Strong interaction physics at the luminosity frontier with 22 GeV electrons at Jefferson Lab

Accardi, A; Achenbach, P; Adhikari, D; Afanasev, A; Akondi, Cs; Akopov, N; Albaladejo, M; Albataineh, H; Albrecht, M; Almeida-Zamora, B; Amaryan, M; Androić, D; Armstrong, W; Armstrong, Ds; Arratia, M; Arrington, J; Asaturyan, A; Austregesilo, A; Avakian, H; Averett, T; Gayoso, Ca; Bacchetta, A; Balantekin, Ab; Baltzell, N; Barion, L; Barry, Pc; Bashir, A; Battaglieri, M; Bellini, V; Belov, I; Benhar, O; Benkel, B; Benmokhtar, F; Bentz, W; Bertone, V; Bhatt, H; Bianconi, A; Bibrzycki, L; Bijker, R; Binosi, D; Biswas, D; Boër, M; Boeglin, W; Bogacz, Sa; Boglione, M; Bondí, M; Boos, Ee; Bosted, P; Bozzi, G; Brash, Ej; Briceño, Ra; Brindza, Pd; Briscoe, Wj; Brodsky, Sj; Brooks, Wk; Burkert, Vd; Camsonne, A; Cao, T; Cardman, Ls; Carman, Ds; Carpinelli, M; Cates, Gd; Caylor, J; Celentano, A; Celiberto, Fg; Cerutti, M; Chang, L; Chatagnon, P; Chen, C; Chen, J-; Chetry, T; Christopher, A; Christy, E; Chudakov, E; Cisbani, E; Cloët, Ic; Cobos-Martinez, Jj; Cohen, Eo; Colangelo, P; Cole, Pl; Constantinou, M; Contalbrigo, M; Costantini, G; Cosyn, W; Cotton, C; Courtoy, A; Dusa, Sc; Crede, V; Cui, Z-; D'Angelo, A; Döring, M; Dalton, Mm; Danilkin, I; Davydov, M; Day, D; De Fazio, F; De Napoli, M; De Vita, R; Dean, Dj; Defurne, M; De Paula, W; De Téramond, Gf; Deur, A; Devkota, B; Dhital, S; Di Nezza, P; Diefenthaler, M; Diehl, S; Dilks, C; Ding, M; Djalali, C; Dobbs, S; Dupré, R; Dutta, D; Edwards, Rg; Egiyan, H; Ehinger, L; Eichmann, G; Elaasar, M; Elouadrhiri, L; Alaoui, Ae; Fassi, Le; Emmert, A; Engelhardt, M; Ent, R; Ernst, Dj; Eugenio, P; Evans, G; Fanelli, C; Fegan, S; Fernández-Ramírez, C; Fernandez, La; Fernando, Ip; Filippi, A; Fischer, Cs; Fogler, C; Fomin, N; Frankfurt, L; Frederico, T; Freese, A; Fu, Y; Gamberg, L; Gan, L; Gao, F; Garcia-Tecocoatzi, H; Gaskell, D; Gasparian, A; Gates, K; Gavalian, G; Ghoshal, Pk; Giachino, A; Giacosa, F; Giannuzzi, F; Gilfoyle, G-; Girod, F-; Glazier, Di; Gleason, C; Godfrey, S; Goity, Jl; Golubenko, Aa; Gonzàlez-Solís, S; Gothe, Rw; Gotra, Y; Griffioen, K; Grocholski, O; Grube, B; Guèye, P; Guo, F-; Guo, Y; Guo, L; Hague, Tj; Hammoud, N; Hansen, J-; Hattawy, M; Hauenstein, F; Hayward, T; Heddle, D; Heinrich, N; Hen, O; Higinbotham, Dw; Higuera-Angulo, Im; Hiller Blin, An; Hobart, A; Hobbs, T; Holmberg, De; Horn, T; Hoyer, P; Huber, Gm; Hurck, P; Hutauruk, Ptp; Ilieva, Y; Illari, I; Ireland, Dg; Isupov, El; Italiano, A; Jaegle, I; Jarvis, Ns; Jenkins, Dj; Jeschonnek, S; C. -R., J; H. 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doi:10.1140/epja/s10050-024-01282-x

Thepurposeofthisdocumentistooutlinethedevelopingsci entific case for pursuing an energy upgrade to 22 GeV of the Continuous Electron Beam Accelerator Facility (CEBAF) at the ThomasJefferson National Accelerator Facility (TJNAF, or JLab). This document was developed with input from a series of workshops held in the period between March 2022 and April 2023 that were organized by the JLab user com munity and staff with guidance from JLab management (see Sect. 10). The scientific case for the 22 GeV energy upgrade leverages existing or already planned Hall equipment and world-wide uniqueness of CEBAF high-luminosity opera tions.

Accardi, A., Achenbach, P., Adhikari, D., Afanasev, A., Akondi, C.s., Akopov, N., et al. (2024). Strong interaction physics at the luminosity frontier with 22 GeV electrons at Jefferson Lab. EUROPEAN PHYSICAL JOURNAL. A, HADRONS AND NUCLEI, 60(9) [10.1140/epja/s10050-024-01282-x].