CERN Accelerating science

CERN Document Server 2,050 záznamov nájdených  1 - 10ďalšíkoniec  skoč na záznam: Hľadanie trvalo 0.45 sekúnd. 
1.
Search for streaming dark matter axions or other exotica / Gardikiotis, A. (Patras U.) ; Anastassopoulos, V. (Patras U.) ; Bertolucci, S. (INFN, Bologna ; LNF, Dafne Light) ; Cantatore, G. (INFN, Trieste ; Trieste U.) ; Cetin, S. (Istanbul Bilgi U.) ; Fischer, H. (Freiburg U.) ; Funk, W. (CERN) ; Hoffmann, D.H.H. (Xian Jiaotong U.) ; Hofmann, S. (Munich U. ; Frankfurt U.) ; Karuza, M. (INFN, Trieste ; Rijeka U.) et al.
We suggest a new approach to search for galactic axions or other similar exotica. [...]
arXiv:1803.08588.
- 2018. - 4 p.
Full text
2.
Search for streaming dark matter axions or other exotica / Gardikiotis, A (Patras U.) ; Anastassopoulos, V (Patras U.) ; Bertolucci, S (INFN, Bologna) ; Cantatore, G (U. Trieste (main) ; INFN, Trieste) ; Cetin, S (Istanbul Bilgi U.) ; Fischer, H (Freiburg U.) ; Funk, W (CERN) ; Hoffmann, D H H (XJTLU, Suzhou ; Moscow Phys. Eng. Inst.) ; Hofmann, S (Unlisted, DE) ; Karuza, M (Rijeka U. ; INFN, Trieste) et al.
We suggest a new approach to search for galactic axions or other similar exotica. Streaming dark matter (DM) could have a better discovery potential because of flux enhancement, due to gravitational lensing when the Sun and/or a planet are aligned with a DM stream [1]. [...]
DESY-PROC-2017-02.- 2018 - 4 p. - Published in : 10.3204/DESY-PROC-2017-02/gardikiotis_antonios Fulltext: PDF;
In : 13th Patras Workshop on Axions, WIMPs and WISPs - Axion-WIMP 2017, Thessaloniki, Greece, 13 - 19 May 2017, pp.19-22
3.
Search for axions in streaming dark matter / Zioutas, K. (CERN ; Patras U.) ; Anastassopoulos, V. (Patras U.) ; Bertolucci, S. (INFN, Bologna) ; Cantatore, G. (INFN, Trieste ; Trieste U.) ; Cetin, S.A. (Bogazici U.) ; Fischer, H. (Freiburg U.) ; Funk, W. (CERN) ; Gardikiotis, A. (Patras U.) ; Hoffmann, D.H. H. (Darmstadt, Tech. U.) ; Hofmann, S. (Unlisted, DE) et al.
A new search strategy for the detection of the elusive dark matter (DM) axion is proposed. [...]
arXiv:1703.01436.
- 2017. - 5 p.
Full text
4.
New CAST Limit on the Axion-Photon Interaction / CAST Collaboration
During 2003--2015, the CERN Axion Solar Telescope (CAST) has searched for $a\to\gamma$ conversion in the 9 T magnetic field of a refurbished LHC test magnet that can be directed toward the Sun. In its final phase of solar axion searches (2013--2015), CAST has returned to evacuated magnet pipes, which is optimal for small axion masses. [...]
arXiv:1705.02290.- 2017-05-01 - 8 p. - Published in : Nature Phys. 13 (2017) 584-590 Fulltext: arXiv:1705.02290 - PDF; nphys4109 - PDF; External links: Nature Phys.; Fulltext
5.
aKWISP: investigating short-distance interactions at sub-micron scales / Cantatore, G. (INFN, Trieste ; Trieste U.) ; Anastassopoulos, V. (Patras U.) ; Cetin, S. (Istanbul Bilgi U.) ; Fischer, H. (Freiburg U.) ; Funk, W. (CERN) ; Gardikiotis, A. (Patras U.) ; Hoffmann, D.H.H. (Darmstadt, Tech. U.) ; Karuza, M. (INFN, Trieste ; Trieste U. ; Rijeka U.) ; Semertzidis, Y.K. (IBS, Daejeon) ; Vitali, D. (Camerino U.) et al.
