Figure - available from: AIP Advances
This content is subject to copyright. Terms and conditions apply.
Time evolution of the (a) photon number density and (b) electron number density summed over the y-axis. (a) At t < 0, photons are emitted in the forward direction at the speed of light with two ωL periodicity from the nanowire tip during the turning point of the j × B heating. The number density of photons increases at t > 0, as a result of the nonlinear inverse Compton scattering between the attosecond bunches and the reflected laser field. At t ∼ 20 fs, some photons are observed to propagate in the backward direction, which is attributed to the scattering with the reflux electrons. (b) Electrons are constantly being pulled out and pushed back into the nanowire tip due to the oscillating term of the ponderomotive force at the rising edge of the laser pulse (t < 0). Some electrons are observed to penetrate the supporting substrate, as shown between 6.5 and 8 µm. These electrons, without enough energy, will re-enter the nanowire and move in the −x direction.

Time evolution of the (a) photon number density and (b) electron number density summed over the y-axis. (a) At t < 0, photons are emitted in the forward direction at the speed of light with two ωL periodicity from the nanowire tip during the turning point of the j × B heating. The number density of photons increases at t > 0, as a result of the nonlinear inverse Compton scattering between the attosecond bunches and the reflected laser field. At t ∼ 20 fs, some photons are observed to propagate in the backward direction, which is attributed to the scattering with the reflux electrons. (b) Electrons are constantly being pulled out and pushed back into the nanowire tip due to the oscillating term of the ponderomotive force at the rising edge of the laser pulse (t < 0). Some electrons are observed to penetrate the supporting substrate, as shown between 6.5 and 8 µm. These electrons, without enough energy, will re-enter the nanowire and move in the −x direction.

Source publication
Article
Full-text available
A highly energetic photon is emitted via nonlinear inverse Compton scattering after an electron undergoes scattering with an ultra-intense relativistic laser pulse. In the laser-nanostructured interaction, gamma photons are emitted in different directions due to different electron heating mechanisms. However, the physics that leads to such gamma-ph...

Similar publications

Preprint
Full-text available
1LHAASO J0249+6022 is an extended very-high-energy gamma-ray source discovered by the Large High-Altitude Air Shower Observatory. Based on nearly 16.1 years of data from the Fermi Large Area Telescope, we report the probable gamma-ray emission from 1LHAASO J0249+6022 in the 0.03-1 TeV energy range. The results show that its gamma-ray spectrum can b...
Preprint
Full-text available
The non-linear Compton scattering rate in a rotating electric field is explicitly calculated for the first time. For this purpose, a novel solution to the Klein-Gordon equation in the presence of a rotating electric field is applied. An analytical expression for the emission rate is obtained, as well as a simplified approximation adequate for emple...