TY  - JOUR
PB  - SciPost Foundation
DO  - 10.21468/SciPostPhysProc.13.006
TI  - New determination of the production cross section for secondary positrons and electrons in the Galaxy
PY  - 2023/09/28
UR  - https://scipost.org/SciPostPhysProc.13.006
JF  - SciPost Physics Proceedings
JA  - SciPost Phys. Proc.
VL  - 
IS  - 13
SP  - 006
A1  - Orusa, Luca
AU  - Di Mauro, Mattia
AU  - Donato, Fiorenza
AU  - Korsmeier, Michael
AB  - The cosmic-ray fluxes of electrons and positrons ($e^{±}$) are measured with high precision by the space-borne particle spectrometer AMS-02. To infer a precise interpretation of the production processes for $e^{±}$ in our Galaxy, it is necessary to have an accurate description of the secondary component, produced by the interaction of cosmic-ray proton and helium with the interstellar medium atoms. We determine new analytical functions of the Lorentz invariant cross section for the production of $e^±$ by fitting data from collider experiments. The total differential cross section $d\sigma/dT_{e^±}(p+p→ e^±+X)$ is predicted with an uncertainty of about 5-7% in the energies relevant for AMS-02 positron flux. For further information about this work refer to [Phys. Rev. D 105, 123021 (2022)].
ER  -

@Article{10.21468/SciPostPhysProc.13.006,
	title={{New determination of the production cross section for secondary positrons and electrons in the Galaxy}},
	author={Luca Orusa and Mattia Di Mauro and Fiorenza Donato and Michael Korsmeier},
	journal={SciPost Phys. Proc.},
	pages={006},
	year={2023},
	publisher={SciPost},
	doi={10.21468/SciPostPhysProc.13.006},
	url={https://scipost.org/10.21468/SciPostPhysProc.13.006},
}