.
659 Shaltev, M.
660 Shapiro, B.
661 Shawhan, P.
662 Shoemaker, D. H.
663 Sidery, T. L.
664 Siemens, X.
665 Sigg, D.
666 Simakov, D.
667 Singer, A.
668 Singer, L.
669 Sintes, A. M.
670 Skelton, G. R.
671 Slagmolen, B. J. J.
672 Slutsky, J.
673 Smith, J. R.
674 Smith, M. R.
675 Smith, R. J. E.
676 Smith-Lefebvre, N. D.
677 Somiya, K.
678 Sorazu, B.
679 Speirits, F. C.
680 Sperandio, L.
681 Stefszky, M.
682 Steinert, E.
683 Steinlechner, J.
684 Steinlechner, S.
685 Steplewski, S.
686 Stochino, A.
687 Stone, R.
688 Strain, K. A.
689 Strigin, S. E.
690 Stroeer, A. S.
691 Sturani, R.
692 Stuver, A. L.
693 Summerscales, T. Z.
694 Sung, M.
695 Susmithan, S.
696 Sutton, P. J.
697 Swinkels, B.
698 Szeifert, G.
699 Tacca, M.
700 Taffarello, L.
701 Talukder, D.
702 Tanner, D. B.
703 Tarabrin, S. P.
704 Taylor, R.
705 ter Braacka, A. P. M.
706 Thomas, P.
707 Thorne, K. A.
708 Thorne, K. S.
709 Thrane, E.
710 Thuering, A.
711 Titsler, C.
712 Tokmakov, K. V.
713 Tomlinson, C.
714 Toncelli, A.
715 Tonelli, M.
716 Torrea, O.
717 Torres, C. V.
718 Torrie, C. I.
719 Tournefier, E.
720 Travasso, F.
721 Traylor, G.
722 Tse, M.
723 Tucker, E.
724 Ugolini, D.
725 Vahlbruch, H.
726 Vajente, G.
727 van den Brandab, J. F. J.
728 Van den Broeck, C.
729 van der Putten, S.
730 van Veggel, A. A.
731 Vass, S.
732 Vasuth, M.
733 Vaulin, R.
734 Vavoulidis, M.
735 Vecchio, A.
736 Vedovato, G.
737 Veitch, J.
738 Veitch, P. J.
739 Venkateswara, K.
740 Verkindt, D.
741 Vetrano, F.
742 Vicere, A.
743 Villar, A. E.
744 Vinet, J-Y
745 Vitale, S.
746 Vocca, H.
747 Vorvick, C.
748 Vyatchanin, S. P.
749 Wade, A.
750 Wade, L.
751 Wade, M.
752 Waldman, S. J.
753 Wallace, L.
754 Wan, Y.
755 Wang, M.
756 Wang, X.
757 Wanner, A.
758 Ward, R. L.
759 Was, M.
760 Weinert, M.
761 Weinstein, A. J.
762 Weiss, R.
763 Welborn, T.
764 Wen, L.
765 Wessels, P.
766 West, M.
767 Westphal, T.
768 Wette, K.
769 Whelan, J. T.
770 Whitcomb, S. E.
771 White, D. J.
772 Whiting, B. F.
773 Wiesner, K.
774 Wilkinson, C.
775 Willems, P. A.
776 Williams, L.
777 Williams, R.
778 Willke, B.
779 Wimmer, M.
780 Winkelmann, L.
781 Winkler, W.
782 Wipf, C. C.
783 Wiseman, A. G.
784 Wittel, H.
785 Woan, G.
786 Wooley, R.
787 Worden, J.
788 Yablon, J.
789 Yakushin, I.
790 Yamamoto, H.
791 Yamamoto, K.
792 Yancey, C. C.
793 Yang, H.
794 Yeaton-Massey, D.
795 Yoshida, S.
796 Yvert, M.
797 Zadrozny, A.
798 Zanolin, M.
799 Zendri, J-P
800 Zhang, F.
801 Zhang, L.
802 Zhao, C.
803 Zotov, N.
804 Zucker, M. E.
805 Zweizig, J.
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166 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address  1
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JournalClassical and Quantum Gravity
Volume29
Number15
Secondary MarkB1_ASTRONOMIA_/_FÍSICA A2_ENGENHARIAS_I B1_ENGENHARIAS_IV C_ENSINO_DE_CIÊNCIAS_E_MATEMATICA A1_INTERDISCIPLINAR B1_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA
History (UTC)2018-06-05 04:14:43 :: administrator -> marciana :: 2012
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractBetween 2007 and 2010 Virgo collected data in coincidence with the LIGO and GEO gravitational-wave (GW) detectors. These data have been searched for GWs emitted by cataclysmic phenomena in the universe, by non-axisymmetric rotating neutron stars or from a stochastic background in the frequency band of the detectors. The sensitivity of GW searches is limited by noise produced by the detector or its environment. It is therefore crucial to characterize the various noise sources in a GW detector. This paper reviews the Virgo detector noise sources, noise propagation, and conversion mechanisms which were identified in the three first Virgo observing runs. In many cases, these investigations allowed us to mitigate noise sources in the detector, or to selectively flag noise events and discard them from the data. We present examples from the joint LIGO-GEO-Virgo GW searches to show how well noise transients and narrow spectral lines have been identified and excluded from the Virgo data. We also discuss how detector characterization can improve the astrophysical reach of GW searches.
AreaCEA
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Next Higher Units8JMKD3MGPCW/3ETR8EH
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6. Notes
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Reference TypeJournal Article
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/3D7B4LL
Repositorysid.inpe.br/mtc-m19/2012/12.12.16.33   (restricted access)
Last Update2013:01.24.13.02.37 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19/2012/12.12.16.33.14
Metadata Last Update2018:06.05.04.13.28 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1038/nature11597
ISSN0028-0836
Citation KeyOrtizSBALDPILCAUJMTGCCDMTGLGMCLMJWMSBOBRVWRSHDMHCAOCLOKSPGCE:2012:AlAtCo
TitleAlbedo and atmospheric constraints of dwarf planet Makemake from a stellar occultation
Year2012
MonthNov.
Access Date2024, Apr. 19
Secondary TypePRE PI
Number of Files1
Size424 KiB
2. Context
Author 1 Ortiz, J. L.
 2 Sicardy, B.
 3 Braga-Ribas, F.
 4 Alvarez-Candal, A.
 5 Lellouch, E.
 6 Duffard, R.
 7 Pinilla-Alonso, N.
 8 Ivanov, V. D.
 9 Littlefair, S. P.
10 Camargo, J. I. B.
11 Assafin, M.
12 Unda-Sanzana, E.
13 Jehin, E.
14 Morales, N.
15 Tancredi, G.
16 Gil-Hutton, R.
17 de la Cueva, I.
