English
Related papers

Related papers: Plasma Lens Backgrounds at a Future Linear Collide…

200 papers

The sensitivity of astronomical X-ray detectors is limited by the instrumental background. The background is especially important when observing low surface brightness sources that are critical for many of the science cases targeted by…

Instrumentation and Methods for Astrophysics · Physics 2022-08-18 D. R. Wilkins , S. W. Allen , E. D. Miller , M. Bautz , T. Chattopadhyay , R. Foster , C. E. Grant , S. Hermann , R. Kraft , R. G. Morris , P. Nulsen , G. Schellenberger

Particle accelerators for high energy physics will generate TeV-scale particle beams in large, multi-Km size machines colliding high brightness beams at the interaction point [1-4]. The high luminosity in such machines is achieved by…

The 4th generation light source has achieved tremendous success and leveraged scientific research in material science, biology and chemistry fundamentally. This paper discussed progress in LCLS as introduction and the possibility of…

Accelerator Physics · Physics 2018-08-13 S. Kumar

This report on Photon Colliders briefly reviews three main issues: physics motivation, possible parameters and technical feasibility, plans of works and international cooperation. New scheme of laser optics at the interaction region is…

High Energy Physics - Experiment · Physics 2011-01-13 Valery Telnov

Our beam-beam parameter study using beam-beam simulations and PWFA (particle-driven plasma acceleration) beam parameters indicates that at 3 TeV, for examined electron beam lengths ${2~\mu\mathrm{m}\leq\sigma_z\leq 10~\mu\mathrm{m}}$, the…

Accelerator Physics · Physics 2020-10-05 Jian Bin Ben Chen , Daniel Schulte , Erik Adli

The International Linear Collider is a planned electron-positron linear collider with its positron source producing positrons by aiming undulator radiation onto a rotating target. The resulting, highly divergent positron beam requires…

Accelerator Physics · Physics 2023-09-06 M. Formela , N. Hamann , G. Moortgat-Pick , G. Loisch , M. Mewes , M. Thévenet , J. Osterhoff , G. Boyle

In this paper we describe a method of luminosity measurement at the future linear collider ILC that estimates and corrects for the impact of the dominant sources of systematic uncertainty originating from the beam-induced effects and the…

Accelerator Physics · Physics 2015-06-15 I. Bozovic-Jelisavcic , S. Lukic , G. Milutinovic Dumbelovic , M. Pandurovic , I. Smiljanic

Last two years were very important in history of a photon colliders. This option is included now in conceptual design reports of the NLC, JLC and TESLA/SBLC projects. All the designs foresee two interaction regions: one for e+e- and the…

Accelerator Physics · Physics 2008-02-03 Valery Telnov

Using the laser backscattering method at future TeV linear colliders one can obtain gamma-gamma and electron-gamma colliding beams (photon colliders) with the energy and luminosity comparable to that in e+e- collisions. Now this option is…

Accelerator Physics · Physics 2015-06-26 Valery Telnov

Plasma wakefield acceleration (PWFA) holds much promise for advancing the energy frontier because it can potentially provide a 1000-fold or more increase in acceleration gradient with excellent power efficiency in respect with standard…

In this paper we review the physics opportunities at linear $e^+e^-$ colliders with a special focus on high centre-of-mass energies and beam polarisation, take a fresh look at the various accelerator technologies available or under…

