Speaker
Dr
Denis Bernard
(LLR, CNRS/IN2P3)
Description
gamma-ray astronomy is polarization-blind as no significant
polarimetry of a cosmic source has been performed since the [OSO-8 measurement on the Crab nebula][1] in the X-ray band.
gamma-ray polarimetry would enable to [tag the curvature-synchrotron radiation transition in pulsars][2], to [decipher leptonic from hadronic
radiation models for blazars][3] .. and [much more][4].
We [demonstrated][5] that with a low-density homogeneous active target such
as a gas TPC (time projection chamber), the single-track angular
resolution is so good after a low radiation-length thickness that
polarimetry should be possible with gamma conversions to e+e- pairs.
**With a TPC prototype in a gamma-ray beam, we demonstrated
experimentally the effective polarimetry with an excellent
polarization-asymmetry dilution** [AstroPart. Phys. 97 (2018) 10][6].
Spin-offs of interest to the community:
An analytical analysis of the single-track angular resolution with an
optimal tracking à la Kalman, an optimal method to measure a track
momentum in a non-magnetic tracker from the analysis of the
deflections due to multiple scattering ([Kalman][7] helping [Molière][8]),
interest to silicon-detector based telescopes (Fermi-LAT, AGILE,
e-ASTROGAM, AMEGO) [NIM A 867 (2017) 182][9].
An exact Monte carlo event generator of the five-dimensional (5D)
Bethe-Heitler differential cross section (polarized or not, nuclear
or triplet conversion, pure QED or with electron cloud screening) and
strictly energy-momentum conserving, [to appear in NIM A][10].
Good hope of a deployment of the G4BetheHeitler5DModel physics model
in the 10.5beta Geant4 release at the end of June 2018.
[1]: http://dx.doi.org/10.1086/182648
[2]: http://inspirehep.net/record/1641719
[3]: http://inspirehep.net/record/1242827
[4]: https://inspirehep.net/record/1498288
[5]: http://inspirehep.net/record/1242601
[6]: https://inspirehep.net/record/1606056
[7]: http://inspirehep.net/record/259509
[8]: http://zfn.mpdl.mpg.de/data/Reihe_A/10/ZNA-1955-10a-0177.pdf
[9]: https://inspirehep.net/record/1605726
[10]: https://doi.org/10.1016/j.nima.2018.05.021
Primary author
Dr
Denis Bernard
(LLR, CNRS/IN2P3)