18 Colque, J. P.
19 Da Silva Neto, D. N.
20 Manfroid, J.
21 Thirouin, A.
22 GutiŽrrez, P. J.
23 Lecacheux, J.
24 Gillon, M.
25 Maury, A.
26 Colas, F.
27 Licandro, J.
28 Mueller, T.
29 Jacques, C.
30 Weaver, D.
31 Milone, A.
32 Salvo, R.
33 Bruzzone, S.
34 Organero, F.
35 Behrend, R.
36 Roland, S.
37 Vieira-Martins, R.
38 Widemann, T.
39 Roques, F.
40 Santos-Sanz, P.
41 Hestroffer, D.
42 Dhillon, V. S.
43 Marsh, T. R.
44 Harlingten, C.
45 Campo Bagatin, A.
46 Alonso, M. L.
47 Ortiz, M.
48 Colazo, C.
49 Lima, H.
50 Oliveira, A.
51 Kerber, L. O.
52 Smiljanic, R.
53 Pimentel, E.
54 Giacchini, B.
55 Cacella, P.
56 Emilio, M.
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31 Instituto Nacional de Pesquisas Espaciais (INPE)
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e-Mail Addressmarcelo.pazos@inpe.br
JournalNature
Volume491
Number7425
Pages566-569
History (UTC)2013-01-24 13:02:37 :: marcelo.pazos@sid.inpe.br -> administrator :: 2012
2018-06-05 04:13:28 :: administrator -> marcelo.pazos@inpe.br :: 2012
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Keywordstrans-neptunian objects
Kuiper-Belt objects
photometric-observations
Pluto
size
ERIS
ice
variability
centaurs
surface
AbstractPluto and Eris are icy dwarf planets with nearly identical sizes, comparable densities and similar surface compositions as revealed by spectroscopic studies(1,2). Pluto possesses an atmosphere whereas Eris does not; the difference probably arises from their differing distances from the Sun, and explains their different albedos(3). Makemake is another icy dwarf planet with a spectrum similar to Eris and Pluto(4), and is currently at a distance to the Sun intermediate between the two. Although Makemake's size (1,420 +/- 60 km) and albedo are roughly known(5,6), there has been no constraint on its density and there were expectations that it could have a Pluto-like atmosphere(4,7,8). Here we report the results from a stellar occultation by Makemake on 2011 April 23. Our preferred solution that fits the occultation chords corresponds to a body with projected axes of 1,430 +/- 9 km (1 sigma) and 1,502 +/- 45 km, implying a V-band geometric albedo p(V) = 0.77 +/- 0.03. This albedo is larger than that of Pluto, but smaller than that of Eris. The disappearances and reappearances of the star were abrupt, showing that Makemake has no global Pluto-like atmosphere at an upper limit of 4-12 nano-bar (1 sigma) for the surface pressure, although a localized atmosphere is possible. A density of 1.7 +/- 0.3 g cm(-3) is inferred from the data.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Albedo and atmospheric...
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Next Higher Units8JMKD3MGPCW/3ETR8EH
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Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn label lineage mark nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project resumeid rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject targetfile tertiarymark tertiarytype typeofwork url versiontype
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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/3D7AR9B
Repositorysid.inpe.br/mtc-m19/2012/12.12.15.15
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Metadata Repositorysid.inpe.br/mtc-m19/2012/12.12.15.15.12
Metadata Last Update2018:06.05.04.13.28 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1029/2012JA017820
ISSN0148-0227
2156-2202
Citation KeyLiNinAbdWanHu:2012:PrSiEv
TitlePrecursor signatures and evolution of post-sunset equatorial spread-F observed over Sanya
Year2012
MonthAug.
Access Date2024, Apr. 19
Secondary TypePRE PI
Number of Files1
Size4046 KiB
2. Context
Author1 Li, Guozhu
2 Ning, Baiqi
3 Abdu, M. A.
4 Wan, Weixing
5 Hu, Lianhuan
Group1
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3 DAS-CEA-INPE-MCTI-GOV-BR
Affiliation1 Chinese Acad Sci, Beijing Natl Observ Space Environm, Inst Geol & Geophys, Beijing 100029, Peoples R China.
2 Chinese Acad Sci, Beijing Natl Observ Space Environm, Inst Geol & Geophys, Beijing 100029, Peoples R China.
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Chinese Acad Sci, Beijing Natl Observ Space Environm, Inst Geol & Geophys, Beijing 100029, Peoples R China.
5 Chinese Acad Sci, Beijing Natl Observ Space Environm, Inst Geol & Geophys, Beijing 100029, Peoples R China.
JournalJournal of Geophysical Research
Volume117
NumberA08321
Secondary MarkB1_ASTRONOMIA_/_FÍSICA B2_CIÊNCIA_DA_COMPUTAÇÃO A1_CIÊNCIAS_AGRÁRIAS_I A1_ECOLOGIA_E_MEIO_AMBIENTE A1_ENGENHARIAS_I A2_ENGENHARIAS_II A1_ENGENHARIAS_III A2_ENGENHARIAS_IV A1_GEOCIÊNCIAS A1_INTERDISCIPLINAR
History (UTC)2012-12-12 15:23:39 :: marciana -> administrator :: 2012
2012-12-12 15:23:50 :: administrator -> marciana :: 2012
2013-01-31 14:49:36 :: marciana -> administrator :: 2012
2013-02-04 17:32:33 :: administrator -> banon :: 2012
2013-02-04 17:33:17 :: banon -> administrator :: 2012
2018-06-05 04:13:28 :: administrator -> marciana :: 2012
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsplasma bubbles
electric-field
irregularities
ionosphere
radar
campaign
drift
AbstractRecent case studies on the precursor signatures of equatorial spread-F (ESF) have shown a one-to-one correspondence between the large-scale wave structures (LSWS) and ESF development at equatorial latitude. In this study, the LSWS and the onset and development of the ESF are investigated over Sanya (18 degrees N, 109 degrees E), a station located at 13 degrees north of the magnetic equator, during both geomagnetic quiet and disturbed conditions in September-October 2011. High-time-resolution ionograms from Digisonde Portable Sounder (DPS-4D) provided the satellite trace measurements that were used to indicate the occurrence of the LSWS. The development of local ESF activity was identified using GPS scintillation and VHF coherent radar echo measurements from the same site, together with the range type spread-F (RSF) in ionograms. Additionally, the Sanya VHF radar five-beam scanning measurements in east-west direction were used to characterize the longitudinal difference in establishing the initial conditions for ESF development. Correlative studies between the LSWS and ESF activities during the observational period offer consolidated evidence that the LSWS is a necessary precursor for the ESF development. It is shown that the LSWS and ESF have nearly a one-to-one relationship when the F layer undergoes an abrupt post-sunset rise (PSSR), revealing that the magnitude of the pre-reversal enhancement in zonal electric field (PRE) that elevates the F layer to a high enough altitude is an important parameter controlling the generation of post-sunset ESF. However, in the absence of the PSSR, the ESF and GPS scintillation did not always occur following the appearance of LSWS. Sometimes the LSWS events preceded the generation of bottom type spread-F (BSF) that did not develop vertically into ESF and radar plumes. This result may indicate that under inexpressive, weak, or even moderate PRE conditions, the appearance of the LSWS alone may not be sufficient to produce the post-sunset F region irregularities responsible for ionospheric scintillations. More factors, other than the LSWS, could play crucial roles favoring the growth of ESF instabilities responsible for ionospheric scintillations.
