Probing Nucleon Spin Structure with a Polarized Gamma Beam from Compton Backscattering at FCC-ee
Abstract
We present a kinematic and optical design of a high-energy polarized gamma-ray facility based on Compton backscattering of lasers against the FCC-ee electron beams in its Z, WW, ZH and tt modes. The conversion point is located in the FCC-ee full-energy booster, allowing parasitic CBS operation without dedicated interaction-point optics. Saturating the safe value of the kinematic parameter κ= 4.35 in each mode fixes the laser wavelength and yields backscattered photons up to ω = 148~GeV. The facility operates in a parasitic mode with Compton fraction f CBS = 10-8 per bunch crossing, preserving the nominal FCC-ee collider luminosity; the corresponding operational laser pulse energies are in the millijoule range. Polarized photon selection is performed event-by-event via a pair spectrometer that reconstructs Eγ on the high-energy Compton edge, delivering circular polarization | S2| > 0.99. We project the resulting sensitivity to the polarized gluon distribution Δg(x) through open-charm photoproduction γp ccX on an NH3 dynamic-nuclear-polarization target, including next-to-leading-order QCD corrections via K-factors and propagating polarized-PDF uncertainties through the 100 Monte Carlo replicas of NNPDFpol2.0. The projected total precision on Δg(x)/g(x) is δ(Δg/g) tot 1.8--3.0× 10-2, a factor of 4--7 smaller than the total uncertainty of the most precise existing direct world measurement (HERMES, dominated by Monte-Carlo model uncertainties), with four distinct values of x in the medium-x region 0.07≤ x≤ 0.19. The proposed facility would set the dominant constraint on the polarized gluon distribution in the medium-x region, complementary to the low-x reach of the Electron--Ion Collider.
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