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相关论文: Photon splitting above the pair creation threshold…

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The photon-neutrino process gamma gamma -> nu bar nu and photon splitting are considered in a strong magnetic field. The partial polarization amplitudes are calculated within the standard model in the limit of a strong field. The amplitudes…

高能物理 - 唯象学 · 物理学 2007-05-23 M. V. Chistyakov , A. V. Kuznetsov , N. V. Mikheev

The process of photon splitting, becomes allowed in the presence of strong magnetic field. We calculate the influence of magnetized plasma on the photon splitting absorption coefficient. We calculate the refraction coefficients and…

天体物理学 · 物理学 2007-05-23 Tomasz Bulik

Photon splitting in a very strong magnetic field is analyzed for energy $\omega < 2m$. The amplitude obtained on the base of operator-diagram technique is used. It is shown that in a magnetic field much higher than critical one the…

高能物理 - 理论 · 物理学 2009-10-30 V. N. Baier , A. I. Milstein , R. Zh. Shaisultanov

The process of photon splitting is investigated in the presence of strongly magnetized electron-positron plasma. The amplitude of the process is calculated in general case of plasma with nonzero chemical potential and temperature. The…

高能物理 - 唯象学 · 物理学 2012-09-03 M. V. Chistyakov , D. A. Rumyantsev , N. S. Stus'

withdrawn - wrong selection rules used.

高能物理 - 唯象学 · 物理学 2008-02-03 M. Kachelriess , G. Wunner

We recalculate the amplitude for photon splitting in a strong magnetic field below the pair production threshold, using the worldline path integral variant of the Bern--Kosower formalism. Numerical comparison (using programs that we have…

高能物理 - 理论 · 物理学 2009-10-30 Stephen L. Adler , Christian Schubert

We present the results of a numerical calculation of the photon splitting rate below the electron-pair creation threshold ($\omega \le 2m$) in magnetic fields $B ~{> \atop \sim}~ B_{\rm cr} = m^2 /e = 4.414 \times 10^{9}$ T. Our results…

高能物理 - 理论 · 物理学 2009-10-30 C. Wilke , G. Wunner

We reassess the importance of photon splitting to spectral formation in cosmic X-ray and $\gamma$-ray sources with magnetic fields of several $10^{12}$ gauss. Our analysis is based on the recent numerically accurate evaluation of the full…

天体物理学 · 物理学 2009-10-28 Günter Wunner , Robert Sang , Dagmar Berg

We discuss the polarization selection rules for splitting of the two principal electromagnetic modes that propagate in a vacuum polarized by a superstrong magnetic field (B>0.1B_{cr} ~ 4x10^{12} G). We show that below the threshold of free…

天体物理学 · 物理学 2011-04-04 Vladimir V. Usov

The magnetospheres of neutron stars provide a valuable testing ground for as-yet unverified theoretical predictions of quantum electrodynamics (QED) in strong electromagnetic fields. Exhibiting magnetic field strengths well in excess of a…

天体物理学 · 物理学 2009-06-23 Matthew G. Baring

The process of pair creation by a photon in a strong magnetic field is investigated basing on the polarization operator in the field. The total probability of the process is found in a relatively simple form. The probability exhibits a…

高能物理 - 唯象学 · 物理学 2008-11-26 V. N. Baier , V. M. Katkov

Magnetic photon splitting, a QED process that becomes important only in magnetic fields approaching the quantum critical value, B_cr = 4.41 X 10^13 Gauss, is investigated as a mechanism for attenuation of gamma-rays emitted near the surface…

天体物理学 · 物理学 2009-10-28 Alice K. Harding , Matthew G. Baring , Peter L. Gonthier

The splitting of photons in the presence of an intense magnetic field has recently found astrophysical applications in polar cap models of gamma-ray pulsars and in magnetar scenarios for soft gamma repeaters. Numerical computation of the…

天体物理学 · 物理学 2009-10-30 Matthew G. Baring , Alice K. Harding

The process of the photon decay into the neutrino - antineutrino pair in a magnetic field is investigated. The amplitude and the probability are analysed in the limits of relatively small and strong fields. The probability is suppressed by…

高能物理 - 唯象学 · 物理学 2009-10-30 A. V. Kuznetsov , N. V. Mikheev , L. A. Vassilevskaya

Photon splitting is a QED process that can potentially suppress pair production in the inner magnetosphere of a pulsar with a super-strong magnetic field, and hence, may quench radio emission from these objects. While it is unknown how many…

天体物理学 · 物理学 2007-05-23 Bing Zhang , Alice K. Harding

The recent association of soft gamma repeaters (SGRs) with counterparts in other wavebands has sparked much interest in these sources. One of the recent models for these objects is that they originate in the environs of neutron stars with…

天体物理学 · 物理学 2009-10-28 M. G. Baring , A. K. Harding

Magnetars are neutron stars characterized by strong surface magnetic fields generally exceeding the quantum critical value of 44.1 TeraGauss. High-energy photons propagating in their magnetospheres can be attenuated by QED processes like…

高能天体物理现象 · 物理学 2022-11-30 Kun Hu , Matthew G. Baring , Alice K. Harding , Zorawar Wadiasingh

The photon splitting gamma -> gamma gamma in a time-independent and inhomogeneous magnetized background is considered when neutral and ultralight spin-0 particles are coupled to two-photons. Depending on the inhomogeneity scale of the…

高能物理 - 唯象学 · 物理学 2007-05-23 Emidio Gabrielli , Massimo Giovannini

Various differential cross sections of high-energy photon splitting in the electric fields of heavy atoms are calculated exactly in the parameter \al. The consideration is based on the quasiclassical approach applicable for small angles…

高能物理 - 唯象学 · 物理学 2008-11-26 R. N. Lee , A. I. Milstein , V. M. Strakhovenko

Damping of an electromagnetic wave in a strong magnetic field is analyzed in the kinematic region near the threshold of electron-positron pair production. Damping of the electromagnetic field is shown to be noticeably nonexponential in this…

高能物理 - 唯象学 · 物理学 2010-11-15 N. V. Mikheev , M. V. Chistyakov
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