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The measurements of the fluxes of atmospheric neutrinos give evidence for the disappearance of muon neutrinos. The determination of the dependence of the disappearance probability on the neutrino energy and trajectory allows in principle to…

High Energy Physics - Phenomenology · Physics 2009-10-31 Paolo Lipari , Maurizio Lusignoli

We plan to develop a new nuclear database for muon-induced nuclear reactions (muon nuclear data). The database will consist of (1) energies and intensities of the muonic X rays, (2) lifetimes of the muonic atom, (3) production branching…

Half-lives of proton emission for Z$\ge$51 nuclei are calculated within a simple analytical model based on the WKB approximation for the barrier penetration probability which includes the centrifugal and overlapping effects besides the…

Nuclear Theory · Physics 2017-09-13 R. Budaca , A. I. Budaca

We propose to measure the rate \Rd\ for muon capture on the deuteron to better than 1.5% precision. This process is the simplest weak interaction process on a nucleus that can both be calculated and measured to a high degree of precision.…

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

A joint effort of cryogenic microcalorimetry (CM) and high-precision Penning-trap mass spectrometry (PT-MS) in investigating atomic orbital electron capture (EC) can shed light on the possible existence of heavy sterile neutrinos with…

High Energy Physics - Phenomenology · Physics 2015-06-18 P. E. Filianin , K. Blaum , S. A. Eliseev , L. Gastaldo , Yu. N. Novikov , V. M. Shabaev , I. I. Tupitsyn , J. Vergados

MACRO can detect three topologies of neutrino induced events, corresponding to different parent neutrino energies. The most numerous sample is made of upward throughgoing muons induced by atmospheric neutrinos of average energy 100 GeV. We…

High Energy Physics - Experiment · Physics 2019-08-14 T. Montaruli

Recent measurements of pre-equilibrium neutron and proton transverse emission from (112,124)Sn+(112,124)Sn reactions at 50 MeV/A have been completed at the National Superconducting Cyclotron Laboratory. Free nucleon transverse emission…

This study conducted an analysis of muons, protons, and charged pions emitted from $\nu_{\mu}$ charged-current interactions on iron using a nuclear emulsion detector. The emulsion detector with a 65$\,$kg iron target was exposed to a…

The atmospheric neutrino passing fraction, or self-veto, is defined as the probability for an atmospheric neutrino not to be accompanied by a detectable muon from the same cosmic-ray air shower. Building upon previous work, we propose a…

High Energy Physics - Phenomenology · Physics 2018-08-08 Carlos A. Argüelles , Sergio Palomares-Ruiz , Austin Schneider , Logan Wille , Tianlu Yuan

The detection of the radio emission following a neutrino interaction in ice is a promising technique to obtain significant sensitivities to neutrinos with energies above PeV. The detectable radio emission stems from particle showers in the…

High Energy Astrophysical Phenomena · Physics 2020-10-21 Daniel García-Fernández , Christian Glaser , Anna Nelles

We study the neutrino distributions that arise in a simulation of a neutron star merger that uses a Monte Carlo (MC) neutrino transport scheme. In a snapshot taken 1 ms after merger, we calculate relevant observables to test when neutrinos…

High Energy Astrophysical Phenomena · Physics 2026-03-10 Mark G. Alford , Liam Brodie , Francois Foucart , Alexander Haber

Beams of protons and pions of 5.9 GeV/c were incident on a C target. Neutrons emitted into the back hemisphere, in the laboratory system, were detected in (triple) coincidence with two emerging $p_t>$0.6 GeV/c particles. We present the…

Cosmic-rays with energies up to $3\times10^{20}$ eV have been observed. The nuclear composition of these cosmic rays is unknown but if the incident nuclei are protons then the corresponding center of mass energy is $\sqrt{s_{nn}} = 700$…

Nuclear Experiment · Physics 2009-11-18 Spencer R. Klein

Atmospheric muons are the most frequently observed form of cosmic radiation. Despite this, the existence of the muon flux component produced in decays of short-lived parent particles, called prompt muon flux still awaits experimental…

High Energy Physics - Experiment · Physics 2024-02-07 Piotr Kalaczyński

The MuCap experiment measures the singlet rate Lambda_S of muon capture on the proton. A negative muon beam is stopped in a time projection chamber filled with ultra-pure hydrogen gas at 10 bar and room temperature. In combination with the…