AreaCST
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Precursor signatures and...
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP7W/3D7AR9B
zipped data URLhttp://urlib.net/zip/8JMKD3MGP7W/3D7AR9B
Languageen
User Groupadministrator
banon
marciana
Reader Groupadministrator
marciana
Visibilityshown
Archiving Policydenypublisher6 allowfinaldraft
Update Permissionnot transferred
5. Allied materials
Mirror Repositorysid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Next Higher Units8JMKD3MGPCW/3ETR8EH
DisseminationWEBSCI; AGU; MGA; COMPENDEX.
Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress electronicmailaddress format isbn label lineage mark nextedition notes orcid pages parameterlist parentrepositories previousedition previouslowerunit progress project readpermission resumeid rightsholder schedulinginformation secondarydate session shorttitle sponsor subject targetfile tertiarymark tertiarytype typeofwork url
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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/3D76SBL
Repositorysid.inpe.br/mtc-m19/2012/12.11.17.36
Last Update2013:01.23.17.25.03 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19/2012/12.11.17.36.41
Metadata Last Update2018:06.05.04.13.27 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1111/j.1365-2966.2012.21848.x
ISSN1365-2966
Citation KeyLaBarberaFeCaBrChPaMe:2012:ReStPo
TitleSPIDER - VII. Revealing the stellar population content of massive early-type galaxies out to 8Re
Year2012
MonthNov.
Access Date2024, Apr. 19
Secondary TypePRE PI
Number of Files1
Size1364 KiB
2. Context
Author1 La Barbera, F.
2 Ferreras, I.
3 Carvalho, R. R.
4 Bruzual, G.
5 Charlot, S.
6 Pasquali, A.
7 Merlin, E.
Group1
2
3 DAS-CEA-INPE-MCTI-GOV-BR
Affiliation1 INAF Osservatorio Astron Capodimonte, Naples, Italy.
2 Univ Coll London, MSSL, Dorking RH5 6NT, Surrey, England
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Univ Nacl Autonoma Mexico, Ctr Radioastron & Astrofis, Mexico City, DF, Mexico
5 UPMC, Inst Astrophys Paris, UMR7095, F-75014 Paris, France
6 Univ Heidelberg, Zentrum Astron, Astron Rechen Inst, D-69120 Heidelberg, Germany
7 INAF Osservatorio Astron Padova, Padua, Italy
JournalMonthly Notices of the Royal Astronomical Society
Volume426 10.1111/j.1365-2966.2012.21848.x
Number3
Pages2300 - 2317
Secondary MarkA2_ASTRONOMIA_/_FÍSICA A1_ENGENHARIAS_III C_ENSINO_DE_CIÊNCIAS_E_MATEMATICA A1_INTERDISCIPLINAR A2_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA A1_QUÍMICA
History (UTC)2012-12-11 17:41:36 :: marciana -> administrator :: 2012
2013-01-23 17:20:54 :: administrator -> marciana :: 2012
2013-02-26 19:29:09 :: marciana -> administrator :: 2012
2018-06-05 04:13:27 :: administrator -> marciana :: 2012
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Keywordselliptical and lenticular galaxies
cD
galaxy evolution
galaxy formation
stellar content
AbstractRadial trends of stellar populations in galaxies provide a valuable tool to understand the mechanisms of galaxy growth. In this paper, we present the first comprehensive analysis of opticaloptical and opticalNIR colours, as a function of galaxy mass, out to the halo region (8Re) of early-type galaxies (ETGs). We select a sample of 674 massive ETGs (M⋆> 3 × 1010M⊙) from the SDSS-based SPIDER survey. By com-paring with a large range of population synthesis models, we derive robust constraints on the radial trends in age and metallicity. Metallicity is unambiguously found to decrease outwards, with a measurable steepening of the slope in the outer regions (Re < R < 8Re). The gradients in stellar age are found to be more sensitive to the models used, but in general, the outer regions of ETGs feature older populations compared to the cores. This trend is strongest for the most massive galaxies in our sample (M⋆> 1011M⊙). Furthermore, when segregating with respect to large scale environment, the age gradient is more significant in ETGs residing in higher density regions. These results shed light on the processes leading from the formation of the central core to the growth of the stellar envelope of massive galaxies. The fact that the populations in the outer regions are older and more metal-poor than in the core suggests a process whereby the envelope of massive galaxies is made up of accreted small satellites (i.e. minor mergers) whose stars were born during the first stages of galaxy formation.
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Sitemtc-m16d.sid.inpe.br
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Secondary KeyINPE--PRE/
DOI10.1088/1475-7516/2012/11/054
ISSN1475-7516
Citation KeyBessadaPintSiffMira:2012:StBaRe
TitleStochastic background of relic gravitons in a bouncing quantum cosmological model
Year2012
Access Date2024, Apr. 19
Secondary TypePRE PI
Number of Files1
Size359 KiB
2. Context
Author1 Bessada, Dennis
2 Pinto-Neto, Nelson
3 Siffertb, Beatriz B.
4 Miranda, Oswaldo D.
Group1
2
3
4 DAS-CEA-INPE-MCTI-GOV-BR
Affiliation1
2
3
4 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1
2
3
4 oswaldo@das.inpe.br
e-Mail Addressmarcelo.pazos@inpe.br
JournalJournal of Cosmology and Astroparticle Physics
Volume117
Number54
Secondary MarkA1_ASTRONOMIA_/_FÍSICA A1_GEOCIÊNCIAS
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Reference TypeJournal Article
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/3D66M7E
Repositorysid.inpe.br/mtc-m19/2012/12.05.12.56
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Secondary KeyINPE--PRE/
DOI10.1103/PhysRevD.86.083502
ISSN1550-2368
1550-7998
Citation KeyBessadaKinn:2012:AtSoTa
TitleAttractor solutions in tachyacoustic cosmology
ProjectNational Science Foundation NSF-PHY-1066278 Brazilian agency FAPESP 2009/15612-6
Year2012
MonthOct.
