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CERN Accelerating science

CERN Document Server Znaleziono 2,031 rekordów  1 - 10następnykoniec  skocz do rekordu: Szukanie trwało 0.28 sekund. 
1.
Signals for invisible matter from solar-terrestrial observations / Bertolucci, Sergio (CERN ; Frascati) ; Zioutas, Konstantin (CERN ; Patras U.) ; Hofmann, Sebastian (Unlisted, DE) ; Maroudas, Marios (Patras U.)
Gravitational lensing of invisible streaming matter towards the Sun or the Earth could be the explanation of puzzling solar/terrestrial phenomena. We have analyzed solar flares, EUV emission and also the global ionization content of the Earth atmosphere. [...]
2017 - 8 p. - Published in : EPJ Web Conf. 164 (2017) 07041 Fulltext: PDF;
In : 5th International Conference on New Frontiers in Physics, Kolymbari, Greece, 6 - 14 Jul 2016, pp.07041
2.
Signals for invisible matter from solar - terrestrial observations / Bertolucci, Sergio (CERN ; INFN, Italy) ; Zioutas, Konstantin (CERN ; Patras U.) ; Hofmann, Sebastian (Unlisted, DE) ; Maroudas, Marios (Patras U.)
Gravitational lensing of invisible streaming matter towards the Sun or the Earth could be the explanation of puzzling solar/terrestrial phenomena. We have analyzed solar flares, EUV emission and also the global ionization content of the Earth atmosphere. [...]
2017 - 7 p. - Published in : 10.3204/DESY-PROC-2009-03/Zioutas_Konstantin Fulltext: PDF;
In : 12th Patras Workshop on Axions, WIMPs and WISPs, Jeju Island, South Korea, 20 - 24 Jun 2016, pp.168-174
3.
Signals for invisible matter from solar-terrestrial observations / Zioutas, Konstantin (speaker) (University of Patras (GR))
We observe a strong correlation between the orbital position of the planets with solar phenomena like flares or the variation of EUV irradiance. Similarly, a correlation is found in the study of the ionization content of the Earth atmosphere. [...]
2016 - 5376. EP Seminar External link: Event details In : Signals for invisible matter from solar-terrestrial observations
4.
The Sun and its Planets as detector for invisible matter / Bertolucci, Sergio (CERN ; LNF, Dafne Light) ; Zioutas, Konstantin (CERN ; Patras U.) ; Hofmann, Sebastian ; Maroudas, Marios (Patras U.)
Gravitational lensing of invisible streaming matter towards the Sun could be the explanation of the puzzling solar flares and the unexplained solar emission in the EUV. Assuming that this invisible matter has some form of interaction with normal matter and that there exist preferred directions in its flow, then one would expect a more pronounced solar activity at certain planetary heliocentric longitudes. [...]
arXiv:1602.03666.- 2017 - 18 p. - Published in : Phys. Dark Universe 17 (2017) 13-21 Fulltext: 1-s2.0-S2212686417300365-main - PDF; arXiv:1602.03666 - PDF; 10.1016_j.dark.2017.06.001 - PDF; External link: Preprint
5.
On the Direct Detection of Dark Matter in the Stratosphere / Cantatore, Giovanni (INFN, Trieste ; Trieste U.) ; Çetin, Serkant A. (Koc U.) ; Fischer, Horst (Freiburg U.) ; Funk, Wolfgang (CERN) ; Karuza, Marin (Rijeka U. ; INFN, Trieste) ; Kryemadhi, Abaz (Messiah Coll.) ; Maroudas, Marios (Patras U.) ; Özbozduman, Kaan (Bogazici U.) ; Semertzidis, Yannis K. (IBS, Daejeon) ; Zioutas, Konstantin (Patras U.)
We investigate the prospects for direct detection of Dark Matter (DM) particles, such as dark photons, incident on the upper atmosphere. A recent work relates the burst-like temperature excursions in the stratosphere at heights of ~38-47 km with incident invisible streaming matter. [...]
arXiv:2012.03353.- 2023-05-29 - 10 p. - Published in : Symmetry 15 (2023) 1167 Fulltext: 2012.03353 - PDF; Publication - PDF;
6.
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
7.
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
8.
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
9.
Recent results from the LHCf experiment / Tiberio, A (Florence U. ; INFN, Florence) ; Adriani, O (Florence U. ; INFN, Florence) ; Berti, E (Florence U. ; INFN, Florence) ; Bonechi, L (INFN, Florence) ; Bongi, M (Florence U. ; INFN, Florence) ; Castellini, G (INFN, Florence ; IFAC, Florence) ; D'Alessandro, R (Florence U. ; INFN, Florence) ; Del Prete, M (Florence U. ; INFN, Florence) ; Haguenauer, M (Ecole Polytechnique) ; Itow, Y (Nagoya U., Solar-Terrestrial Environ. Lab. ; KMI, Nagoya) et al.
The LHC-forward (LHCf) experiment, situated at the LHC accelerator, has measured neutral particles production in a very forward region (pseudo-rapidity > 8.4) in proton-proton and proton-lead collisions. The main purpose of the LHCf experiment is to test hadronic interaction models used in cosmic rays experiments to imulate cosmic rays induced air-showers in Earth's atmosphere..
2015 - 5 p. - Published in : EPJ Web Conf. 96 (2015) 01031 EDP Sciences Open Access article: PDF;
In : Dark Matter, Hadron Physics and Fusion Physics, Messina, Italy, 24 - 26 Sep 2014, pp.01031
10.
Latest LHCf results and preparation to the LHC run for 13 TeV proton–proton interactions / Bonechi, L (INFN, Florence) ; Adriani, O (INFN, Florence ; Florence U.) ; Berti, E (Florence U.) ; Bongi, M (INFN, Florence ; Florence U.) ; Castellini, G (IFAC, Florence) ; D'Alessandro, R (INFN, Florence ; Florence U.) ; Del Prete, M (INFN, Florence ; Florence U.) ; Haguenauer, M (Unlisted, FR) ; Itow, Y (Nagoya U., Solar-Terrestrial Environ. Lab. ; KMI, Nagoya) ; Kasahara, K (Waseda U., RISE) et al.
The LHCf experiment is a CERN experiment dedicated to forward physics which is optimized to measure the neutral particle flow at extreme pseudo-rapidity values, ranging from 8.4 up to infinity. LHCf results are extremely important for the calibration of the hadronic interaction models used for the study of the development of atmospheric showers in the Earth atmosphere. [...]
2015 - 7 p. - Published in : EPJ Web Conf. 95 (2015) 04010 EDP Sciences Open Access article: PDF;
In : 3rd International Conference on New Frontiers in Physics, Kolymbari, Crete, Greece, 28 Jul - 06 Aug 2014, pp.04010

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