000600408 001__ 600408 000600408 005__ 20250715173016.0 000600408 0247_ $$2doi$$a10.1088/1748-0221/18/06/T06001 000600408 0247_ $$2INSPIRETeX$$aSchroeder:2022xdu 000600408 0247_ $$2inspire$$ainspire:2053625 000600408 0247_ $$2arXiv$$aarXiv:2203.08366 000600408 0247_ $$2datacite_doi$$a10.3204/PUBDB-2023-07965 000600408 0247_ $$2altmetric$$aaltmetric:150728253 000600408 0247_ $$2WOS$$aWOS:001026537200006 000600408 0247_ $$2openalex$$aopenalex:W4379016383 000600408 037__ $$aPUBDB-2023-07965 000600408 041__ $$aEnglish 000600408 082__ $$a610 000600408 088__ $$2arXiv$$aarXiv:2203.08366 000600408 1001_ $$0P:(DE-H253)PIP1107017$$aSchroeder, Chris$$b0$$eCorresponding author 000600408 1112_ $$aSnowmass 2021$$cSeattle$$d2022-07-17 - 2022-07-26$$wUnited States 000600408 245__ $$aLinear colliders based on laser-plasma accelerators 000600408 260__ $$aLondon$$bInst. of Physics$$c2023 000600408 3367_ $$2DRIVER$$aarticle 000600408 3367_ $$0PUB:(DE-HGF)8$$2PUB:(DE-HGF)$$aContribution to a conference proceedings$$mcontrib 000600408 3367_ $$2DataCite$$aOutput Types/Journal article 000600408 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1704273786_1788882 000600408 3367_ $$2BibTeX$$aARTICLE 000600408 3367_ $$2ORCID$$aJOURNAL_ARTICLE 000600408 3367_ $$00$$2EndNote$$aJournal Article 000600408 500__ $$aContribution to Snowmass 2021, Accelerator Frontier 000600408 520__ $$aLaser-plasma accelerators are capable of sustainingaccelerating fields of 10–100 GeV/m, 100–1000 times that ofconventional technology and the highest fields produced by any ofthe widely researched advanced accelerator concepts. Laser-plasmaaccelerators also intrinsically accelerate short particle bunches,several orders of magnitude shorter than that of conventionaltechnology, which leads to reductions in beamstrahlung and, hence,savings in the overall power consumption to reach a desiredluminosity. These properties make laser-plasma accelerators apromising accelerator technology for a more compact, less expensivehigh-energy linear collider providing multi-TeV polarized leptons.In this submission to the Snowmass 2021 Accelerator Frontier, wediscuss the motivation for a laser-plasma-accelerator-based linearcollider, the status of the field, and potential linear colliderconcepts up to 15 TeV. We outline the research and developmentpath toward a collider based on laser-plasma accelerator technology,and highlight near-term and mid-term applications of this technologyon the collider development path. The required experimentalfacilities to carry out this research are described. We concludewith community recommendations developed during Snowmass. 