7–12 May 2023
Venice, Italy
Europe/Zurich timezone

Increasing the flux of a Thomson source while maintaining a narrow bandwidth by using large energy spread primary particles

TUPL177
9 May 2023, 16:30
2h
Sala Laguna

Sala Laguna

Poster Presentation MC2.A23: Other Linac Based Photon Sources Tuesday Poster Session

Speaker

Marcel Ruijter (Istituto Nazionale di Fisica Nucleare)

Description

Thomson/Compton scattering is a method to produce high energy photons through the collision of low energy photons in a laser pulse onto relativistic electrons. In the linear (incoherent) Thomson/Compton regime, the flux scales linearly with the number of primary particles and the bandwidth of the produced photons depend, amongst other factors, on the energy spread of them. In general, an increase of the primary particles is connected to a larger energy spread (e.g.non-constant acceleration gradients, collective effects, etc). Therefore their number is restricted by the desired bandwidth, and thus limits the flux.
In our previous (theoretical) studies we showed that the ideal Thomson spectrum can be retrieved when an electron bunch with a linear energy correlation of several percent collides with a matched linearly chirped laser pulse. Here we extend the scheme to allow for higher order energy correlations and quantify how the electron distribution influences the bandwidth. Furthermore we discuss the practical viability to maximize the primary particles, with the focus on linear accelerators (LINACS) for the electrons and laser pulses based on the chirped pulse amplification (CPA) scheme. These could potentially provide up to tens of nano-Coulomb electron bunches and tens, or even over a hundred, Joule lasers pulses respectively.

I have read and accept the Privacy Policy Statement Yes

Primary author

Marcel Ruijter (Istituto Nazionale di Fisica Nucleare)

Co-authors

Alberto Bacci (Istituto Nazionale di Fisica Nucleare) Andrea Rossi (Istituto Nazionale di Fisica Nucleare) Illya Drebot (Istituto Nazionale di Fisica Nucleare) Luca Serafini (Istituto Nazionale di Fisica Nucleare) Marcello Rossetti Conti (Istituto Nazionale di Fisica Nucleare) Michele Opromolla (Università degli Studi di Milano) Sanae Samsam (Istituto Nazionale di Fisica Nucleare) Vittoria Petrillo (Universita' degli Studi di Milano)

Presentation materials

There are no materials yet.