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Related papers: Underground Muon Physics with the MACRO experiment

200 papers

We present first results about the measurement of the characteristics of charged hadrons production by atmospheric muons in the rock above MACRO. Selection criteria which allow to discriminate hadron cascades from e.m. showers generated by…

High Energy Physics - Experiment · Physics 2007-05-23 G. Battistoni

Using a sample of 38.5 million underground muons collected by the MACRO detector we have performed an all-sky search for pointlike sources producing excesses of muons above the expected background. The d.c. muon flux upper limit at the…

High Energy Physics - Experiment · Physics 2019-08-14 C. Satriano

The flux of low energy atmospheric neutrinos (E_nu ~ 4 GeV) has been studied with the MACRO detector at Gran Sasso by detecting nu_mu interactions inside the apparatus, and by upward-going stopping muons. The updated analysis of the data…

High Energy Physics - Experiment · Physics 2019-08-14 A. Surdo

The MACRO detector is located in the Gran Sasso Laboratory. MACRO's overburden varies from 3150 to 7000 hg/cm^2. A transition radiation detector (TRD) has been added to the MACRO detector in order to measure the residual energy of muons…

High Energy Physics - Experiment · Physics 2019-08-14 M. N. Mazziotta

We present updated results of the measurement of upward-going muons produced by neutrino interactions in the rock below the MACRO detector. These data support MACRO's previously published results. They favor a neutrino oscillation…

High Energy Physics - Experiment · Physics 2007-05-23 F. Ronga

We present the result of a search for correlations in the arrival times of high energy muons collected from 1995 till 2000 with the streamer tube system of the complete MACRO detector at the underground Gran Sasso Lab. Large samples of…

A measurement of the flux of neutrino-induced muons using the MACRO detector is presented. Different event topologies, corresponding to different neutrino parent energies can be detected. The upward throughgoing muon sample is the larger…

High Energy Physics - Experiment · Physics 2008-11-26 F. Ronga

The flux of neutrino-induced muons has been measured with the MACRO detector. Different event topologies have been detected, due to neutrino interactions in the apparatus and in the rock below it. The upward-throughgoing muon sample is the…

High Energy Physics - Experiment · Physics 2007-05-23 Paolo Bernardini

We present first results about the measurement of the charged hadrons production by atmopsheric muons in the rock above MACRO. A comparison between the measurerate with the Monte Carlo expectation is presented.

High Energy Physics - Experiment · Physics 2019-08-14 E. Scapparone

We present a review of atmospheric and underground muon flux measurements. The relevance of these data for the atmospheric neutrino flux computation is emphasized. Possible sources of systematic errors in the measurements are discussed,…

High Energy Physics - Experiment · Physics 2007-05-23 S. Cecchini , M. Sioli

High-energy cosmic rays are observed indirectly by detecting the extensive air showers initiated in Earth's atmosphere. The interpretation of experimental data relies on accurate modeling of the air shower development. Simulations based on…

High Energy Astrophysical Phenomena · Physics 2025-09-23 Lilly Pyras , Dennis Soldin , Felix Riehn

The flux of muons induced by atmospheric neutrinos has been measured with the MACRO detector. Different event topologies have been detected, due to neutrino interactions in the apparatus and in the rock below it. The upward-throughgoing…

High Energy Physics - Experiment · Physics 2007-05-23 Paolo Bernardini

We present first results about the measurement of the charged hadrons production by atmopsheric muons in the rock above MACRO. A comparison between the measure rate with the Monte Carlo expectation is presented

High Energy Physics - Experiment · Physics 2019-08-14 E. Scapparone

A dedicated cosmic muon Monte-Carlo event generator CMSCGEN has been developed for the CMS experiment. The simulation relies on parameterisations of the muon energy and the incidence angle, based on measured and simulated data of the cosmic…

High Energy Physics - Experiment · Physics 2011-07-05 Lars Sonnenschein

We have measured directly the residual energy of cosmic ray muons crossing the MACRO detector at the Gran Sasso Laboratory. For this measurement we have used a transition radiation detector consisting of three identical modules, each of…

High Energy Physics - Experiment · Physics 2008-11-26 The MACRO Collaboration , M. Ambrosio et al

We present a review of atmospheric muon flux and energy spectrum measurements over almost six decades of muon momentum. Sea-level and underground/water/ice experiments are considered. Possible sources of systematic errors in the…

Earth and Planetary Astrophysics · Physics 2012-08-16 Stefano Cecchini , Maurizio Spurio

The muon intensity attenuation method to detect heterogeneities in large matter volumes is analyzed. Approximate analytical expressions to estimate the collection time and the signal to noise ratio, are proposed and validated by Monte Carlo…

Instrumentation and Detectors · Physics 2008-11-26 V. Grabski , R. Reche , R. Alfaro , E. Belmont , A. Martinez , A. Sandoval , A. Menchaca-Rocha

The paper describes two Monte Carlo codes dedicated to muon simulations: MUSIC (MUon SImulation Code) and MUSUN (MUon Simulations UNderground). MUSIC is a package for muon transport through matter. It is particularly useful for propagating…

Computational Physics · Physics 2009-11-13 V. A. Kudryavtsev

A search for aligned events has been done throughout the muon group events measured with Baksan Underground Scintillation Telescope (BUST) during a long period of time. Only groups of multiplicity >3 for muon threshold energies equal to…

Astrophysics · Physics 2007-05-23 A. L. Tsyabuk , R. A. Mukhamedshin , Yu. V. Stenkin

Background induced by neutrons in deep underground laboratories is a critical issue for all experiments looking for rare events, such as dark matter interactions or neutrinoless 2-beta decay. Neutrons can be produced either by natural…

Astrophysics · Physics 2009-06-23 V. A. Kudryavtsev , L. Pandola , V. Tomasello