000600408 536__ $$0G:(DE-HGF)POF4-621$$a621 - Accelerator Research and Development (POF4-621)$$cPOF4-621$$fPOF IV$$x0 000600408 588__ $$aDataset connected to CrossRef, INSPIRE, Journals: bib-pubdb1.desy.de 000600408 650_7 $$2autogen$$aAccelerator Applications 000600408 650_7 $$2autogen$$aWake-field acceleration (laser-driven, electron-driven) 000600408 693__ $$0EXP:(DE-MLZ)NOSPEC-20140101$$5EXP:(DE-MLZ)NOSPEC-20140101$$eNo specific instrument$$x0 000600408 7001_ $$0P:(DE-H253)PIP1095524$$aAlbert, Félicie$$b1 000600408 7001_ $$0P:(DE-H253)PIP1096246$$aBenedetti, Marc$$b2 000600408 7001_ $$0P:(DE-H253)PIP1100214$$aBromage, Jake$$b3 000600408 7001_ $$0P:(DE-HGF)0$$aBruhwiler, D.$$b4 000600408 7001_ $$0P:(DE-HGF)0$$aBulanov, S. S.$$b5 000600408 7001_ $$0P:(DE-H253)PIP1085227$$aCampbell, Graeme$$b6 000600408 7001_ $$0P:(DE-H253)PIP1101813$$aCook, Cameron John$$b7$$udesy 000600408 7001_ $$0P:(DE-H253)PIP1030930$$aCros, Brigitte$$b8 000600408 7001_ $$0P:(DE-HGF)0$$aDowner, M. C.$$b9 000600408 7001_ $$0P:(DE-HGF)0$$aEsarey, E.$$b10 000600408 7001_ $$0P:(DE-HGF)0$$aFroula, D. H.$$b11 000600408 7001_ $$0P:(DE-H253)PIP1107428$$aFuchs, Maximilian$$b12 000600408 7001_ $$0P:(DE-HGF)0$$aGeddes, C. G. R.$$b13 000600408 7001_ $$0P:(DE-HGF)0$$aGessner, S. J.$$b14 000600408 7001_ $$0P:(DE-H253)PIP1032909$$aGonsalves, Anthony Joseph$$b15 000600408 7001_ $$0P:(DE-HGF)0$$aHogan, M. J.$$b16 000600408 7001_ $$0P:(DE-H253)PIP1032810$$aHooker, Simon$$b17 000600408 7001_ $$0P:(DE-HGF)0$$aHuebl, A.$$b18 000600408 7001_ $$0P:(DE-HGF)0$$aJing, C.$$b19 000600408 7001_ $$0P:(DE-H253)PIP1107507$$aJoshi, Suresh Chandra$$b20 000600408 7001_ $$0P:(DE-H253)PIP1106481$$aKrushelnick, Karl$$b21 000600408 7001_ $$0P:(DE-H253)PIP1087150$$aLeemans, W. P.$$b22 000600408 7001_ $$0P:(DE-HGF)0$$aLehe, R.$$b23 000600408 7001_ $$0P:(DE-H253)PIP1082382$$aMaier, Andre$$b24 000600408 7001_ $$0P:(DE-HGF)0$$aMilchberg, H. M.$$b25 000600408 7001_ $$0P:(DE-HGF)0$$aMori, W. B.$$b26 000600408 7001_ $$0P:(DE-H253)PIP1021445$$aNakamura, Katsuro$$b27 000600408 7001_ $$0P:(DE-H253)PIP1012785$$aOsterhoff, J.$$b28 000600408 7001_ $$0P:(DE-HGF)0$$aPalastro, J. P.$$b29 000600408 7001_ $$0P:(DE-HGF)0$$aPalmer, M.$$b30 000600408 7001_ $$0P:(DE-H253)PIP1030949$$aPoder, K.$$b31 000600408 7001_ $$0P:(DE-HGF)0$$aPower, J. G.$$b32 000600408 7001_ $$0P:(DE-HGF)0$$aShadwick, B. A.$$b33 000600408 7001_ $$0P:(DE-HGF)0$$aTerzani, D.$$b34 000600408 7001_ $$0P:(DE-H253)PIP1093740$$aThevenet, M.$$b35 000600408 7001_ $$0P:(DE-H253)PIP1087744$$aThomas, Andrew$$b36 000600408 7001_ $$0P:(DE-H253)PIP1008661$$avan Tilborg, Jeroen$$b37 000600408 7001_ $$0P:(DE-HGF)0$$aTurner, M.$$b38 000600408 7001_ $$0P:(DE-HGF)0$$aVafaei-Najafabadi, N.$$b39 000600408 7001_ $$0P:(DE-HGF)0$$aVay, J.-L.$$b40 000600408 7001_ $$0P:(DE-H253)PIP1097248$$aZhou, Tao$$b41 000600408 7001_ $$0P:(DE-HGF)0$$aZuegel, J.$$b42 000600408 773__ $$0PERI:(DE-600)2235672-1$$a10.1088/1748-0221/18/06/T06001$$gVol. 18, no. 06, p. 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