The HARP detector at the CERN PS

The HARP detector at the CERN PS
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DOI:
10.1016/j.nima.2006.08.132
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发表时间:
2007-02
影响因子:
1.4
通讯作者:
M. Catanesi;M. Muciaccia;E. Radicioni;S. Simone;R. Edgecock;M. Ellis;S. Robbins;F. Soler;C. Gössling;M. Maß;S. Bunyatov;A. Chukanov;O. Klimov;I. Krasin;A. Krasnoperov;D. Kustov;B. Popov;V. Serdiouk;V. Tereshchenko;V. Carassiti;E. Capua;F. Evangelisti;G. Vidal-Sitjes;A. Artamonov;P. Arce;R. Brocard;G. Decreuse;B. Friend;S. Giani;S. Gilardoni;P. Gorbunov;A. Grant;A. Grossheim;P. Gruber;V. Ivanchenko;J. Legrand;A. Kayis-Topaksu;J. Panman;I. Papadopoulos;J. Pasternak;E. Tcherniaev;I. Tsukerman;R. Vlugt;R. Veenhof;C. Wiebusch;P. Zucchelli;A. Blondel;S. Borghi;M. Campanelli;A. Cervera-Villanueva;M. Morone;G. Prior;R. Schroeter;I. Kato;U. Gastaldi;G. Mills;J. Graulich;G. Grégoire;M. Bonesini;F. Chignoli;F. Ferri;F. Paleari;M. Kirsanov;V. Postoev;A. Bagulya;V. Grichine;N. Polukhina;V. Palladino;L. Coney;D. Schmitz;G. Barr;A. Santo;C. Pattison;K. Zuber;G. Barichello;F. Bobisut;D. Gibin;A. Guglielmi;M. Laveder;A. Menegolli;M. Mezzetto;A. Pepato;J. Dumarchez;S. Troquereau;F. Vannucci;U. Dore;A. Iaciofano;M. Lobello;F. Marinilli;D. Orestano;D. Panayotov;M. Pasquali;F. Pastore;A. Tonazzo;L. Tortora;C. Booth;C. Buttar;P. Hodgson;L. Howlett;R. Nicholson;M. Bogomilov;K. Burin;M. Chizhov;D. Kolev;P. Petev;I. Rusinov;R. Tsenov;S. Piperov;P. Temnikov;M. Apollonio;P. Chimenti;G. Giannini;G. Santin;J. Burguet-Castell;J. Gómez-Cadenas;P. Novella;M. Sorel;A. Tornero
M. Catanesi;M. Muciaccia;E. Radicioni;S. Simone;R. Edgecock;M. Ellis;S. Robbins;F. Soler;C. Gössling;M. Maß;S. Bunyatov;A. Chukanov;O. Klimov;I. Krasin;A. Krasnoperov;D. Kustov;B. Popov;V. Serdiouk;V. Tereshchenko;V. Carassiti;E. Capua;F. Evangelisti;G. Vidal-Sitjes;A. Artamonov;P. Arce;R. Brocard;G. Decreuse;B. Friend;S. Giani;S. Gilardoni;P. Gorbunov;A. Grant;A. Grossheim;P. Gruber;V. Ivanchenko;J. Legrand;A. Kayis-Topaksu;J. Panman;I. Papadopoulos;J. Pasternak;E. Tcherniaev;I. Tsukerman;R. Vlugt;R. Veenhof;C. Wiebusch;P. Zucchelli;A. Blondel;S. Borghi;M. Campanelli;A. Cervera-Villanueva;M. Morone;G. Prior;R. Schroeter;I. Kato;U. Gastaldi;G. Mills;J. Graulich;G. Grégoire;M. Bonesini;F. Chignoli;F. Ferri;F. Paleari;M. Kirsanov;V. Postoev;A. Bagulya;V. Grichine;N. Polukhina;V. Palladino;L. Coney;D. Schmitz;G. Barr;A. Santo;C. Pattison;K. Zuber;G. Barichello;F. Bobisut;D. Gibin;A. Guglielmi;M. Laveder;A. Menegolli;M. Mezzetto;A. Pepato;J. Dumarchez;S. Troquereau;F. Vannucci;U. Dore;A. Iaciofano;M. Lobello;F. Marinilli;D. Orestano;D. Panayotov;M. Pasquali;F. Pastore;A. Tonazzo;L. Tortora;C. Booth;C. Buttar;P. Hodgson;L. Howlett;R. Nicholson;M. Bogomilov;K. Burin;M. Chizhov;D. Kolev;P. Petev;I. Rusinov;R. Tsenov;S. Piperov;P. Temnikov;M. Apollonio;P. Chimenti;G. Giannini;G. Santin;J. Burguet-Castell;J. Gómez-Cadenas;P. Novella;M. Sorel;A. Tornero
