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Electron beam quality kQ,Q0 factors for various ionization chambers: A Monte Carlo investigation with PENELOPE
(INSTITUTE OF PHYSICS PUBLISHING, 2014-11-07)
In this work we calculate the beam quality correction factor kQ,Q0 for various plane-parallel ionization chambers. A set of Monte Carlo calculations using the code penelope/penEasy have been carried out to calculate the ...
Electron beam quality kQ,Q0 factors for various ionization chambers: a Monte Carlo investigation with penelope
(2014)
n this work we calculate the beam quality correction factor ${{k}_{\text{Q},{{\text{Q}}_{0}}}}$ for various plane-parallel ionization chambers. A set of Monte Carlo calculations using the code penelope/penEasy have been ...
Chemodynamics of green pea galaxies - I. Outflows and turbulence driving the escape of ionizing photons and chemical enrichment
(Wiley Blackwell Publishing, Inc, 2020-05)
We investigate the ionized gas kinematics, physical properties, and chemical abundances of Sloan Digital Sky Survey J142947, a Green Pea galaxy at redshift z ∼ 0.17 with strong, double-peak Ly α emission and indirect ...
Two, three and four photon absorption of naphthaleneTwo, three and four photon absorption of naphthalene
(Revista Mexicana de Física, 2010)
Electron beam quality kQ,Q0 factors for various ionization chambers: A Monte Carlo investigation with PENELOPE
(INSTITUTE OF PHYSICS PUBLISHING, 2018)
Kinetic Energy Release Of The Singly And Doubly Charged Methylene Chloride Molecule: The Role Of Fast Dissociation
(Amer Chemical SocWashington, 2016)
Sub-Poissonian angular momentum distribution near threshold in atomic ionization by short-laser pulses
(American Physical Society, 2008-12)
We analyze the angular momentum distribution of electrons near threshold in atomic ionization by short laser pulses. The radial fanlike pattern in the two-dimensional momentum distribution observed in experiments is ...
Ionized gas, molecules and dust in Sh2-132
(Wiley, 2010-07)
We analyse the various interstellar components of the H II region Sh2-132. The main stellar source is the double binary system that includes the Wolf–Rayet star WR 153ab. We use radio continuum images at 408 and 1420 MHz, ...
Desenvolvimento de uma câmara de ionização para o LNLS
([s.n.], 1996)