語系:
繁體中文
English
說明(常見問題)
登入
回首頁
切換:
標籤
|
MARC模式
|
ISBD
Neutrino Astrophysics with the ANTAR...
~
Kulikovskiy, Vladimir.
Neutrino Astrophysics with the ANTARES Telescope
紀錄類型:
書目-語言資料,印刷品 : Monograph/item
正題名/作者:
Neutrino Astrophysics with the ANTARES Telescope/ by Vladimir Kulikovskiy.
作者:
Kulikovskiy, Vladimir.
面頁冊數:
XIII, 119 p. 85 illus., 34 illus. in color.online resource. :
Contained By:
Springer Nature eBook
標題:
Particle acceleration. -
電子資源:
https://doi.org/10.1007/978-3-319-20412-3
ISBN:
9783319204123
Neutrino Astrophysics with the ANTARES Telescope
Kulikovskiy, Vladimir.
Neutrino Astrophysics with the ANTARES Telescope
[electronic resource] /by Vladimir Kulikovskiy. - 1st ed. 2015. - XIII, 119 p. 85 illus., 34 illus. in color.online resource. - Springer Theses, Recognizing Outstanding Ph.D. Research,2190-5053. - Springer Theses, Recognizing Outstanding Ph.D. Research,.
Introduction -- The ANTARES Detector -- Simulation of the ANTARES Detector Work -- Event Reconstruction and Data Selection -- Fermi Bubbles Analysis -- Conclusions.
This thesis is devoted to ANTARES, the first underwater neutrino telescope in the Mediterranean sea. As the main scientific analysis, a search for high-energy neutrino emission from the region of the Fermi bubbles has been performed using data from the ANTARES detector. A method for the background estimation using off-zones has been developed specially for this measurement. A new likelihood for the limits calculation which treats both observations in the on-zone and in the off-zone in the similar way and also includes different systematic uncertainties has been constructed. The analysis of 2008–2011 ANTARES data yielded a 1.2 σ excess of events in the Fermi bubble regions, compatible with the no-signal hypothesis. For the optimistic case of no energy cutoff in the flux, the upper limit is within a factor of three of the prediction of the purely hadronic model based on the measured gamma-ray flux. The sensitivity improves as more data are accumulated (more than 65% gain in the sensitivity is expected once 2012–2016 data are added to the analysis).
ISBN: 9783319204123
Standard No.: 10.1007/978-3-319-20412-3doiSubjects--Topical Terms:
681844
Particle acceleration.
LC Class. No.: QC770-798
Dewey Class. No.: 539.73
Neutrino Astrophysics with the ANTARES Telescope
LDR
:02672nam a22004095i 4500
001
968585
003
DE-He213
005
20200706103824.0
007
cr nn 008mamaa
008
201211s2015 gw | s |||| 0|eng d
020
$a
9783319204123
$9
978-3-319-20412-3
024
7
$a
10.1007/978-3-319-20412-3
$2
doi
035
$a
978-3-319-20412-3
050
4
$a
QC770-798
072
7
$a
PHP
$2
bicssc
072
7
$a
SCI051000
$2
bisacsh
072
7
$a
PHP
$2
thema
082
0 4
$a
539.73
$2
23
100
1
$a
Kulikovskiy, Vladimir.
$e
author.
$4
aut
$4
http://id.loc.gov/vocabulary/relators/aut
$3
1264195
245
1 0
$a
Neutrino Astrophysics with the ANTARES Telescope
$h
[electronic resource] /
$c
by Vladimir Kulikovskiy.
250
$a
1st ed. 2015.
264
1
$a
Cham :
$b
Springer International Publishing :
$b
Imprint: Springer,
$c
2015.
300
$a
XIII, 119 p. 85 illus., 34 illus. in color.
$b
online resource.
336
$a
text
$b
txt
$2
rdacontent
337
$a
computer
$b
c
$2
rdamedia
338
$a
online resource
$b
cr
$2
rdacarrier
347
$a
text file
$b
PDF
$2
rda
490
1
$a
Springer Theses, Recognizing Outstanding Ph.D. Research,
$x
2190-5053
505
0
$a
Introduction -- The ANTARES Detector -- Simulation of the ANTARES Detector Work -- Event Reconstruction and Data Selection -- Fermi Bubbles Analysis -- Conclusions.
520
$a
This thesis is devoted to ANTARES, the first underwater neutrino telescope in the Mediterranean sea. As the main scientific analysis, a search for high-energy neutrino emission from the region of the Fermi bubbles has been performed using data from the ANTARES detector. A method for the background estimation using off-zones has been developed specially for this measurement. A new likelihood for the limits calculation which treats both observations in the on-zone and in the off-zone in the similar way and also includes different systematic uncertainties has been constructed. The analysis of 2008–2011 ANTARES data yielded a 1.2 σ excess of events in the Fermi bubble regions, compatible with the no-signal hypothesis. For the optimistic case of no energy cutoff in the flux, the upper limit is within a factor of three of the prediction of the purely hadronic model based on the measured gamma-ray flux. The sensitivity improves as more data are accumulated (more than 65% gain in the sensitivity is expected once 2012–2016 data are added to the analysis).
650
0
$a
Particle acceleration.
$3
681844
650
0
$a
Astrophysics.
$3
646223
650
0
$a
Physical measurements.
$3
902742
650
0
$a
Measurement .
$3
1253766
650
1 4
$a
Particle Acceleration and Detection, Beam Physics.
$3
671851
650
2 4
$a
Astrophysics and Astroparticles.
$3
782546
650
2 4
$a
Measurement Science and Instrumentation.
$3
769080
710
2
$a
SpringerLink (Online service)
$3
593884
773
0
$t
Springer Nature eBook
776
0 8
$i
Printed edition:
$z
9783319204130
776
0 8
$i
Printed edition:
$z
9783319204116
776
0 8
$i
Printed edition:
$z
9783319387154
830
0
$a
Springer Theses, Recognizing Outstanding Ph.D. Research,
$x
2190-5053
$3
1253569
856
4 0
$u
https://doi.org/10.1007/978-3-319-20412-3
912
$a
ZDB-2-PHA
912
$a
ZDB-2-SXP
950
$a
Physics and Astronomy (SpringerNature-11651)
950
$a
Physics and Astronomy (R0) (SpringerNature-43715)
筆 0 讀者評論
多媒體
評論
新增評論
分享你的心得
Export
取書館別
處理中
...
變更密碼[密碼必須為2種組合(英文和數字)及長度為10碼以上]
登入