Access Date2024, Apr. 19
Secondary TypePRE PI
Number of Files1
Size371 KiB
2. Context
Author1 Bessada, Dennis
2 Kinney, William H.
Group1 DAS-CEA-INPE-MCTI-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 SUNY Buffalo, Dept Phys, Buffalo, NY 14260 USA
JournalPhysical Review D
Volume86
Number8
PagesArticle number083502
Secondary MarkA2_ASTRONOMIA_/_FÍSICA B1_INTERDISCIPLINAR A2_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA
History (UTC)2013-01-30 16:19:34 :: marciana -> administrator :: 2012
2013-01-30 16:22:36 :: administrator -> marciana :: 2012
2013-02-04 16:24:15 :: marciana -> administrator :: 2012
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KeywordsINFLATIONARY UNIVERSE
SCENARIO
FLATNESS
HORIZON
AbstractWe study the dynamical stability of tachyacoustic cosmological models, in which primordial perturbations are generated by a shrinking sound horizon during a period of decelerating expansion. Such models represent a potential alternative to inflationary cosmology, but the phase-space behavior of tachyacoustic solutions has not previously been investigated. We numerically evaluate the dynamics of two noncanonical Lagrangians, a cuscuton-like Lagrangian and a Dirac-Born-Infeld Lagrangian, which generate a scale-invariant spectrum of perturbations. We show that the power-law background solutions in both cases are dynamical attractors.
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Reference TypeJournal Article
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/3D57R2B
Repositorysid.inpe.br/mtc-m19/2012/11.29.15.33   (restricted access)
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Secondary KeyINPE--PRE/
DOI10.1088/1475-7516/2012/09/018
ISSN1475-7516
Citation KeyBessada:2012:NoSiTa
TitleNon-Gaussian signatures of tachyacoustic cosmology
Year2012
MonthSet.
Access Date2024, Apr. 19
Secondary TypePRE PI
Number of Files1
Size469 KiB
2. Context
AuthorBessada, Dennis
GroupDAS-CEA-INPE-MCTI-GOV-BR
AffiliationInstituto Nacional de Pesquisas Espaciais (INPE); Universidade Federal de São Paulo, Laboratório de Física Teórica e Computação Científica, Rua São Nicolau, 210, 09913-030, Diadema, SP, Brazil
JournalJournal of Cosmology and Astroparticle Physics
Volume2012
Number9
PagesArticle number018
History (UTC)2012-12-05 11:55:33 :: marciana -> administrator :: 2012
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Keywordsalternatives to inflation
cosmological perturbation theory
physics of the early universe
AbstractI investigate non-Gaussian signatures in the context of tachyacoustic cosmology, that is, a noninflationary model with superluminal speed of sound. I calculate the full non-Gaussian amplitude , its size fNL, and corresponding shapes for a red-tilted spectrum of primordial scalar perturbations. Specifically, for cuscuton-like models I show that fNL ~ (1), and the shape of its non-Gaussian amplitude peaks for both equilateral and local configurations, the latter being dominant. These results, albeit similar, are quantitatively distinct from the corresponding ones obtained by Magueijo et al. in the context of superluminal bimetric models.
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Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress electronicmailaddress format isbn label lineage mark nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project resumeid rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject targetfile tertiarymark tertiarytype typeofwork url
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Reference TypeJournal Article
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/3CGEBGE
Repositorysid.inpe.br/mtc-m19/2012/08.24.17.08   (restricted access)
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Secondary KeyINPE--PRE/
DOI10.1016/j.asr.2012.03.004
ISSN0273-1177
Citation KeyFernandesDutrCunhSawa:2012:FlLoPa
TitleFlaring loop parameters estimated from solar decimeter type U-like and type J-like fine structures
ProjectCNPq 480045/2008-9
Year2012
MonthJune
Access Date2024, Apr. 19
Secondary TypePRE PI
Number of Files1
Size494 KiB
2. Context
Author1 Fernandes, Francisco C. R.
2 Dutra, José Augusto S. S
3 Cunha Da Silva, Rafael D.
4 Sawant, Hanumant S.
Group1
2
3
4 DAS-CEA-INPE-MCTI-GOV-BR
Affiliation1 Laboratório de Física e Astronomia, IP and D, UNIVAP, Av. Shishima Hifumi. 2911-Urbanova, CEP 12244-000, São José dos Campos, SP, Brazil
2 Laboratório de Física e Astronomia, IP and D, UNIVAP, Av. Shishima Hifumi. 2911-Urbanova, CEP 12244-000, São José dos Campos, SP, Brazil
3 Laboratório de Física e Astronomia, IP and D, UNIVAP, Av. Shishima Hifumi. 2911-Urbanova, CEP 12244-000, São José dos Campos, SP, Brazil
4 Instituto Nacional de Pesquisas Espaciais (INPE)
JournalAdvances in Space Research
Volume49
Number11
Pages1607-1614
History (UTC)2012-08-24 17:08:04 :: marciana -> administrator ::
2012-08-24 17:08:06 :: administrator -> marciana :: 2012
2012-08-30 18:03:34 :: marciana -> banon :: 2012
2013-02-19 13:53:59 :: banon -> marciana :: 2012
2013-02-19 14:11:08 :: marciana -> banon :: 2012
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2018-06-05 04:12:55 :: administrator -> marciana :: 2012
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KeywordsElectron beams - Frequency bands - Magnetic fields - Solar radiation - Sun
AbstractThis work presents the analysis of five fine structures in the solar radio emission, observed between June 2000 and October 2001 by the Brazilian Solar Spectroscope (BSS), in the decimeter frequency band of 950-2500 MHz. Based on their morphological characteristics identified in the dynamic spectra, the fine structures had been classified as type U-like or type J-like bursts. Such emissions are variants of the type III bursts. They support the hypothesis of generation by plasma emission mechanism, from interaction of electron beams accelerated during solar flares, propagating along closed magnetic structures, within the trapped plasma of the solar corona. The spectral and temporal characteristics of the five fine structures had been obtained from the dynamic spectra and the parameters of the agent and the emitting source have been determined, assuming both fundamental and harmonic emissions. The analysis revealed the flux density of the structures is less than 20-80 s.f.u. For assumption of harmonic emission, the interval of values for the source parameters estimated are: the loop size is (0.3-5.1) × 1010 cm; the electron beam velocity is in the range of 0.16-0.53 c; the temperature of coronal loop top is of the order of (0.25-1.55) × 107 K; and the low limit for the magnetic field is of 7-26 G. These results are in agreement with previous determinations reported in the literature.
