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Related papers: High energy leptons from muons in transit

200 papers

We calculate the muon flux from annihilation of the dark matter in the core of the Sun, in the core of the Earth and from cosmic diffuse neutrinos produced in dark matter annihilation in the halos. We consider model-independent direct…

High Energy Physics - Phenomenology · Physics 2009-09-02 Arif Emre Erkoca , Mary Hall Reno , Ina Sarcevic

We present the results of (anti)neutrino induced CCQE cross sections from some nuclear targets in the energy region of $E_\nu \le 1 GeV$. The aim of the study is to confront electron and muon production cross sections relevant for $\nu_\mu…

Nuclear Theory · Physics 2016-11-23 M. Sajjad Athar , F. Akbar , M. Rafi Alam , S. Chauhan , S. K. Singh , F. Zaidi

We evaluate neutrino-nucleon cross section for energies up to $10^{21} eV$ in light of new information on the small-$x$ behavior of parton distributions. We give predictions for large underground neutrino telescope event rates for…

High Energy Physics - Phenomenology · Physics 2007-05-23 Raj Gandhi , Chris Quigg , M. H. Reno , Ina Sarcevic

Measurements of the production of events containing isolated high energy leptons (electrons and muons) produced in ep collisions have been performed with the H1 and ZEUS detectors at HERA, using data collected in the period 1994-2007.…

High Energy Physics - Experiment · Physics 2014-11-20 David M. South

We explore the low energy neutrinos from stopped cosmic ray muons in the Earth. Based on the muon intensity at the sea level and the muon energy loss rate, the depth distributions of stopped muons in the rock and sea water can be derived.…

High Energy Physics - Phenomenology · Physics 2019-05-01 Wan-Lei Guo

Cross sections for the production of two isolated muons up to high di-muon masses are measured in ep collisions at HERA with the H1 detector in a data sample corresponding to an integrated luminosity of 71 pb^-1 at a centre of mass energy…

High Energy Physics - Experiment · Physics 2012-08-27 H1 Collaboration

Tracks events at the IceCube Observatory are characterized by an energetic muon crossing several kilometers before decaying. Such muons are dominantly produced in charged current (CC) muon neutrino - hadron interactions. However, muons are…

High Energy Physics - Phenomenology · Physics 2024-07-31 Reinaldo Francener , Victor P. Goncalves , Diego R. Gratieri

An accurate modeling of neutrino flux attenuation and the distribution of leptons they produce in transit through the Earth is an essential component to determine neutrino flux sensitivities of underground, sub-orbital and space-based…

We calculate contained and upward muon flux and contained shower event rates from neutrino interactions, when neutrinos are produced from annihilation of the dark matter in the Galactic Center. We consider model-independent direct neutrino…

High Energy Physics - Phenomenology · Physics 2014-11-20 Arif Emre Erkoca , Graciela Gelmini , Mary Hall Reno , Ina Sarcevic

Charged current interactions of neutrinos inside the Earth can result in secondary muons and $\tau$-leptons which are detectable by several existing and planned neutrino experiments through a wide variety of event topologies. Consideration…

Conserved muonic number may turn out to be a conserved muonic charge, coupled to muonic photons, gamma_mu. Muons and muonic neutrinos would emit gamma_mu's, which might be discovered by analysing the data from the past and future high…

High Energy Physics - Phenomenology · Physics 2009-10-30 V. A. Ilyin , L. B. Okun , A. N. Rozanov

In the framework of hypercolor scenario of multicomponent Dark Matter, inelastic interaction of high energy photons with the Dark Matter candidates is considered. This reaction results in production of energetic leptons and neutrinos, and…

High Energy Physics - Phenomenology · Physics 2022-11-21 Vitaly Beylin

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 energy of atmospheric neutrinos detected by MACRO was estimated using multiple coulomb scattering of upward throughgoing muons. This analysis allows a test of atmospheric neutrino oscillations, relying on the distortion of the muon…

High Energy Physics - Experiment · Physics 2012-08-27 The MACRO Collaboration

We present the measurement of the the flux and angular distribution of atmospheric muon neutrinos using the MACRO detector. Three different event topologies are detected in two different energy ranges. High energy neutrinos (E~80 GeV) via…

High Energy Physics - Experiment · Physics 2009-10-31 M. Spurio

We present a new calculation of the energy distribution of high-energy neutrinos from the decay of charm and bottom hadrons produced at the Large Hadron Collider (LHC). In the kinematical region of very forward rapidities, heavy-flavor…

High Energy Physics - Phenomenology · Physics 2020-06-11 Weidong Bai , Milind Diwan , Maria Vittoria Garzelli , Yu Seon Jeong , Mary Hall Reno

The ICAL at INO is designed to mainly observe the muons produced in the charged current interactions of atmospheric muon neutrinos and anti-neutrinos. The track of the muon is reconstructed using the hits they produce in the detector. From…

Instrumentation and Detectors · Physics 2020-08-26 Mohammad Nizam , S. Uma Sankar

The IceCube detector allows for the first time a measurement of atmospheric muon and neutrino energy spectra from tens of GeV up to the PeV range. The lepton flux in the highest energy region depends on both the primary cosmic ray…

High Energy Astrophysical Phenomena · Physics 2019-08-13 P. Berghaus

We evaluate both the tau lepton energy loss produced by photonuclear interactions and the neutrino charged current cross section at ultra-high energies, relevant to neutrino bounds with Earth-skimming tau neutrinos, using different…

High Energy Physics - Phenomenology · Physics 2008-11-26 N. Armesto , C. Merino , G. Parente , E. Zas
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