2020
DOI: 10.1088/1367-2630/ab623b
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Spin-dependent radiative deflection in the quantum radiation-reaction regime

Abstract: A new spin-dependent deflection mechanism is revealed by considering the spin-correlated radiationreaction force during laser-electron collision. We found that such deflection originates from the nonzero work done by the radiation-reaction force along the laser polarization direction in each halfperiod, which is larger/smaller for spin-anti-paralleled/spin-paralleled electrons. The resulted antisymmetric deflection is further accumulated when the spin-projection onto the laser magnetic field is reversed in adj… Show more

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Cited by 21 publications
(15 citation statements)
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“…Due to a spin-dependent radiation reaction, a monochromatic, elliptically polarized laser pulse can split an initially unpolarized relativistic electron ensemble along the propagation direction into two oppositely transversely polarized parts; see Figure 1. A similar spin-dependent deflection mechanism is found by Geng et al [36] , who study the spin-correlated radiation-reaction force during the interaction of an initially polarized electron bunch with a linearly polarized laser pulse. The discovered mechanism dominates over the Stern-Gerlach force, which can provide a new perspective for studying spin-dependent QED effects.…”
Section: Polarization Build-up From Interactions With Relativistic Lasupporting
confidence: 75%
See 1 more Smart Citation
“…Due to a spin-dependent radiation reaction, a monochromatic, elliptically polarized laser pulse can split an initially unpolarized relativistic electron ensemble along the propagation direction into two oppositely transversely polarized parts; see Figure 1. A similar spin-dependent deflection mechanism is found by Geng et al [36] , who study the spin-correlated radiation-reaction force during the interaction of an initially polarized electron bunch with a linearly polarized laser pulse. The discovered mechanism dominates over the Stern-Gerlach force, which can provide a new perspective for studying spin-dependent QED effects.…”
Section: Polarization Build-up From Interactions With Relativistic Lasupporting
confidence: 75%
“…In general, the radiation-reaction force exceeds the Stern-Gerlach force by far if the particles are relativistic (kinetic energies well above 1 GeV) or even ultrarelativistic (above 1 TeV) (see also Ref. [36]). There are, however, some field configurations that reverse this situation, so that the radiation-reaction force can be neglected compared to the Stern-Gerlach force (see e.g., Ref.…”
Section: Theoretical Backgroundmentioning
confidence: 99%
“…The spin modifies the particle momentum indirectly, by affecting the radiation power (Del and thereby the strength of radiation reaction. Signatures of spindependent radiative deflection in tightly focused lasers are studied in Geng et al (2020). However, if the external electromagnetic field is non-homogeneous, its interaction with the spin also leads directly to a force on the particle; this contribution to the equation of motion is often referred to as the 'Stern-Gerlach force', after the seminal experiment that demonstrated the intrinsic quantum nature of the electron magnetic moment (Gerlach and Stern, 1922).…”
Section: 𝑔 𝑠mentioning
confidence: 99%
“…To simulate the radiative polarization under this condition, various numerical calculation models have been developed. One of the commonly used models is based on the Monte Carlo method with the help of an artificially selected axis, and the axis is called the spin quantization axis (SQA) in some articles [16,[34][35][36]. Specifically, the electron emits photons following the same method as the normal Monte Carlo model of photon emission where the spin polarization is not considered [37][38][39][40][41][42][43][44], and once the electron emits a photon, the spin falls on a certain state of the SQA (i.e., the state oriented in the same or in the opposite direction with respect to the direction of the SQA) determined by a random number according to the probability.…”
Section: Introductionmentioning
confidence: 99%