中科院分区:
物理与天体物理3区
文献类型:
--
作者:
M. Catanesi;M. Muciaccia;E. Radicioni;S. Simone;R. Edgecock;M. Ellis;S. Robbins;F. Soler;C. Gössling;M. Maß;S. Bunyatov;A. Chukanov;O. Klimov;I. Krasin;A. Krasnoperov;D. Kustov;B. Popov;V. Serdiouk;V. Tereshchenko;V. Carassiti;E. Capua;F. Evangelisti;G. Vidal-Sitjes;A. Artamonov;P. Arce;R. Brocard;G. Decreuse;B. Friend;S. Giani;S. Gilardoni;P. Gorbunov;A. Grant;A. Grossheim;P. Gruber;V. Ivanchenko;J. Legrand;A. Kayis-Topaksu;J. Panman;I. Papadopoulos;J. Pasternak;E. Tcherniaev;I. Tsukerman;R. Vlugt;R. Veenhof;C. Wiebusch;P. Zucchelli;A. Blondel;S. Borghi;M. Campanelli;A. Cervera-Villanueva;M. Morone;G. Prior;R. Schroeter;I. Kato;U. Gastaldi;G. Mills;J. Graulich;G. Grégoire;M. Bonesini;F. Chignoli;F. Ferri;F. Paleari;M. Kirsanov;V. Postoev;A. Bagulya;V. Grichine;N. Polukhina;V. Palladino;L. Coney;D. Schmitz;G. Barr;A. Santo;C. Pattison;K. Zuber;G. Barichello;F. Bobisut;D. Gibin;A. Guglielmi;M. Laveder;A. Menegolli;M. Mezzetto;A. Pepato;J. Dumarchez;S. Troquereau;F. Vannucci;U. Dore;A. Iaciofano;M. Lobello;F. Marinilli;D. Orestano;D. Panayotov;M. Pasquali;F. Pastore;A. Tonazzo;L. Tortora;C. Booth;C. Buttar;P. Hodgson;L. Howlett;R. Nicholson;M. Bogomilov;K. Burin;M. Chizhov;D. Kolev;P. Petev;I. Rusinov;R. Tsenov;S. Piperov;P. Temnikov;M. Apollonio;P. Chimenti;G. Giannini;G. Santin;J. Burguet-Castell;J. Gómez-Cadenas;P. Novella;M. Sorel;A. Tornero

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HARP是一个高统计、大立体角的实验,利用动量在1.5~15GeV/c之间的质子和π介子束撞击从低到高Z的许多不同固体和液体靶来测量强子产生。该实验位于CERN PS的T9光束中,于2001年和2002年获得数据。为了测量产生的粒子的动量和识别粒子类型,该实验包括一个基于时间投影室和电阻板室系统的大角度光谱仪,以及一个配备有一套大型漂移室、阈值切伦科夫探测器、飞行时间墙和电磁量能器的前向光谱仪。大角度系统使用螺线管磁体,而前向光谱仪基于偶极磁体。在粒子识别中的冗余度已经被寻求,以使交叉校准的效率,并获得几个百分点的总精度的横截面测量。报道了探测器的结构、运行和初步物理性能。此外,还描述了从触发器到软件框架的数据记录和分析的全链条。
HARP is a high-statistics, large solid angle experiment to measure hadron production using proton and pion beams with momenta between 1.5 and 15GeV/c impinging on many different solid and liquid targets from low to high Z. The experiment, located in the T9 beam of the CERN PS, took data in 2001 and 2002. For the measurement of momenta of produced particles and for the identification of particle types, the experiment includes a large-angle spectrometer, based on a Time Projection Chamber and a system of Resistive Plate Chambers, and a forward spectrometer equipped with a set of large drift chambers, a threshold Cherenkov detector, a time-of-flight wall and an electromagnetic calorimeter. The large angle system uses a solenoidal magnet, while the forward spectrometer is based on a dipole magnet. Redundancy in particle identification has been sought, to enable the cross-calibration of efficiencies and to obtain a few percent overall accuracy in the cross-section measurements. Detector construction, operation and initial physics performances are reported. In addition, the full chain for data recording and analysis, from trigger to the software framework, is described.