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2020-01-10
06:24
Studies of the conventional beams working group within the physics beyond colliders framework at CERN / Montbarbon, E (CERN) ; Banerjee, D (CERN ; Illinois U., Urbana) ; Bernhard, J (CERN) ; Brugger, M (CERN) ; Charitonidis, N (CERN) ; D'Alessandro, G L (CERN ; Royal Holloway, U. of London) ; Doble, N (CERN ; INFN, Pisa) ; Gatignon, L (CERN) ; Gerbershagen, A (CERN) ; Rae, B (CERN) et al.
An exploratory study has been launched at CERN in 2016 aiming at exploiting the full scientific potential of CERN’s accelerator complex and its scientific infrastructure through projects complementary to the LHC, HL-LHC and other possible future colliders. These projects will address possible experiments over the period from 2021 to about 2040. [...]
2020 - 4 p. - Published in : Nucl. Instrum. Methods Phys. Res., B 464 (2020) 1-4

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2018-09-05
06:01
Time development of hadronic showers in a Highly Granular Analog Hadron Calorimeter / Brianne, Eldwan
This thesis presents the study of the time development of hadronic showers in a highly granular hadron calorimeter using data collected by the CALICE Analog Hadron Calorimeter (AHCAL) technological prototype at the Super Proton Synchrotron (SPS) at CERN in July 2015 in μ−, e− and hadron beams u [...]
Hamburg, Germany : DESY, 2018. - 259 p.


10.3204/PUBDB-2018-02769
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2018-08-25
06:58
Double-sided 3D silicon detectors for the high-luminosity LHC / Köhler, Michael
To extend the physics potential of the Large Hadron Collider (LHC) at CERN, the European Organization for Nuclear Research, a luminosity upgrade is planned [...]
207 p.


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2018-08-15
08:13
Silicon for High-Luminosity Tracking Detectors : Recent RD50 Results / Parzefall, U (Freiburg U.) /RD50
In order to harvest the maximum physics potential of the CERN Large Hadron Collider (LHC), it is foreseen to significantly increase the LHC luminosity by upgrading the LHC towards the HL-LHC (High Luminosity LHC) [1] . Especially the final upgrade (Phase-II Upgrade) foreseen beyond 2020 will mean unprecedented radiation levels. [...]
2012 - 8 p. - Published in : Phys. Procedia 37 (2012) 899-906 Fulltext: PDF;
In : 2nd International Conference on Technology and Instrumentation in Particle Physics, Chicago, IL, USA, 9 - 14 Jun 2011, pp.899-906

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2018-06-16
06:17
Measurement of H, He, C and O Cosmic ray primaries : preliminary results from the CREAM II experiment / Mognet, Samuel
The direct measurement of the energy spectrum and composition of the incoming cosmic-ray flux at multi-TeV energies is of great interest [...]
193 p.

Penn State U. server - Full text
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2018-06-16
06:17
Exploring the Cosmic Ray Spectrum with the CREAM Experiment / Anderson, Tyler B
The Cosmic Ray Energetics and Mass (CREAM) project endeavors to resolve the cosmic-ray spectrum in an energy range between 10^{10} and 10^{15} eV for all particles with charges in the range Z = 1 (hydrogen) to Z = 26 (iron) [...]
167 p.

Penn State U. server - Full text
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2018-06-16
06:17
The CREAM-III Calorimeter / Malinin, A (Maryland U.) ; Lee, M H (Maryland U.) ; Ahn, H S (Maryland U.) ; Ganel, O (Maryland U.) ; Han, J H (Maryland U.) ; Jeon, J A (Ewha Women's U., Seoul) ; Kim, C H (Maryland U.) ; Kim, K C (Maryland U.) ; Lutz, L (Maryland U.) ; Nam, S (Ewha Women's U., Seoul) et al.
After successful recovery of the first CREAM (Cosmic Ray Energetics And Mass) instrument during the 2004\/5 Antarctic campaign, the calorimeter was refurbished for the third launch, planned for December 2007. In this CREAM-III calorimeter, the optics were replaced with multi-clad fiber ribbons to enhance the light signal. [...]
2007 - 4 p. - Published in : : 2 (2008) , pp. 409-412 Fulltext: PDF; External link: INDICO
In : 30th International Cosmic Ray Conference, Merida, Mexico, 3 - 11 Jul 2007, pp.409-412

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2018-06-16
06:17
Elemental Spectra from the CREAM-I Flight / Ahn, Hoseok ; Allison, P S ; Bagliesi, M G ; Beatty, J J ; Bigongiari, G ; Boyle, P J ; Childers, J T ; Conklin, N B ; Coutu, S ; Duvernois, M A et al.
The Cosmic Ray Energetics And Mass (CREAM) instrument is a balloon-borne experiment designed to measure the composition and energy spectra of cosmic rays of charge Z = 1 to 26 up to an energy of ∼1015 eV. CREAM had two successful flights on long-duration balloons (LDB) launched from McMurdo Station, Antarctica, in December 2004 and December 2005. [...]
2007 - 4 p. - Published in : : 2, pp. 63-66 Fulltext: PDF; External link: INDICO
In : 30th International Cosmic Ray Conference, Merida, Mexico, 3 - 11 Jul 2007, pp.63-66

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2018-06-16
06:17
Measurements of High-Energy Heavy Nuclei with the CREAM-I TRD / Wakely, Scott P (Chicago U.) ; Ahn, H S (Maryland U.) ; Allison, P S (Ohio State U.) ; Bagliesi, M G (U. Siena (main) ; INFN, Siena) ; Beatty, J J (Ohio State U.) ; Bigongiari, G (U. Siena (main) ; INFN, Siena) ; Boyle, P J (Chicago U., EFI) ; Brandt, T J (Ohio State U.) ; Childers, J T (Minnesota U.) ; Conklin, N B (Penn State U.) et al.
The balloon-borne cosmic-ray experiment CREAM-I (Cosmic-Ray Energetics And Mass) completed a successful 42-day flight during the 2004-2005 NASA\/NSF\/NSBF Antarctic expedition. CREAM-I combines an imaging calorimeter with charge detectors and a precision transition radiation detector (TRD). [...]
2007 - 4 p. - Published in : : 2, pp. 187-190 Fulltext: PDF; External link: INDICO
In : 30th International Cosmic Ray Conference, Merida, Mexico, 3 - 11 Jul 2007, pp.187-190

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2018-06-16
06:17
A New Transition Radiation Detector for the CREAM experiment / Malinin, A (Maryland U.) ; Akhnazarov, V (TRIUMF) ; Angelaszek, D (Maryland U.)
The Cosmic Ray Energetics And Mass (CREAM) experiment is designed to investigate the source, propagation and acceleration mechanism of high energy cosmic-ray nuclei, by directly measuring their energy and charge. Incorporating a Transition Radiation Detector (TRD) provides a model independent energy measurement complementary to the calorimeter, as well as additional track reconstruction capability. [...]
4 p. - Published in : 10.7529/ICRC2011/V06/1223 Fulltext: PDF;
In : 32nd International Cosmic Ray Conference, Beijing, China, 11 - 18 Aug 2011, pp.415

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