High Energy Physics - Experiment · Physics 2025-12-24 H. Abramowicz , E. Adli , F. Alharthi , M. Almanza-Soto , M. M. Altakach , W. Altmannshofer , S. Ampudia Castelazo , D. Angal-Kalinin , J. A. Anguiano , R. B. Appleby , O. Apsimon , A. Arbey , F. Arco , O. Arquero , A. Aryshev , S. Asai , D. Attie , J. L. Avila-Jimenez , H. Baer , J. A. Bagger , Y. Bai , I. R. Bailey , C. Balazs , P. Bambade , T. Barklow , J. Baudot , P. Bechtle , T. Behnke , A. B. Bellerive , S. Belomestnykh , Y. Benhammou , J. Berenguer-Antequera , M. Berger , M. Berggren , M. Bertucci , M. Besancon , D. Bett , P. -C. Bhat , T. Biekoetter , S. Bilanishvili , B. Bilki , B. Bilki , J. Bjorklund Svensson , V. M. Bjelland , C. Blanch , B. Bliewert , M. Boehler , S. Boogert , M. Boronat , V. Boudry , D. Bourilkov , I. Bozovic , J. Braathen , J. E. Brau , C. Breuning , J. -C. Brient , I. Brock , B. Brudnowski , K. Buesser , E. Bulyak , P. N. Burrows , G. Burt , O. Cakir , A. Caldwell , A. C. Canbay , F. G. Celiberto , E. Cenni , I. Chaikovska , R. Chehab , G. Chen , J. B. B. Chen , T. Chikamatsu , V. Cilento , P. Colas , M. Coman , L. Corner , F. Cornet , F. Cornet-Gomez , F. Corriveau , R. Corsini , J. Cvach , R. D'Arcy , C. Damerell , A. Das , S. Dasu , J. de Blas , E. Del Core , M. Demarteau , H. Denizli , R. Dermisek , A. Dhar , S. Dittmaier , F. Djurabekova , E. M. Donegani , A. Doyle , P. Drobniak , T. A. du Pree , B. Dudar , H. Duran Yildiz , G. Durieux , J. Dutta , S. Easo , G. Eckerlin , U. Einhaus , C. Emma , E. Esarey , D. Esperante , D. Espriu , L. R Evans , J. Farmer , A. Faus Golfe , M. Fernandez , J. C. Fernandez-Ortega , M. Formela , A. Formenti , L. J. Forrester , B. Foster , N. Fourches , M. C. Fouz , A. Freitas , C. D. Fu , K. Fujii , J. Fujimoto , B. Fuks , J. Fuster , N. Fuster-Martinez , M. Gabelmann , F. Gaede , M. Galletti , E. Gallo , S. Ganjour , M. V. Garzelli , R. L. Geng , S. Gessner , I. D. Gialamas , B. Gimeno , J. Goldstein , M. Goncerz , A. J. Gonsalves , F. J. Gonzalez , D. Gonzalez-Iglesias , S. Gori , J. Grames , P. Grannis , L. Gray , G. Grenier , H. Guler , H. E. Haber , K. Hamaguchi , N. Hamann , O. Hartbrich , N. M. Hartman , G. Huetsi , S. Heinemeyer , G. Heinrich , C. Hensel , K. Hidaka , S. Hirose , A. H. Hoang , M. J. Hogan , W. Hollik , Y. Horii , R. Hosokawa , S. Huang , D. Hynds , M. I. Idzik , S. Iguro , Y. Iiyama , K. Ikematsu , A. Irles , A. Ishikawa , M. Ishino , I. P. Ivanov , Y. Iwashita , M. Jacewicz , R. Jaramillo , D. Jeans , C. Jing , R. M Jones , W. Kaabi , M. Kagan , J. Kalinowski , D. K Kalvik , J. Kaminski , S. Kanemura , K. Kannike , A. Karam , Y. Kato , K. Kawagoe , D. Kaefer , L. Kennedy , J. Kersten , S. A. Khan , V. A. Khoze , W. Kilian , J. Klamka , P. Kluit , K. Kong , P. Koppenburg , A. Korsun , A. V. Kotwal , S. Kraml , K. Krueger , K. Kubo , T. Kubo , M. Kucharczyk , S. Kuday , A. Kumar , N. Kumar , M. Kurata , Y. Kurihara , M. Kuriki , J. Kvasnicka , K. Kyoya , I. Laktineh , A. Latina , F. LeDiberder , A. Levy , M. Liepe , C. A. Lindstroem , J. List , B. List , M. Litos , V. N. Litvinenko , A. Lopez-Virto , X. Lu , T. Luo , M. Lupberger , B. Madison , T. Madlener , J. Maeda , F. Mahmoudi , E. Maina , N. Majernik , R. Margraf-O'Neal , T. W. Markiewicz , P. Martin-Luna , A. Martens , V. J. Martin , L. Marzola , V. I. Maslov , K. T. Matchev , S. Matsumoto , K. Mawatari , J. P. Marquez , M. M. Muehlleitner , A. McIlvenny , P. A. McIntosh , K. Mekala , D. Melini , F. Meloni , A. Menandez , S. Michizono , K. Mimasu , V. Miralles , W. Mitaroff , V. A. Mitsou , L. Monaco , G. Moortgat-Pick , M. Moreno-Llcer , T. Mori , J. M. Moron , S. Morton , D. Moya , M. Mulder , P. Munbodh , H. Murayama , E. Musumeci , V. V. Mytrochenko , N. Nagata , E. Nagy , T. Nakada , J. Nakajima , K. Nakamura , E. A. Nanni , E. Nardi , S. Narita , M. T. Nunez Pardo de Vera , M. Nojiri , D. Ntounis , A. Ody , O. M. Ogreid , T. Ohl , Y. Okada , C. Oleari , M. Olvegard , M. Omet , T. Omori , Y. Onel , H. Ono , W. Ootani , C. Orero , J. Osborne , K. Osterberg , J. Osterhoff , M. Ouchemhou , Q. Ouyang , S. Pagan Griso , R. Paparella , S. C. Park , J. Pata , J. R. Patterson , R. Poeschl , F. Pena , L. K Pedraza-Motavita , M. E. Peskin , F. Pilat , P. Piot , S. Plaetzer , I. Polak , W. Porod , K. Potamianos , C. T. Potter , P. Poulose , J. G. Power , D. Protopopescu , H. R. Qi , J. Rabara Bailey , A. Racioppi , M. Raidal , J. P. Ralston , A. Rastogi , L. Reichenbach , L. Reichwein , L. Reina , J. Reuter , F. Richard , S. Riemann , R. A. Rimmer , T. Robens , A. Robson , G. Rodrigo , C. S. Rogan , J. Rojo , M. Q. Ruan , S. Rudrabhatla , A. Ruiz Jimeno , T. Saeki , H. Sakai , Y. Sakaki , F. Salvatore , T. Sanuki , S. Sasikumar , T Schoerner , A. Scheinker , C. B. Schroeder , S. Schroeder , I. Schulthess , M. Schumacher , A. Schwartzman , Y. Seiya , A. Senol , H. Sert , D. Sertore , A. Seryi , T. Shidara , K. Sjobak , I. Smiljanic , S. Spannagel , M. Spira , M. Stanitzki , S. Stapnes , D. Storey , J. Strube , S. Su , A. Subba , A. Subba , T. Suehara , H. Sugawara , K. Sugizaki , Z. Sun , R. Szafron , T. Takahashi , T. Takeshita , T. Tauchi , G. Taylor , N. Terunuma , D. Terzani , T. Teubner , J. Tian , J. Timmermans , M. Titov , R. Tomas Garcia , T. Tong , J. M. Torndal , M. Trautwein , A. Tricoli , K. Tsumura , B. Tuchming , D. Tuckler , I. Turk Cakir , M. Tytgat , A. Ukleja , C. Vallee , R. Van Kooten , J. van Tilborg , A. Vauth , M. Vellasco , C. Vernieri , L. Verra , M. Vicente Barreto Pinto , I. Vidakovic , H. Videau , E. Viklund , I. Vila , M. Villaplana , M. Vos , N. Vukasinovic , N. Walker , K. Wandall-Christensen , Y. Wang , B. F. L. Ward , Z. Was , T. Watanabe , N. K. Watson , G. Weiglein , J. D. Wells , H. Wennloef , M. Wenskat , S. Westhoff , J. W. Wetzel , A. P. White , P. H. Williams , M. Williams , G. W. Wilson , M. Wing , M. Winter , A. Winter , T. Wojton , J. C. Wood , W. Wuensch , X. Xia , K. Yagyu , K. Yamamoto , Y. Yamamoto , H. Yamamoto , A. Yamamoto , S. Yamashita , M. Yamauchi , K. Yokoya , M. Yoshioka , J. Zalesak , A. F. Zarnecki , K. Zembaczynski , D. Zerwas , J. Zhang , Y. Zhang , W. Zhang , Y. -M. Zhong , M. Zielinski , M. Zobov

