L.G. Dedenko M.V. Lomonosov Moscow State University, 119992 Moscow, Russia

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The Hybrid Scheme of Simulations of the Electron- photon and Electron-hadron Cascades In a Dense Medium at Ultra-high Energies. L.G. Dedenko M.V. Lomonosov Moscow State University, 119992 Moscow, Russia. Content. Introduction Hybrid multilevel scheme The 5-level scheme for the atmosphere - PowerPoint PPT Presentation

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  • The Hybrid Scheme of Simulations of the Electron- photon and Electron-hadron Cascades In a Dense Medium at Ultra-high EnergiesL.G. Dedenko M.V. Lomonosov Moscow State University, 119992 Moscow, Russia

  • ContentIntroductionHybrid multilevel schemeThe 5-level scheme for the atmosphereExamplesConclusion

  • GOALS Simulations of cascades at ultra-high energiesAcoustical (radio) signals productionTransport of acoustical (radio) signals in the real matterDetections of signals

  • ENERGY SCALE

  • SPACE SCALE

  • Transport equations for hadrons:here k=1,2,....m number of hadron types; - number of hadrons k in bin EE+dE and depth bin xx+dx; k(E) interaction length; Bk decay constant; Wik(E,E) energy spectra of hadrons of type k produced by hadrons of type i.

  • The integral form: here

    E0 energy of the primary particle; Pb (E,xb) boundary condition; xb point of interaction of the primary particle.

  • The decay products of neutral pions are regarded as a source function S(E,x) of gamma quanta which give origins of electron-photon cascades in the atmosphere:

    Here a number of neutral pions decayed at depth x+ dx with energies E+dE

  • The basic cascade equations for electrons and photons can be written as follows:

    where (E,t), P(E,t) the energy spectra of photons and electrons at the depth t; the ionization losses; e, the absorption coefficients; Wb, Wp the bremsstrahlung and the pair production cross-sections; Se, S the source terms for electrons and photons.

  • The integral form:

    where

    At last the solution of equations can be found by the method of subsequent approximations. It is possible to take into account the Compton effect and other physical processes.

  • Source functions for low energy electrons and gamma quanta

    x=min(E0;E/)

  • For the various energies Emin Ei Eth (Emin=1 MeV, Eth=10 GeV)

    and starting points of cascades0XkX0 (X0=1020 gcm-2)

    simulations of ~ 2108 cascades in the atmosphere with help of CORSIKA code and responses (signals) of the scintillator detectors using GEANT 4 code SIGN(Rj,Ei,Xk)SIGN(Rj,Ei,Xk)10mRj2000mhave been calculated

  • SIGNAL ESTIMATION

  • Responses of scintillator detectors at distance Rj from the shower core (signals S(Rj))

    Eth=10 GeVEmin=1 MeV

  • ENERGY DEPOSITION

  • POSITIVE CHARGE (GEANT4)

  • NEGATIVE CHARGE (GEANT4)

  • FOR HADRON CASCADESFLUCTUATIONS ARE OF IMPORTANCE

  • CHARGE EXCESS (GEANT4)

  • THIS FUNCTIONS SHOULD BE ESTIMATED WITH THE GEANT4 CODE WITH STATISTICS OF 10**6

  • FOR E=10**12 GEV NEARLY10**12 PARTICLES SHOULD BETAKEN INTO ACCOUNT

  • FOR ELECTRON-PHOTON CASCADES FLUCTUATIONS ARE VERY IMPORTANT DUE TO THE LPM-EFFECT

  • EXAMPLESor

  • The Poisson formulae

  • Energy deposition Q=dE/dV in water

  • Energy deposition in water

  • Energy deposition in water

  • Energy deposition in water

  • ENERGY DEPOSITION IN WATER

  • ENERGY DEPOSITION IN WATER

  • ENERGY DEPOSITION IN WATER

  • ENERGY DEPOSITION IN WATER

  • ENERGY DEPOSITION IN WATER

  • Charge excess

  • Lateral distributions of gammas, electrons and positrons

  • ENERGY DEPOSITION in detector

  • Energy distributions of gammas, electrons, positrons

  • Ratio of a signal to a charge particle density

  • el_ed.jpg

  • ga_ed.jpg

  • pos_ed.jpg

  • ConclusionThe hybrid multilevel scheme has been suggested to estimate acoustical (radio) signals produced by e and eh cascades in dense medium.

  • AcknowledgementsWe thank G.T. Zatsepin for useful discussions, the RFFI (grant 03-02-16290), INTAS (grant 03-51-5112) and LSS-1782.2003.2 for financial support.

  • Number of muons in a group with hk(xk) and Ei :

    here P(E,x) from equations for hadrons; D(E,E) decay function; limits Emin(E), Emax(E); W(E,Ethr,x,x0) probability to survive.

  • Transverse impulse distribution:

    here p0=0.2 /.

  • The angle :

    here hk= hk(xk) production height for hadrons.

  • Direction of muon velocity is defined by directional cosines:

    All muons are defined in groups with bins of energy EiEi+E; angles jj+j, m m+ m and height production hk hk +hk. The average values have been used: , , and . Number of muons and were regarded as some weights.

  • The relativistic equation:

    here m muon mass; e charge; lorentz factor; t time; geomagnetic field.

  • The explicit 2-d order scheme:

    here ; Ethr , E threshold energy and muon energy.

  • Ratio with to without magnetic field