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Reference TypeJournal Article
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/3CG6U78
Repositorysid.inpe.br/mtc-m19/2012/08.23.00.46
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Secondary KeyINPE--PRE/
DOI10.1103/PhysRevD.85.122007
ISSN1550-2368
1550-7998
Citation KeyAbadieAAAAAAAAAAAAACAAAAAAAAAAAABBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCDDDDDDDDDDDDRDDDPDDDDDDDDEDDDDDDDDDDDEEEEEEEEEEEFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHIIIIIJJJJJJJJJJKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMNNNNNNNNNNNNNOOOOOOOOOOOOOOPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPQQRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSTTTTTTTTTTTTTTTTTTTTTTTTUVVBVPVVVVVVVVVVVVVVVVVVVWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWYYYYYYYYYZZZZZZZZZZCC:2012:AlSeGr
TitleAll-sky search for gravitational-wave bursts in the second joint LIGO-Virgo run
Year2012
MonthJun.
Access Date2024, Apr. 19
Secondary TypePRE PI
Number of Files1
Size1353 KiB
2. Context
Author  1 Abadie, J.
  2 Abbott, B. P.
  3 Abbott, R.
  4 Abbott, T. D.
  5 Abernathy, M.
  6 Accadia, T.
  7 Acernese, F.
  8 Adams, C.
  9 Adhikari, R.
 10 Affeldt, C.
 11 Agathos, M.
 12 Agatsuma, K.
 13 Ajith, P.
 14 Allen, B.
 15 Ceron, E. Amador
 16 Amariutei, D.
 17 Anderson, S. B.
 18 Anderson, W. G.
 19 Arai, K.
 20 Arain, M. A.
 21 Araya, M. C.
 22 Aston, S. M.
 23 Astone, P.
 24 Atkinson, D.
 25 Aufmuth, P.
 26 Aulbert, C.
 27 Aylott, B. E.
 28 Babak, S.
 29 Baker, P.
 30 Ballardin, G.
 31 Ballmer, S.
 32 Barayoga, J. C. B.
 33 Barker, D.
 34 Barone, F.
 35 Barr, B.
 36 Barsotti, L.
 37 Barsuglia, M.
 38 Barton, M. A.
 39 Bartos, I.
 40 Bassiri, R.
 41 Bastarrika, M.
 42 Basti, A.
 43 Batch, J.
 44 Bauchrowitz, J.
 45 Bauer, Th. S.
 46 Bebronne, M.
 47 Beck, D.
 48 Behnke, B.
 49 Bejger, M.
 50 Beker, M. G.
 51 Bell, A. S.
 52 Belletoile, A.
 53 Belopolski, I.
 54 Benacquista, M.
 55 Berliner, J. M.
 56 Bertolini, A.
 57 Betzwieser, J.
 58 Beveridge, N.
 59 Beyersdorf, P. T.
 60 Bilenko, I. A.
 61 Billingsley, G.
 62 Birch, J.
 63 Biswas, R.
 64 Bitossi, M.
 65 Bizouard, M. A.
 66 Black, E.
 67 Blackburn, J. K.
 68 Blackburn, L.
 69 Blair, D.
 70 Bland, B.
 71 Blom, M.
 72 Bock, O.
 73 Bodiya, T. P.
 74 Bogan, C.
 75 Bondarescu, R.
 76 Bondu, F.
 77 Bonelli, L.
 78 Bonnand, R.
 79 Bork, R.
 80 Born, M.
 81 Boschi, V.
 82 Bose, S.
 83 Bosi, L.
 84 Bouhou, B.
 85 Braccini, S.
 86 Bradaschia, C.
 87 Brady, P. R.
 88 Braginsky, V. B.
 89 Branchesi, M.
 90 Brau, J. E.
 91 Breyer, J.
 92 Briant, T.
 93 Bridges, D. O.
 94 Brillet, A.
 95 Brinkmann, M.
 96 Brisson, V.
 97 Britzger, M.
 98 Brooks, A. F.
 99 Brown, D. A.
100 Bulik, T.
101 Bulten, H. J.
102 Buonanno, A.
103 Burguet-Castell, J.
104 Buskulic, D.
105 Buy, C.
106 Byer, R. L.
107 Cadonati, L.
108 Cagnoli, G.
109 Calloni, E.
110 Camp, J. B.
111 Campsie, P.
112 Cannizzo, J.
113 Cannon, K.
114 Canuel, B.
115 Cao, J.
116 Capano, C. D.
117 Carbognani, F.
118 Carbone, L.
119 Caride, S.
120 Caudill, S.
121 Cavaglia, M.
122 Cavalier, F.
123 Cavalieri, R.
124 Cella, G.
125 Cepeda, C.
126 Cesarini, E.
127 Chaibi, O.
128 Chalermsongsak, T.
129 Charlton, P.
130 Chassande-Mottin, E.
131 Chelkowski, S.
132 Chen, W.
133 Chen, X.
134 Chen, Y.
135 Chincarini, A.
136 Chiummo, A.
137 Cho, H. S.
138 Chow, J.
139 Christensen, N.
140 Chua, S. S. Y.
141 Chung, C. T. Y.
142 Chung, S.
143 Ciani, G.
144 Clara, F.
145 Clark, D. E.
146 Clark, J.
147 Clayton, J. H.
148 Cleva, F.
149 Coccia, E.
150 Cohadon, P. -F.
151 Colacino, C. N.
152 Colas, J.
153 Colla, A.
154 Colombini, M.
155 Conte, A.
156 Conte, R.
157 Cook, D.
158 Corbitt, T. R.
159 Cordier, M.
160 Cornish, N.
161 Corsi, A.
162 Costa, César Augusto
163 Coughlin, M.
164 Coulon, J. -P.
165 Couvares, P.
166 Coward, D. M.
167 Cowart, M.
168 Coyne, D. C.
169 Creighton, J. D. E.
170 Creighton, T. D.
171 Cruise, A. M.
172 Cumming, A.
173 Cunningham, L.
174 Cuoco, E.
175 Cutler, R. M.
176 Dahl, K.
177 Danilishin, S. L.
178 Dannenberg, R.
179 D'Antonio, S.
180 Danzmann, K.
181 Dattilo, V.
182 Daudert, B.
183 Daveloza, H.
184 Davier, M.
185 Daw, E. J.
186 Day, R.
187 Dayanga, T.
188 De Rosa, R.
189 DeBra, D.
190 Debreczeni, G.
191 Del Pozzo, W.
192 del Prete, M.