Nuclear Experiment · Physics 2015-05-30 P. Winter

The T2K collaboration: reports evidence for electron neutrino appearance at the atmospheric mass splitting, |\Delta m_{32}^2|=2.4x10^{-3} eV^2. An excess of electron neutrino interactions over background is observed from a muon neutrino…

High Energy Physics - Experiment · Physics 2019-08-17 T2K Collaboration , K. Abe , N. Abgrall , H. Aihara , T. Akiri , J. B. Albert , C. Andreopoulos , S. Aoki , A. Ariga , T. Ariga , S. Assylbekov , D. Autiero , M. Barbi , G. J. Barker , G. Barr , M. Bass , M. Batkiewicz , F. Bay , S. W. Bentham , V. Berardi , B. E. Berger , S. Berkman , I. Bertram , D. Beznosko , S. Bhadra , F. d. M. Blaszczyk , A. Blondel , C. Bojechko , S. Boyd , D. Brailsford , A. Bravar , C. Bronner , D. G. Brook-Roberge , N. Buchanan , R. G. Calland , J. Caravaca Rodriguez , S. L. Cartwright , R. Castillo , M. G. Catanesi , A. Cervera , D. Cherdack , G. Christodoulou , A. Clifton , J. Coleman , S. J. Coleman , G. Collazuol , K. Connolly , L. Cremonesi , A. Curioni , A. Dabrowska , I. Danko , R. Das , S. Davis , M. Day , J. P. A. M. de Andre , P. de Perio , G. De Rosa , T. Dealtry , S. Dennis , C. Densham , F. Di Lodovico , S. Di Luise , J. Dobson , O. Drapier , T. Duboyski , F. Dufour , J. Dumarchez , S. Dytman , M. Dziewiecki , M. Dziomba , S. Emery , A. Ereditato , L. Escudero , A. J. Finch , E. Frank , M. Friend , Y. Fujii , Y. Fukuda , A. Furmanski , V. Galymov , A. Gaudin , S. Giffin , C. Giganti , K. Gilje , T. Golan , J. J. Gomez-Cadenas , M. Gonin , N. Grant , D. Gudin , D. R. Hadley , A. Haesler , M. D. Haigh , P. Hamilton , D. Hansen , T. Hara , M. Hartz , T. Hasegawa , N. C. Hastings , Y. Hayato , C. Hearty , R. L. Helmer , M. Hierholzer , J. Hignight , A. Hillairet , A. Himmel , T. Hiraki , S. Hirota , J. Holeczek , S. Horikawa , K. Huang , A. K. Ichikawa , K. Ieki , M. Ieva , M. Ikeda , J. Imber , J. Insler , T. J. Irvine , T. Ishida , T. Ishii , S. J. Ives , K. Iyogi , A. Izmaylov , A. Jacob , B. Jamieson , R. A. Johnson , J. H. Jo , P. Jonsson , K. K. Joo , C. K. Jung , A. Kaboth , H. Kaji , T. Kajita , H. Kakuno , J. Kameda , Y. Kanazawa , D. Karlen , I. Karpikov , E. Kearns , M. Khabibullin , F. Khanam , A. Khotjantsev , D. Kielczewska , T. Kikawa , A. Kilinski , J. Y. Kim , J. Kim , S. B. Kim , B. Kirby , J. Kisiel , P. Kitching , T. Kobayashi , G. Kogan , A. Kolaceke , A. Konaka , L. L. Kormos , A. Korzenev , K. Koseki , Y. Koshio , K. Kowalik , I. Kreslo , W. Kropp , H. Kubo , Y. Kudenko , S. Kumaratunga , R. Kurjata , T. Kutter , J. Lagoda , K. Laihem , A. Laing , M. Laveder , M. Lawe , M. Lazos , K. P. Lee , C. Licciardi , I. T. Lim , T. Lindner , C. Lister , R. P. Litchfield , A. Longhin , G. D. Lopez , L. Ludovici , M. Macaire , L. Magaletti , K. Mahn , M. Malek , S. Manly , A. Marchionni , A. D. Marino , J. Marteau , J. F. Martin , T. Maruyama , J. Marzec , P. Masliah , E. L. Mathie , V. Matveev , K. Mavrokoridis , E. Mazzucato , N. McCauley , K. S. McFarland , C. McGrew , T. McLachlan , M. Messina , C. Metelko , M. Mezzetto , P. Mijakowski , C. A. Miller , A. Minamino , O. Mineev , S. Mine , A. Missert , M. Miura , L. Monfregola , S. Moriyama , Th. A. Mueller , A. Murakami , M. Murdoch , S. Murphy , J. Myslik , T. Nagasaki , T. Nakadaira , M. Nakahata , T. Nakai , K. Nakajima , K. Nakamura , S. Nakayama , T. Nakaya , K. Nakayoshi , D. Naples , T. C. Nicholls , C. Nielsen , M. Nirkko , K. Nishikawa , Y. Nishimura , H. M. O'Keeffe , Y. Obayashi , R. Ohta , K. Okumura , T. Okusawa , W. Oryszczak , S. M. Oser , M. Otani , R. A. Owen , Y. Oyama , M. Y. Pac , V. Palladino , V. Paolone , D. Payne , G. F. Pearce , O. Perevozchikov , J. D. Perkin , Y. Petrov , E. S. Pinzon Guerra , P. Plonski , E. Poplawska , B. Popov , M. Posiadala , J. -M. Poutissou , R. Poutissou , P. Przewlocki , B. Quilain , E. Radicioni , P. N. Ratoff , M. Ravonel , M. A. M. Rayner , M. Reeves , E. Reinherz-Aronis , F. Retiere , A. Robert , P. A. Rodrigues , E. Rondio , S. Roth , A. Rubbia , D. Ruterbories , R. Sacco , K. Sakashita , F. Sanchez , E. Scantamburlo , K. Scholberg , J. Schwehr , M. Scott , D. I. Scully , Y. Seiya , T. Sekiguchi , H. Sekiya , D. Sgalaberna , M. Shibata , M. Shiozawa , S. Short , Y. Shustrov , P. Sinclair , B. Smith , R. J. Smith , M. Smy , J. T. Sobczyk , H. Sobel , M. Sorel , L. Southwell , P. Stamoulis , J. Steinmann , B. Still , A. Suzuki , K. Suzuki , S. Y. Suzuki , Y. Suzuki , T. Szeglowski , M. Szeptycka , R. Tacik , M. Tada , S. Takahashi , A. Takeda , Y. Takeuchi , H. A. Tanaka , M. M. Tanaka , M. Tanaka , I. J. Taylor , D. Terhorst , R. Terri , L. F. Thompson , A. Thorley , S. Tobayama , W. Toki , T. Tomura , Y. Totsuka , C. Touramanis , T. Tsukamoto , M. Tzanov , Y. Uchida , K. Ueno , A. Vacheret , M. Vagins , G. Vasseur , T. Wachala , A. V. Waldron , C. W. Walter , D. Wark , M. O. Wascko , A. Weber , R. Wendell , R. J. Wilkes , M. J. Wilking , C. Wilkinson , Z. Williamson , J. R. Wilson , R. J. Wilson , T. Wongjirad , Y. Yamada , K. Yamamoto , C. Yanagisawa , S. Yen , N. Yershov , M. Yokoyama , T. Yuan , A. Zalewska , L. Zambelli , K. Zaremba , M. Ziembicki , E. D. Zimmerman , M. Zito , J. Zmuda

We consider two basic nuclear reactions: Radiative capture of neutrons by protons, $n+p\to \gamma+~d$ and its time-reversed counterpart, photodisintegration of the deuteron, $\gamma +d\to n+p$. In both of these cases we assume that the…

Nuclear Theory · Physics 2018-05-09 Andrei Afanasev , Valery G. Serbo , Maria Solyanik

Although the electromagnetic and muonic components of extensive air showers have been studied in great detail, no comprehensive simulation study of the neutron component is available. This is related to the complexity of neutron transport…

High Energy Physics - Phenomenology · Physics 2024-06-18 Martin Schimassek , Ralph Engel , Alfredo Ferrari , Markus Roth , David Schmidt , Darko Veberič

We estimate the benefit of muon colliders for photon physics. We calculate the rate at which photons are emitted from muon beams in different production mechanisms. Bremsstrahlung is reduced, beamstrahlung disappears, and laser…

High Energy Physics - Phenomenology · Physics 2014-11-17 Michael Klasen