The dense beams used at CLIC to achieve a high luminosity will cause a large amount of background particles through beam-beam interactions. Generator level studies with GuineaPig and full detector simulation studies with an ILD based CLIC…

Instrumentation and Detectors · Physics 2010-06-18 André Sailer

The existence of dark matter is currently one of the strongest motivations for physics beyond the standard model. Its implications for future colliders are discussed. In the case of neutralino dark matter, cosmological bounds do not provide…

High Energy Physics - Phenomenology · Physics 2009-10-31 Jonathan L. Feng

We quantify the discovery potential of future multi-TeV plasma wakefield colliders for new electroweak multiplets. We include beam-beam effects through realistic luminosity spectra, comparing five collider configurations: $e^+e^-$ and…

High Energy Physics - Phenomenology · Physics 2025-12-12 So Chigusa , Simon Knapen , Toby Opferkuch , Inbar Savoray , Christiane Scherb , Weishuang Linda Xu

Multi-TeV center of mass energy ep colliders based on the Future Circular Collider (FCC) and linear colliders (LC) are proposed and corresponding luminosity values are estimated. Parameters of upgraded versions of the FCC are determined to…

Accelerator Physics · Physics 2016-02-10 Y. C. Acar , U. Kaya , B. B. Oner , S. Sultansoy

Plasma acceleration has emerged as a promising technology for future particle accelerators, particularly linear colliders. Significant progress has been made in recent decades toward high-efficiency and high-quality acceleration of…

Accelerator Physics · Physics 2024-03-06 G. J. Cao , C. A. Lindstrøm , E. Adli , S. Corde , S. Gessner

Photon colliders (gamma-gamma, gamma-e) are based on backward Compton scattering of laser light off the high energy electrons of linear colliders. Recent study has shown that the gamma-gamma luminosity in the high energy peak can reach…

High Energy Physics - Experiment · Physics 2009-11-07 Valery Telnov

Positron sources are the key elements for the future and current lepton collider projects such as ILC, CLIC, SuperKEKB, FCC-ee, Muon Collider/LEMMA, etc., introducing challenging critical requirements for high intensity and low emittance…

Future linear $e^+e^-$ colliders aim for extremely high precision measurements. To achieve this, not only excellent detectors and well controlled machine conditions are needed, but also the best possible estimate of backgrounds. To avoid…

High Energy Physics - Experiment · Physics 2022-09-21 Mikael Berggren

In future normal-conducting linear colliders, the beams will be delivered in short bursts with a length of the order of 100 ns. The pulses will be separated by several ms. In order to maintain high luminosity, feedback is necessary on a…

Accelerator Physics · Physics 2007-05-23 D. Schulte