193 Dent, T.
194 Dergachev, V.
195 DeRosa, R.
196 DeSalvo, R.
197 Dhurandhar, S.
198 Di Fiore, L.
199 Di Lieto, A.
200 Di Palma, I.
201 Emilio, M. Di Paolo
202 Di Virgilio, A.
203 Diaz, M.
204 Dietz, A.
205 Donovan, F.
206 Dooley, K. L.
207 Drago, M.
208 Drever, R. W. P.
209 Driggers, J. C.
210 Du, Z.
211 Dumas, J. -C.
212 Dwyer, S.
213 Eberle, T.
214 Edgar, M.
215 Edwards, M.
216 Effler, A.
217 Ehrens, P.
218 Endroczi, G.
219 Engel, R.
220 Etzel, T.
221 Evans, K.
222 Evans, M.
223 Evans, T.
224 Factourovich, M.
225 Fafone, V.
226 Fairhurst, S.
227 Fan, Y.
228 Farr, B. F.
229 Fazi, D.
230 Fehrmann, H.
231 Feldbaum, D.
232 Feroz, F.
233 Ferrante, I.
234 Fidecaro, F.
235 Finn, L. S.
236 Fiori, I.
237 Fisher, R. P.
238 Flaminio, R.
239 Flanigan, M.
240 Foley, S.
241 Forsi, E.
242 Forte, L. A.
243 Fotopoulos, N.
244 Fournier, J. -D.
245 Franc, J.
246 Frasca, S.
247 Frasconi, F.
248 Frede, M.
249 Frei, M.
250 Frei, Z.
251 Freise, A.
252 Frey, R.
253 Fricke, T. T.
254 Friedrich, D.
255 Fritschel, P.
256 Frolov, V. V.
257 Fujimoto, M. -K.
258 Fulda, P. J.
259 Fyffe, M.
260 Gair, J.
261 Galimberti, M.
262 Gammaitoni, L.
263 Garcia, J.
264 Garufi, F.
265 Gaspar, M. E.
266 Gemme, G.
267 Geng, R.
268 Genin, E.
269 Gennai, A.
270 Gergely, L. A.
271 Ghosh, S.
272 Giaime, J. A.
273 Giampanis, S.
274 Giardina, K. D.
275 Giazotto, A.
276 Gil-Casanova, S.
277 Gill, C.
278 Gleason, J.
279 Goetz, E.
280 Goggin, L. M.
281 Gonzalez, G.
282 Gorodetsky, M. L.
283 Gossler, S.
284 Gouaty, R.
285 Graef, C.
286 Graff, P. B.
287 Granata, M.
288 Grant, A.
289 Gras, S.
290 Gray, C.
291 Gray, N.
292 Greenhalgh, R. J. S.
293 Gretarsson, A. M.
294 Greverie, C.
295 Grosso, R.
296 Grote, H.
297 Grunewald, S.
298 Guidi, G. M.
299 Guido, C.
300 Gupta, R.
301 Gustafson, E. K.
302 Gustafson, R.
303 Ha, T.
304 Hallam, J. M.
305 Hammer, D.
306 Hammond, G.
307 Hanks, J.
308 Hanna, C.
309 Hanson, J.
310 Harms, J.
311 Hardt, A.
312 Harry, G. M.
313 Harry, I. W.
314 Harstad, E. D.
315 Hartman, M. T.
316 Haughian, K.
317 Hayama, K.
318 Hayau, J. -F.
319 Heefner, J.
320 Heidmann, A.
321 Heintze, M. C.
322 Heitmann, H.
323 Hello, P.
324 Hendry, M. A.
325 Heng, I. S.
326 Heptonstall, A. W.
327 Herrera, V.
328 Hewitson, M.
329 Hild, S.
330 Hoak, D.
331 Hodge, K. A.
332 Holt, K.
333 Holtrop, M.
334 Hong, T.
335 Hooper, S.
336 Hosken, D. J.
337 Hough, J.
338 Howell, E. J.
339 Hughey, B.
340 Husa, S.
341 Huttner, S. H.
342 Huynh-Dinh, T.
343 Ingram, D. R.
344 Inta, R.
345 Isogai, T.
346 Ivanov, A.
347 Izumi, K.
348 Jacobson, M.
349 James, E.
350 Jang, Y. J.
351 Jaranowski, P.
352 Jesse, E.
353 Johnson, W. W.
354 Jones, D. I.
355 Jones, G.
356 Jones, R.
357 Ju, L.
358 Kalmus, P.
359 Kalogera, V.
360 Kandhasamy, S.
361 Kang, G.
362 Kanner, J. B.
363 Kasturi, R.
364 Katsavounidis, E.
365 Katzman, W.
366 Kaufer, H.
367 Kawabe, K.
368 Kawamura, S.
369 Kawazoe, F.
370 Kelley, D.
371 Kells, W.
372 Keppel, D. G.
373 Keresztes, Z.
374 Khalaidovski, A.
375 Khalili, F. Y.
376 Khazanov, E. A.
377 Kim, B. K.
378 Kim, C.
379 Kim, H.
380 Kim, K.
381 Kim, N.
382 Kim, Y. M.
383 King, P. J.
384 Kinzel, D. L.
385 Kissel, J. S.
386 Klimenko, S.
387 Kokeyama, K.
388 Kondrashov, V.
389 Koranda, S.
390 Korth, W. Z.
391 Kowalska, I.
392 Kozak, D.
393 Kranz, O.
394 Kringel, V.
395 Krishnamurthy, S.
396 Krishnan, B.
397 Krolak, A.
398 Kuehn, G.
399 Kumar, R.
400 Kwee, P.
401 Lam, P. K.
402 Landry, M.
403 Lantz, B.
404 Lastzka, N.
405 Lawrie, C.
406 Lazzarini, A.
407 Leaci, P.
408 Lee, C. H.
409 Lee, H. K.
410 Lee, H. M.
411 Leong, J. R.
412 Leonor, I.
413 Leroy, N.
414 Letendre, N.
415 Li, J.
416 Li, T. G. F.
417 Liguori, N.
418 Lindquist, P. E.
419 Liu, Y.
420 Liu, Z.
421 Lockerbie, N. A.
422 Lodhia, D.
423 Lorenzini, M.
424 Loriette, V.
425 Lormand, M.
426 Losurdo, G.
427 Lough, J.
428 Luan, J.
429 Lubinski, M.
430 Lueck, H.
431 Lundgren, A. P.
432 Macdonald, E.
433 Machenschalk, B.
434 MacInnis, M.
435 Macleod, D. M.
436 Mageswaran, M.
437 Mailand, K.
438 Majorana, E.
439 Maksimovic, I.
440 Man, N.
441 Mandel, I.
442 Mandic, V.
443 Mantovani, M.
444 Marandi, A.
445 Marchesoni, F.
446 Marion, F.
447 Marka, S.
448 Marka, Z.
449 Markosyan, A.
450 Maros, E.
451 Marque, J.
452 Martelli, F.
453 Martin, I. W.
454 Martin, R. M.
455 Marx, J. N.
456 Mason, K.
457 Masserot, A.
458 Matichard, F.
459 Matone, L.
