Radiation of the magneto-crystalline undulator

Dades bibliogràfiques
Parent link:Journal of Physics: Conference Series
Vol. 732 : Radiation from Relativistic Electrons in Periodic Structures (RREPS2015).— 2016.— [012024, 7 p.]
Autor principal: Epp V.
Autor corporatiu: Национальный исследовательский Томский политехнический университет (ТПУ) Физико-технический институт (ФТИ) Кафедра прикладной физики (№ 12) (ПФ) Международная научно-образовательная лаборатория "Рентгеновская оптика" (МНОЛ РО)
Altres autors: Kaplin V. V. Valery Viktorovich
Sumari:Title screen
The radiation at grazing incidence of relativistic positively charged particles on the crystal surface in the presence of magnetic field is studied theoretically. The magnetic field is supposed to be parallel to the surface. Dependent on the initial conditions the particle can be captured in the channeling mode and perform periodic oscillations along the surface of the crystal. The spectrum, angular distribution and polarization of radiation are calculated. The emission spectrum of a single particle is discrete and it extends up to very large numbers of harmonics. If the magnetic field is much weaker than the electric field of atoms, the frequency range of radiation of the particle beam does not depend on magnetic field and is defined solely by the energy of the particles and by the surface averaged potential, though the frequency of the first harmonic is defined only by the magnetic field. In case of channeled positrons the characteristic energy of the emitted photons is of order 10?3/2 (eV), where ? is the particle relativistic factor. The main part of radiation is bound to a narrow cone and is polarized largely orthogonal to the surface of the crystal.
Publicat: 2016
Col·lecció:Coherent Bremsstrahlung and Channeling Radiation
Matèries:
Accés en línia:http://dx.doi.org/10.1088/1742-6596/732/1/012024
http://earchive.tpu.ru/handle/11683/33960
Format: Electrònic Capítol de llibre
KOHA link:https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=650752

MARC

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330 |a The radiation at grazing incidence of relativistic positively charged particles on the crystal surface in the presence of magnetic field is studied theoretically. The magnetic field is supposed to be parallel to the surface. Dependent on the initial conditions the particle can be captured in the channeling mode and perform periodic oscillations along the surface of the crystal. The spectrum, angular distribution and polarization of radiation are calculated. The emission spectrum of a single particle is discrete and it extends up to very large numbers of harmonics. If the magnetic field is much weaker than the electric field of atoms, the frequency range of radiation of the particle beam does not depend on magnetic field and is defined solely by the energy of the particles and by the surface averaged potential, though the frequency of the first harmonic is defined only by the magnetic field. In case of channeled positrons the characteristic energy of the emitted photons is of order 10?3/2 (eV), where ? is the particle relativistic factor. The main part of radiation is bound to a narrow cone and is polarized largely orthogonal to the surface of the crystal. 
461 0 |0 (RuTPU)RU\TPU\network\3526  |t Journal of Physics: Conference Series 
463 0 |0 (RuTPU)RU\TPU\network\15969  |t Vol. 732 : Radiation from Relativistic Electrons in Periodic Structures (RREPS2015)  |o XI International Symposium, 6–11 September 2015, Saint Petersburg, Russian Federation  |o [proceedings]  |f National Research Tomsk Polytechnic University (TPU)  |v [012024, 7 p.]  |d 2016 
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700 1 |a Epp  |b V. 
701 1 |a Kaplin  |b V. V.  |c physicist  |c senior research fellow at Tomsk Polytechnic University  |f 1947-  |g Valery Viktorovich  |3 (RuTPU)RU\TPU\pers\31532  |9 15693 
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