The sub-micron range in the field of short distance interactions has yet to be opened to experimental investigation, and may well hold the key to understanding al least part of the dark matter puzzle. The aKWISP (advanced-KWISP) project introduces the novel Double Membrane Interaction Monitor (DMIM), a combined source-sensing device where interaction distances can be as short as 100 nm or even 10 nm, much below the 1-10 micron distance which is the lower limit encountered by current experimental efforts. [...]
arXiv:1803.07685.- 2018 - 4 p. - Published in : 10.3204/DESY-PROC-2017-02/cantatore_giovanni Fulltext: 1803.07685 - PDF; fulltext - PDF;
In : 13th Patras Workshop on Axions, WIMPs and WISPs - Axion-WIMP 2017, Thessaloniki, Greece, 13 - 19 May 2017, pp.200-203
6.
Improved Search for Solar Chameleons with a GridPix Detector at CAST / CAST Collaboration
We report on a new search for solar chameleons with the CERN Axion Solar Telescope (CAST). A GridPix detector was used to search for soft X-ray photons in the energy range from 200 eV to 10 keV from converted solar chameleons. [...]
arXiv:1808.00066.- 2019-01-16 - 19 p. - Published in : JCAP 1901 (2019) 032 Fulltext: PDF; Fulltext from Publisher: PDF;
7.
New Upper Limit on the Axion-Photon Coupling with an Extended CAST Run with a Xe-Based Micromegas Detector / CAST Collaboration
Hypothetical axions provide a compelling explanation for dark matter and could be emitted from the hot solar interior. The CERN Axion Solar Telescope (CAST) has been searching for solar axions via their back conversion to X-ray photons in a 9-T 10-m long magnet directed towards the Sun. [...]
arXiv:2406.16840.- 2024-11-27 - 9 p. - Published in : Phys. Rev. Lett. 133 (2024) 221005 Fulltext: Publication - PDF; 2406.16840 - PDF;
8.
First results of the CAST-RADES haloscope search for axions at 34.67 $\mu$eV / CAST Collaboration
We present results of the Relic Axion Dark-Matter Exploratory Setup (RADES), a detector which is part of the CERN Axion Solar Telescope (CAST), searching for axion dark matter in the 34.67$\mu$eV mass range. A radio frequency cavity consisting of 5 sub-cavities coupled by inductive irises took physics data inside the CAST dipole magnet for the first time using this filter-like haloscope geometry. [...]
arXiv:2104.13798; CERN-EP-2021-070.- 2021 - 14 p. - Published in : JHEP 2021 (2021) 075 Fulltext: PDF;
9.
First Results on the Search for Chameleons with the KWISP Detector at CAST / Arguedas Cuendis, S. (CERN) ; Baier, J. (Freiburg U.) ; Barth, K. (CERN) ; Baum, S. (Royal Inst. Tech., Stockholm ; Stockholm U., OKC ; Nordita) ; Bayirli, A. (Istanbul U.) ; Belov, A. (Moscow, INR) ; Bräuninger, H. (Garching, Max Planck Inst., MPE) ; Cantatore, G. (INFN, Trieste ; Trieste U.) ; Carmona, J.M. (Zaragoza U.) ; Castel, J.F. (Zaragoza U.) et al.
We report on a first measurement with a sensitive opto-mechanical force sensor designed for the direct detection of coupling of real chameleons to matter. These dark energy candidates could be produced in the Sun and stream unimpeded to Earth. [...]
arXiv:1906.01084.- 2019-12 - 21 p. - Published in : Phys. Dark Univ. 26 (2019) 100367 Fulltext: 1-s2.0-S2212686419301517-main - PDF; 1906.01084 - PDF; Fulltext from Publisher: PDF;
10.
Search for chameleons with CAST / CAST Collaboration
In this work we present a search for (solar) chameleons with the CERN Axion Solar Telescope (CAST). This novel experimental technique, in the field of dark energy research, exploits both the chameleon coupling to matter ($\beta_{\rm m}$) and to photons ($\beta_{\gamma}$) via the Primakoff effect. [...]
arXiv:1503.04561.- 2015-07-24 - 9 p. - Published in : Phys. Lett. B 749 (2015) 172-180 Article from SCOAP3: PDF; Fulltext: PDF; External link: Preprint

Nenašli ste čo ste hľadali? Skúste Vašu otázku na iných serveroch:
recid:2312304 v Amazon
recid:2312304 v CERN EDMS
recid:2312304 v CERN Intranet
recid:2312304 v CiteSeer
recid:2312304 v Google Books
recid:2312304 v Google Scholar
recid:2312304 v Google Web
recid:2312304 v IEC
recid:2312304 v IHS
recid:2312304 v INSPIRE
recid:2312304 v ISO
recid:2312304 v KISS Books/Journals
recid:2312304 v KISS Preprints
recid:2312304 v NEBIS
recid:2312304 v SLAC Library Catalog