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Related papers: Connecting LHC, ILC, and Quintessence

200 papers

We report the following calculations for a recently proposed bosonic dark matter WIMP with well-defined interactions: (1)~the mass as determined by fitting to the relic abundance; (2)~the current annihilation cross-section for indirect…

High Energy Physics - Phenomenology · Physics 2025-09-10 Bailey Tallman , Jehu Martinez , Rohan Shankar , Kane Rylander , Roland E. Allen

We present a class of dark matter models, in which the dark matter particle is a feebly interacting massive particle (FIMP) produced via the decay of an electrically charged and/or colored parent particle. Given the feeble interaction, dark…

High Energy Physics - Phenomenology · Physics 2019-10-02 G. Bélanger , N. Desai , A. Goudelis , J. Harz , A. Lessa , J. M. No , A. Pukhov , S. Sekmen , D. Sengupta , B. Zaldivar , J. Zurita

The standard paradigm of collisionless cold dark matter is in tension with measurements on large scales. In particular, the best fit values of the Hubble rate $H_0$ and the matter density perturbation $\sigma_8$ inferred from the cosmic…

Cosmology and Nongalactic Astrophysics · Physics 2017-08-10 Zackaria Chacko , Yanou Cui , Sungwoo Hong , Takemichi Okui , Yuhsin Tsai

Weakly Interacting Massive Particles (WIMPs), are a leading candidate for the dark matter that is observed to constitute ~25% of the total mass-energy density of the Universe. The direct detection of relic WIMPs (those produced during the…

Instrumentation and Detectors · Physics 2017-08-23 Tarek Saab

The Large Hadron Collider (LHC) at CERN will provide proton-proton collisions at a centre-of-mass energy of 14 TeV with a design luminosity of 10**34/cm**2/s. The exploitation of the rich physics potential offered by the LHC will be…

High Energy Physics - Experiment · Physics 2007-05-23 Felicitas Pauss , Michael Dittmar

One of the major challenges of modern physics is to decipher the nature of dark matter. Astrophysical observations provide ample evidence for the existence of an invisible and dominant mass component in the observable universe, from the…

Cosmology and Nongalactic Astrophysics · Physics 2015-09-04 Laura Baudis

With the start-up of the LHC, we can hope to find evidences for new physics beyond the Standard Model, and particle candidates for dark matter. Determining the parameters of the full underlying theory will be a long process requiring the…

High Energy Physics - Phenomenology · Physics 2022-03-02 A. Arbey , F. Mahmoudi

Two next-generation high-energy experiments, the Large Hadron Collider (LHC) and the $e^+e^-$ International Linear Collider (ILC), are highly expected to unravel the new structure of matter and forces from the electroweak scale to the TeV…

High Energy Physics - Phenomenology · Physics 2007-11-15 S. Y. Choi

SuperWeakly-Interacting Massive Particles (superWIMPs) produced in the late decays of other particles are well-motivated dark matter candidates and may be favored over standard Weakly-Interacting Massive Particles (WIMPs) by small scale…

High Energy Physics - Phenomenology · Physics 2008-11-26 Jose A. R. Cembranos , Jonathan L. Feng , Arvind Rajaraman , Bryan T. Smith , Fumihiro Takayama

The WIMP "miracle" suggests a new physics threshold ranging from the weak scale up to several tens of TeVs. Obtaining the correct dark matter density in many theories aiming to solve the hierarchy problem may thus require some amount of…

High Energy Physics - Phenomenology · Physics 2014-09-30 Luca Vecchi

The International Linear Collider (ILC) is a proposed electron-positron collider for the centre-of-mass energy range of 200 to 500 GeV and with upgrade options towards 1 TeV. The ILC would be the ideal tool to explore with high precision…

Accelerator Physics · Physics 2013-06-14 Karsten Buesser

Measurement of the integrated luminosity at the International Linear Collider (ILC) will be accomplished by counting the rate of small angle Bhabha scattering events. The physics requirements for ILC set the constraint on the relative…

Instrumentation and Detectors · Physics 2013-01-14 M. Pandurovic , I. Bozovic-Jelisavcic

In these lectures we first concentrate on the cosmological problems which, hopefully, have to do with the new physics to be probed at the LHC: the nature and origin of dark matter and generation of matter-antimatter asymmetry. We give…

Cosmology and Nongalactic Astrophysics · Physics 2015-04-15 V. A. Rubakov

The Large Hadron electron Collider (LHeC) has been designed to push the field of deep inelastic scattering to the high energy and intensity frontier using an intense electron beam with a proton beam from the High Luminosity-Large Hadron…

High Energy Physics - Phenomenology · Physics 2023-05-17 Guo-yuan Huang , Sudip Jana , Alvaro S. de Jesus , Farinaldo S. Queiroz , Werner Rodejohann