460 Matzner, R. A.
461 Mavalvala, N.
462 Mazzolo, G.
463 McCarthy, R.
464 McClelland, D. E.
465 McGuire, S. C.
466 McIntyre, G.
467 McIver, J.
468 McKechan, D. J. A.
469 McWilliams, S.
470 Meadors, G. D.
471 Mehmet, M.
472 Meier, T.
473 Melatos, A.
474 Melissinos, A. C.
475 Mendell, G.
476 Mercer, R. A.
477 Meshkov, S.
478 Messenger, C.
479 Meyer, M. S.
480 Miao, H.
481 Michel, C.
482 Milano, L.
483 Miller, J.
484 Minenkov, Y.
485 Mitrofanov, V. P.
486 Mitselmakher, G.
487 Mittleman, R.
488 Miyakawa, O.
489 Moe, B.
490 Mohan, M.
491 Mohanty, S. D.
492 Mohapatra, S. R. P.
493 Moraru, D.
494 Moreno, G.
495 Morgado, N.
496 Morgia, A.
497 Mori, T.
498 Morriss, S. R.
499 Mosca, S.
500 Mossavi, K.
501 Mours, B.
502 Mow-Lowry, C. M.
503 Mueller, C. L.
504 Mueller, G.
505 Mukherjee, S.
506 Mullavey, A.
507 Mueller-Ebhardt, H.
508 Munch, J.
509 Murphy, D.
510 Murray, P. G.
511 Mytidis, A.
512 Nash, T.
513 Naticchioni, L.
514 Necula, V.
515 Nelson, J.
516 Neri, I.
517 Newton, G.
518 Nguyen, T.
519 Nishizawa, A.
520 Nitz, A.
521 Nocera, F.
522 Nolting, D.
523 Normandin, M. E.
524 Nuttall, L.
525 Ochsner, E.
526 O'Dell, J.
527 Oelker, E.
528 Ogin, G. H.
529 Oh, J. J.
530 Oh, S. H.
531 O'Reilly, B.
532 O'Shaughnessy, R.
533 Osthelder, C.
534 Ott, C. D.
535 Ottaway, D. J.
536 Ottens, R. S.
537 Overmier, H.
538 Owen, B. J.
539 Page, A.
540 Pagliaroli, G.
541 Palladino, L.
542 Palomba, C.
543 Pan, Y.
544 Pankow, C.
545 Paoletti, F.
546 Papa, M. A.
547 Parisi, M.
548 Pasqualetti, A.
549 Passaquieti, R.
550 Passuello, D.
551 Patel, P.
552 Pedraza, M.
553 Peiris, P.
554 Pekowsky, L.
555 Penn, S.
556 Perreca, A.
557 Persichetti, G.
558 Phelps, M.
559 Pichot, M.
560 Pickenpack, M.
561 Piergiovanni, F.
562 Pietka, M.
563 Pinard, L.
564 Pinto, I. M.
565 Pitkin, M.
566 Pletsch, H. J.
567 Plissi, M. V.
568 Poggiani, R.
569 Poeld, J.
570 Postiglione, F.
571 Prato, M.
572 Predoi, V.
573 Prestegard, T.
574 Price, L. R.
575 Prijatelj, M.
576 Principe, M.
577 Privitera, S.
578 Prix, R.
579 Prodi, G. A.
580 Prokhorov, L. G.
581 Puncken, O.
582 Punturo, M.
583 Puppo, P.
584 Quetschke, V.
585 Quitzow-James, R.
586 Raab, F. J.
587 Rabeling, D. S.
588 Racz, I.
589 Radkins, H.
590 Raffai, P.
591 Rakhmanov, M.
592 Rankins, B.
593 Rapagnani, P.
594 Raymond, V.
595 Re, V.
596 Redwine, K.
597 Reed, C. M.
598 Reed, T.
599 Regimbau, T.
600 Reid, S.
601 Reitze, D. H.
602 Ricci, F.
603 Riesen, R.
604 Riles, K.
605 Robertson, N. A.
606 Robinet, F.
607 Robinson, C.
608 Robinson, E. L.
609 Rocchi, A.
610 Roddy, S.
611 Rodriguez, C.
612 Rodruck, M.
613 Rolland, L.
614 Rollins, J. G.
615 Romano, J. D.
616 Romano, R.
617 Romie, J. H.
618 Rosinska, D.
619 Roever, C.
620 Rowan, S.
621 Ruediger, A.
622 Ruggi, P.
623 Ryan, K.
624 Sainathan, P.
625 Salemi, F.
626 Sammut, L.
627 Sandberg, V.
628 Sannibale, V.
629 Santamaria, L.
630 Santiago-Prieto, I.
631 Santostasi, G.
632 Sassolas, B.
633 Sathyaprakash, B. S.
634 Sato, S.
635 Saulson, P. R.
636 Savage, R. L.
637 Schilling, R.
638 Schnabel, R.
639 Schofield, R. M. S.
640 Schreiber, E.
641 Schulz, B.
642 Schutz, B. F.
643 Schwinberg, P.
644 Scott, J.
645 Scott, S. M.
646 Seifert, F.
647 Sellers, D.
648 Sentenac, D.
649 Sergeev, A.
650 Shaddock, D. A.
651 Shaltev, M.
652 Shapiro, B.
653 Shawhan, P.
654 Shoemaker, D. H.
655 Sibley, A.
656 Siemens, X.
657 Sigg, D.
658 Singer, A.
659 Singer, L.
660 Sintes, A. M.
661 Skelton, G. R.
662 Slagmolen, B. J. J.
663 Slutsky, J.
664 Smith, J. R.
665 Smith, M. R.
666 Smith, R. J. E.
667 Smith-Lefebvre, N. D.
668 Somiya, K.
669 Sorazu, B.
670 Soto, J.
671 Speirits, F. C.
672 Sperandio, L.
673 Stefszky, M.
674 Stein, A. J.
675 Stein, L. C.
676 Steinert, E.
677 Steinlechner, J.
678 Steinlechner, S.
679 Steplewski, S.
680 Stochino, A.
681 Stone, R.
682 Strain, K. A.
683 Strigin, S. E.
684 Stroeer, A. S.
685 Sturani, R.
686 Stuver, A. L.
687 Summerscales, T. Z.
688 Sung, M.
689 Susmithan, S.
690 Sutton, P. J.
691 Swinkels, B.
692 Tacca, M.
693 Taffarello, L.
694 Talukder, D.
695 Tanner, D. B.
696 Tarabrin, S. P.
697 Taylor, J. R.
698 Taylor, R.
699 Thomas, P.
700 Thorne, K. A.
701 Thorne, K. S.
702 Thrane, E.
703 Thuering, A.
704 Tokmakov, K. V.
705 Tomlinson, C.
706 Toncelli, A.
707 Tonelli, M.
708 Torre, O.
709 Torres, C.
710 Torrie, C. I.
711 Tournefier, E.
712 Travasso, F.
713 Traylor, G.
