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The goal of the ASACUSA (Atomic Spectroscopy And Collisions Using Slow Antiprotons) CUSP experiment at CERN's Antiproton Decelerator is to measure the ground state hyperfine splitting of antihydrogen in order to test whether CPT invariance…

Radiation damage significantly impacts the performance of silicon tracking detectors in Large Hadron Collider (LHC) experiments such as ATLAS and CMS, with signal reduction being the most critical effect. Adjusting sensor bias voltage and…

High Energy Physics - Experiment · Physics 2025-01-22 Marco Bomben , Keerthi Nakkalil

Radiation damage significantly impacts the performance of silicon tracking detectors in Large Hadron Collider (LHC) experiments such as ATLAS and CMS, with signal reduction being the most critical effect; adjusting sensor bias voltage and…

High Energy Physics - Experiment · Physics 2025-01-22 Keerthi Nakkalil , Marco Bomben

The goal of the ASACUSA-CUSP collaboration at the Antiproton Decelerator of CERN is to measure the ground-state hyperfine splitting of antihydrogen using an atomic spectroscopy beamline. A milestone was achieved in 2012 through the…

Light antinuclei, like antideuteron and antihelium-3, are ideal probes for new, exotic physics because their astrophysical backgrounds are suppressed at low energies. In order to exploit fully the inherent discovery potential of light…

High Energy Physics - Phenomenology · Physics 2023-03-22 M. Kachelriess , S. Ostapchenko , J. Tjemsland

An accurate evaluation of the gravity acceleration from the timing of free fall of anti-hydrogen atoms in the GBAR experiment requires to account for obstacles surrounding the anti-matter source. These obstacles reduce the number of useful…

With the tenfold luminosity increase envisaged at the HL-LHC, the background (photons, neutrons, ...) and the event pile-up probability are expected to increase in proportion in the different experiments, especially in the forward regions…

We investigate in this paper the antideuteron flux produced in high energy collisions of cosmic rays with the interstellar matter. We employ the Monte Carlo generator DPMJET-III together with the coalescence model to simulate, in an…

High Energy Astrophysical Phenomena · Physics 2013-08-09 Alejandro Ibarra , Sebastian Wild

Traditional cosmic ray simulations make use of the Montecarlo method in a very naive way to randomise energy and direction for each simulated particle. The flux of cosmic rays is modelled as a rain coming from a plane above the object of…

High Energy Physics - Experiment · Physics 2025-09-19 David Díez Ibáñez , Luis Obis Aparicio

The ASACUSA (Atomic Spectroscopy And Collisions Using Slow Antiprotons) collaboration at the Antiproton Decelerator at CERN aims to measure the ground state hyperfine structure of antihydrogen. A Rabi-like spectrometer line has been built…

Instrumentation and Detectors · Physics 2016-09-07 Bernadette Kolbinger

An accelerator experiment was performed using a low-energy antiproton beam to measure antiproton detection efficiency of BESS, a balloon-borne spectrometer with a superconducting solenoid. Measured efficiencies showed good agreement with…

An estimate of environmental background hit rate on triple-GEM chambers is performed using Monte Carlo (MC) simulation and compared to data taken by test chambers installed in the CMS experiment (GE1/1) during Run-2 at the Large Hadron…

