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The collimator system of a particle accelerator must efficiently remove stray particles and provide protection against uncontrolled losses. In this article, the basic design concepts of collimators and some realizations are presented.

Accelerator Physics · Physics 2013-08-01 Slawomir Wronka

After a brief description of the basic principle of a photon collider, we summarize the physics potential of such a facility at high energies. Unique opportunities are provided in supersymmetric theories for the discovery of heavy scalar…

High Energy Physics - Phenomenology · Physics 2008-11-26 M. M. Muhlleitner , P. M. Zerwas

Long-lived particles have significant enough lifetimes as to, when produced in collisions, leave a distinct signature in the detectors. Driven by increasingly higher energies, trigger and reconstruction algorithms at particle colliders are…

High Energy Physics - Experiment · Physics 2021-09-14 Rebeca Gonzalez Suarez

The need for ever higher energies in lepton colliders gives rise to the investigation of new accelerator schemes for elementary particle physics experiments. One perceivable way to increase the collision energy would be to combine…

High Energy Physics - Phenomenology · Physics 2014-12-30 Sarah J. Müller , Christoph H. Keitel , Carsten Müller

We point out that even the most intense laser beams available today can provide only a very small fraction of the beam energy required to reach the design luminosity for a future e+e- linear collider. This fact seems to have been overlooked…

Accelerator Physics · Physics 2007-05-23 Adrian C. Melissinos

Collimation systems are essential in particle accelerators to safely and efficiently manage unavoidable beam losses during operation. These systems rely on collimators, which are specially designed movable jaws or absorbers positioned close…

Accelerator Physics · Physics 2026-03-05 Nuria Fuster Martínez

Particle accelerators have enabled forefront research in high energy physics and other research areas for more than half a century. Accelerators have directly contributed to 26 Nobel Prizes in Physics since 1939 as well as another 20 Nobel…

Accelerator Physics · Physics 2022-06-20 Javier Resta-López

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

High Energy Physics - Experiment · Physics 2009-10-31 Valery Telnov

A future e+e- Linear Collider has a large physics potential for the discovery of new physics beyond the Standard Model and precision studies of the Standard Model itself. It is well suited to complement and extend the physics program of the…

High Energy Physics - Phenomenology · Physics 2015-06-25 G. Moortgat--Pick , A. Bartl , K. Hidaka , T. Kernreiter , H. Liivat , R. -K. Loide , I. Ots , W. Porod , R. Saar , H. Uibo

For problems in astrophysics, planetary science and beyond, numerical simulations are often limited to simulating fewer particles than in the real system. To model collisions, the simulated particles (aka superparticles) need to be inflated…

Earth and Planetary Astrophysics · Physics 2020-06-03 David Nesvorny , Andrew N. Youdin , Raphael Marschall , Derek C. Richardson

New particle acceleration schemes open up exciting opportunities, potentially providing more compact or higher-energy accelerators. The AWAKE experiment at CERN is currently taking data to establish the method of proton-driven plasma…

Accelerator Physics · Physics 2019-09-04 M. Wing

Muon colliders have a great potential for high-energy physics. They can offer collisions of point-like particles at very high energies, since muons can be accelerated in a ring without limitation from synchrotron radiation. However, the…

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 interaction of the two beams in a collider leads to a variety of effects that may limit the performance of the machine. This lecture introduces the basic aspects necessary to understand the design of modern colliders.

Accelerator Physics · Physics 2025-10-17 Xavier Buffat

These lectures review the main motivations for future high-energy colliders, focusing on the understanding of electroweak symmetry breaking and on the search for physics beyond the Standard Model. The open questions and the challenges are…

High Energy Physics - Phenomenology · Physics 2019-05-21 Michelangelo Mangano

Dark matter is one of the main puzzles in fundamental physics and the goal of a diverse, multi-pronged research program. Underground and astrophysical searches search for dark matter particles in the cosmos, either by interacting directly…

High Energy Physics - Experiment · Physics 2018-06-13 Bjoern Penning

Black holes have sometimes been described as astrophysical particle accelerators because finite energy particles can collide near the horizon with divergent center-of-mass (CM) energy. The collisions are classified by the radial motion of…

General Relativity and Quantum Cosmology · Physics 2025-08-12 Delilah E. A. Gates

A high-energy $e^+e^-$ Linear Collider has been considered since a long time as an important complement to the LHC. Unprecedented precision measurements as well as the exploration of so far untouched phase space for direct production of new…

High Energy Physics - Phenomenology · Physics 2018-09-26 Jenny List , Gudrid Moortgat-Pick , Jürgen Reuter

This article summarizes main developments of the hadron colliders and physics results obtained since their inception around forty years ago. The increase in the collision energy of over two orders of magnitude and even larger increases in…

Accelerator Physics · Physics 2015-06-16 Dmitri Denisov

The acceleration of charged particles at astrophysical collisionless shock waves is one of the best studied processes for the energization of particles to ultrarelativistic energies, required by multifrequency observations in a variety of…

Astrophysics · Physics 2009-11-10 Pasquale Blasi