714 Tseng, K.
715 Tucker, E.
716 Ugolini, D.
717 Vahlbruch, H.
718 Vajente, G.
719 van den Brand, J. F. J.
720 Van den Broeck, C.
721 van der Putten, S.
722 van Veggel, A. A.
723 Vass, S.
724 Vasuth, M.
725 Vaulin, R.
726 Vavoulidis, M.
727 Vecchio, A.
728 Vedovato, G.
729 Veitch, J.
730 Veitch, P. J.
731 Veltkamp, C.
732 Verkindt, D.
733 Vetrano, F.
734 Vicere, A.
735 Villar, A. E.
736 Vinet, J. -Y.
737 Vitale, S.
738 Vocca, H.
739 Vorvick, C.
740 Vyatchanin, S. P.
741 Wade, A.
742 Wade, L.
743 Wade, M.
744 Waldman, S. J.
745 Wallace, L.
746 Wan, Y.
747 Wang, M.
748 Wang, X.
749 Wang, Z.
750 Wanner, A.
751 Ward, R. L.
752 Was, M.
753 Weinert, M.
754 Weinstein, A. J.
755 Weiss, R.
756 Wen, L.
757 Wessels, P.
758 West, M.
759 Westphal, T.
760 Wette, K.
761 Whelan, J. T.
762 Whitcomb, S. E.
763 White, D. J.
764 Whiting, B. F.
765 Wilkinson, C.
766 Willems, P. A.
767 Williams, L.
768 Williams, R.
769 Willke, B.
770 Winkelmann, L.
771 Winkler, W.
772 Wipf, C. C.
773 Wiseman, A. G.
774 Wittel, H.
775 Woan, G.
776 Wooley, R.
777 Worden, J.
778 Yakushin, I.
779 Yamamoto, H.
780 Yamamoto, K.
781 Yancey, C. C.
782 Yang, H.
783 Yeaton-Massey, D.
784 Yoshida, S.
785 Yu, P.
786 Yvert, M.
787 Zadrozny, A.
788 Zanolin, M.
789 Zendri, J. -P.
790 Zhang, F.
791 Zhang, L.
792 Zhang, W.
793 Zhao, C.
794 Zotov, N.
795 Zucker, M. E.
796 Zweizig, J.
797 Collaboration, LIGO Sci
798 Collaboration, Virgo
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162 DAS-CEA-INPE-MCTI-GOV-BR
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162 Instituto Nacional de Pesquisas Espaciais (INPE)
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162 ccosta@phys.lsu.edu
JournalPhysical Review D
Volume85
Number12
Pages122007-1_15
Secondary MarkA2_ASTRONOMIA_/_FÍSICA B1_INTERDISCIPLINAR A2_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA
History (UTC)2012-08-23 00:46:11 :: administrator -> banon ::
2012-08-23 01:06:05 :: banon -> marciana :: 2012
2012-08-23 19:32:48 :: marciana -> banon :: 2012
2012-09-26 14:03:04 :: banon -> marciana :: 2012
2012-09-26 15:54:38 :: marciana -> banon :: 2012
2012-09-27 17:56:46 :: banon -> administrator :: 2012
2012-10-19 20:28:35 :: administrator -> marciana :: 2012
2012-12-06 16:58:41 :: marciana -> administrator :: 2012
2013-01-30 16:22:33 :: administrator -> marciana :: 2012
2013-02-04 16:29:18 :: marciana -> administrator :: 2012
2018-06-05 04:12:53 :: administrator -> marciana :: 2012
3. Content and structure
Is the master or a copy?is the master
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Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsgravitational-wave bursts
LIGO-Virgo detectors
AbstractWe present results from a search for gravitational-wave bursts in the data collected by the LIGO and Virgo detectors between July 7, 2009 and October 20, 2010: data are analyzed when at least two of the three LIGO-Virgo detectors are in coincident operation, with a total observation time of 207 days. The analysis searches for transients of duration less than or similar to 1 s over the frequency band 64-5000 Hz, without other assumptions on the signal waveform, polarization, direction or occurrence time. All identified events are consistent with the expected accidental background. We set frequentist upper limits on the rate of gravitational-wave bursts by combining this search with the previous LIGO-Virgo search on the data collected between November 2005 and October 2007. The upper limit on the rate of strong gravitational-wave bursts at the Earth is 1.3 events per year at 90\\% confidence. We also present upper limits on source rate density per year and Mpc(3) for sample populations of standard-candle sources. As in the previous joint run, typical sensitivities of the search in terms of the root-sum-squared strain amplitude for these waveforms lie in the range similar to 5 x 10(-22) Hz(-1/2) to similar to 1 x 10(-20) Hz(-1/2). The combination of the two joint runs entails the most sensitive all-sky search for generic gravitational-wave bursts and synthesizes the results achieved by the initial generation of interferometric detectors.
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Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > All-sky search for...
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