Instrumentation and Detectors · Physics 2022-01-05 M. Abbas , M. Abbrescia , H. Abdalla , A. Abdelalim , S. AbuZeid , A. Agapitos , A. Ahmad , A. Ahmed , W. Ahmed , C. Aimè , C. Aruta , I. Asghar , P. Aspell , C. Avila , I. Azhgirey , J. Babbar , Y. Ban , R. Band , S. Bansal , L. Benussi , V. Bhatnagar , M. Bianco , S. Bianco , K. Black , L. Borgonovi , O. Bouhali , A. Braghieri , S. Braibant , S. Butalla , S. Calzaferri , M. Caponero , F. Cassese , A. Castaneda , N. Cavallo , S. S. Chauhan , A. Colaleo , A. Conde Garcia , M. Dalchenko , A. De Iorio , G. De Lentdecker , D. Dell Olio , G. De Robertis , W. Dharmaratna , S. Dildick , B. Dorney , R. Erbacher , F. Fabozzi , F. Fallavollita , A. Ferraro , D. Fiorina , E. Fontanesi , M. Franco , C. Galloni , P. Giacomelli , S. Gigli , J. Gilmore , M. Gola , M. Gruchala , A. Gutierrez , R. Hadjiiska , T. Hakkarainen , J. Hauser , K. Hoepfner , M. Hohlmann , H. Hoorani , T. Huang , P. Iaydjiev , A. Irshad , A. Iorio , F. Ivone , J. Jaramillo , V. Jha , A. Juodagalvis , E. Juska , B. Kailasapathy , T. Kamon , Y. Kang , P. Karchin , A. Kaur , H. Kaur , H. Keller , H. Kim , J. Kim , S. Kim , B. Ko , A. Kumar , S. Kumar , H. Kumawat , N. Lacalamita , J. S. H. Lee , A. Levin , Q. Li , F. Licciulli , L. Lista , K. Liyanage , F. Loddo , M. Luhach , M. Maggi , Y. Maghrbi , N. Majumdar , K. Malagalage , S. Malhotra , S. Mallows , S. Martiradonna , N. Mccoll , C. McLean , J. Merlin , M. Misheva , D. Mishra , G. Mocellin , L. Moureaux , A. Muhammad , S. Muhammad , S. Mukhopadhyay , M. Naimuddin , P. Netrakanti , S. Nuzzo , R. Oliveira , L. Pant , P. Paolucci , I. C. Park , L. Passamonti , G. Passeggio , A. Peck , A. Pellecchia , N. Perera , L. Petre , H. Petrow , D. Piccolo , D. Pierluigi , G. Raffone , M. Rahmani , F. Ramirez , A. Ranieri , G. Rashevski , B. Regnery , M. Ressegotti , C. Riccardi , M. Rodozov , E. Romano , C. Roskas , B. Rossi , P. Rout , D. Roy , J. D. Ruiz , A. Russo , A. Safonov , A. K. Sahota , D. Saltzberg , G. Saviano , A. Shah , A. Sharma , R. Sharma , T. Sheokand , M. Shopova , F. Simone , J. Singh , U. Sonnadara , E. Starling , B. Stone , J. Sturdy , G. Sultanov , Z. Szillasi , D. Teague , D. Teyssier , T. Tuuva , M. Tytgat , I. Vai , N. Vanegas , R. Venditti , P. Verwilligen , W. Vetens , A. K. Virdi , P. Vitulo , A. Wajid , D. Wang , K. Wang , I. J. Watson , N. Wickramage , W. Jang , D. D. C. Wickramarathna , S. Yang , Y. Yang , U. Yang , J. Yongho , I. Yoon , Z. You , I. Yu , S. Zaleski

A new Monte Carlo program for photohadronic interactions of relativistic nucleons with an ambient photon radiation field is presented. The event generator is designed to fulfil typical astrophysical requirements, but can also be used for…

Astrophysics · Physics 2011-05-05 A. Muecke , Ralph Engel , J. P. Rachen , R. J. Protheroe , Todor Stanev

Recent detections of cosmic microwave background (CMB) anisotropy at half-degree angular scales show considerable scatter in the reported amplitude even at similar angular resolution. We use Monte Carlo techniques to simulate the current…

Astrophysics · Physics 2007-05-23 A. Kogut , G. Hinshaw

We present the commissioning of the Fast Annihilation Cryogenic Tracker detector (FACT), installed around the antihydrogen production trap inside the 1 T superconducting magnet of the AE\=gIS experiment. FACT is designed to detect pions…

The radio technique for the detection of cosmic particles has seen a major revival in recent years. New and planned experiments in the lab and the field, such as GLUE, Anita, LUNASKA, Codalema, LOPES as well as sophisticated Monte Carlo…

Astrophysics · Physics 2019-08-15 Heino Falcke

The limited statistics of the available (anti)neutrino-hydrogen (H) interactions has been a longstanding impediment for high-energy neutrino physics. We discuss a practical way to achieve accurate (anti)neutrino-hydrogen measurements,…

High Energy Physics - Phenomenology · Physics 2024-12-31 H. Duyang , B. Guo , S. R. Mishra , R. Petti

High-purity germanium detectors are well suited to analysis the radioactivity of samples. In order to reduce the environmental background, low-activity lead and oxygen free copper are installed outside of the probe to shield gammas, outmost…

We explore the application of Monte Carlo transport methods to solving coupled radiation-hydrodynamics problems. We use a time-dependent, frequency-dependent, 3-dimensional radiation transport code, that is special relativistic and includes…

Instrumentation and Methods for Astrophysics · Physics 2015-06-19 Nathaniel Roth , Daniel Kasen
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