The International Linear Collider (ILC) will allow the precise study of $e^{-}e^{+}\rightarrow q\bar{q}$ interactions at different center-of-mass energies from the $Z$-pole to 1 TeV. In this paper, we discuss the experimental prospects for…

High Energy Physics - Phenomenology · Physics 2024-06-03 A. Irles , J. P. Márquez , R. Pöschl , F. Richard , A. Saibel , H. Yamamoto , N. Yamatsu

A robust mechanism was recently proposed in which thermal freeze-out of WIMPs can provide a unified origin of dark matter and baryon abundances in our universe. We point out that this WIMP-triggered baryogenesis mechanism can exhibit a rich…

High Energy Physics - Phenomenology · Physics 2016-12-28 Yanou Cui , Takemichi Okui , Arash Yunesi

Weakly Interacting Massive Particles (WIMPs) are candidates for non-baryonic Dark Matter. WIMPs are supposed to interact with baryonic matter via scattering off nuclei producing a nuclear recoil with energies up to a few 10 keV with a very…

Physics at the Large Hadron Collider (LHC) and the International e+e- Linear Collider (ILC) will be complementary in many respects, as has been demonstrated at previous generations of hadron and lepton colliders. This report addresses the…

High Energy Physics - Phenomenology · Physics 2012-08-27 LC Study Group , G. Weiglein , T. Barklow , E. Boos , A. De Roeck , K. Desch , F. Gianotti , R. Godbole , J. F. Gunion , H. E. Haber , S. Heinemeyer , J. L. Hewett , K. Kawagoe , K. Monig , M. M. Nojiri , G. Polesello , F. Richard , S. Riemann , W. J. Stirling , A. G. Akeroyd , B. C. Allanach , D. Asner , S. Asztalos , H. Baer , M. Battaglia , U. Baur , P. Bechtle , G. Belanger , A. Belyaev , E. L. Berger , T. Binoth , G. A. Blair , S. Boogert , F. Boudjema , D. Bourilkov , W. Buchmuller , V. Bunichev , G. Cerminara , M. Chiorboli , H. Davoudiasl , S. Dawson , S. De Curtis , F. Deppisch , M. A. Diaz , M. Dittmar , A. Djouadi , D. Dominici , U. Ellwanger , J. L. Feng , I. F. Ginzburg , A. Giolo-Nicollerat , B. K. Gjelsten , S. Godfrey , D. Grellscheid , J. Gronberg , E. Gross , J. Guasch , K. Hamaguchi , T. Han , J. Hisano , W. Hollik , C. Hugonie , T. Hurth , J. Jiang , A. Juste , J. Kalinowski , W. Kilian , R. Kinnunen , S. Kraml , M. Krawczyk , A. Krokhotine , T. Krupovnickas , R. Lafaye , S. Lehti , H. E. Logan , E. Lytken , V. Martin , H. -U. Martyn , D. J. Miller , S. Moretti , F. Moortgat , G. Moortgat-Pick , M. Muhlleitner , P. Niezurawski , A. Nikitenko , L. H. Orr , P. Osland , A. F. Osorio , H. Pas , T. Plehn , W. Porod , A. Pukhov , F. Quevedo , D. Rainwater , M. Ratz , A. Redelbach , L. Reina , T. Rizzo , R. Ruckl , H. J. Schreiber , M. Schumacher , A. Sherstnev , S. Slabospitsky , J. Sola , A. Sopczak , M. Spira , M. Spiropulu , Z. Sullivan , M. Szleper , T. M. P. Tait , X. Tata , D. R. Tovey , A. Tricomi , M. Velasco , D. Wackeroth , C. E. M. Wagner , S. Weinzierl , P. Wienemann , T. Yanagida , A. F. Zarnecki , D. Zerwas , P. M. Zerwas , L. Zivkovic

The potential for detecting DM at the Compact Linear Collider (CLIC) is investigated at \mbox{$\sqrt{s}=$ 3 TeV}. The sensitivity of the search is estimated by computing the 95\% confidence level upper limit cross section as a function of…

High Energy Physics - Experiment · Physics 2021-03-16 J-J. Blaising , P. Roloff , A. Sailer , U. Schnoor

The WIMP proposed here yields the observed abundance of dark matter, and is consistent with the current limits from direct detection, indirect detection, and collider experiments, if its mass is $\sim 72$ GeV/$c^2$. It is also consistent…

High Energy Physics - Phenomenology · Physics 2021-08-02 Reagan Thornberry , Maxwell Throm , Gabriel Frohaug , John Killough , Dylan Blend , Michael Erickson , Brian Sun , Brett Bays , Roland E. Allen