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Related papers: The TeV-mass curvaton

200 papers

In this work, we derive lower mass bounds on the Z' gauge boson based on the dilepton data from LHC with 13 TeV of center-of-mass energy, and forecast the sensitivity of the High-Luminosity-LHC with $L=3000 fb^{-1}$, the High-Energy LHC…

High Energy Physics - Phenomenology · Physics 2022-10-05 A. Alves , L. Duarte , S. Kovalenko , Y. M. Oviedo-Torres , F. S. Queiroz , Y. S. Villamizar

We discuss the possibility of realising a multi-component dark matter scenario with widely separated dark matter masses: one having keV scale mass and the other with GeV-TeV scale mass, within the framework of left right symmetric models.…

High Energy Physics - Phenomenology · Physics 2019-05-30 Debasish Borah , Arnab Dasgupta

We show that collisional damping of adiabatic primordial fluctuations yields constraints on the possible range of mass and interaction rates of Dark Matter particles. Our analysis relies on a general classification of Dark Matter…

Astrophysics · Physics 2009-02-20 C. Boehm , P. Fayet , R. Schaeffer

Diboson resonance with mass of $1.8-2$ TeV is reported successively by CMS and ATLAS experiments in proton-proton collisions at $\sqrt{s}=8$ TeV. We investigate the potentiality of Higgs singlet as the TeV resonance. The challenges of low…

High Energy Physics - Phenomenology · Physics 2015-12-30 Chuan-Hung Chen , Takaaki Nomura

We explore the cosmological consequences of kinetically mixed dark photons with a mass between 1 MeV and 10 GeV, and an effective electromagnetic fine structure constant as small as $10^{-38}$. We calculate the freeze-in abundance of these…

High Energy Physics - Phenomenology · Physics 2014-09-05 Anthony Fradette , Maxim Pospelov , Josef Pradler , Adam Ritz

The growth rate of matter perturbation and the expansion rate of the Universe can be used to distinguish modified gravity and dark energy models in explaining cosmic acceleration. We explore here the inclusion of spatial curvature into the…

Cosmology and Nongalactic Astrophysics · Physics 2009-09-02 Yungui Gong , Mustapha Ishak , Anzhong Wang

Quark-quark and quark-lepton searches for compositenss at the Fermilab Tevatron are summarized. These are of the contact-interaction variety where sqrt(s-hat) < the hypothesized mass scales, Lambda. Tevatron experiments limit a variety of…

High Energy Physics - Experiment · Physics 2007-05-23 J. Andrew Green

We survey the phenomenological constraints on abelian gauge bosons having masses in the MeV to multi-GeV mass range (using precision electroweak measurements, neutrino-electron and neutrino-nucleon scattering, electron and muon anomalous…

High Energy Physics - Phenomenology · Physics 2015-05-27 M. Williams , C. P. Burgess , Anshuman Maharana , F. Quevedo

Leptoquarks in the mass range of 500-1000 GeV can be resonantly produced in significant numbers by PeV neutrino interacting with nuclei at IceCube. We compute the event rates of leptoquark production and decay events and use the 3-year…

High Energy Physics - Phenomenology · Physics 2016-05-10 Ujjal Kumar Dey , Subhendra Mohanty

The physical mechanism behind the TeV gamma-ray source observed at the centre of the Galaxy is still unknown. One intriguing possibility is that the accretion flow onto the central supermassive black hole is responsible for accelerating…

High Energy Astrophysical Phenomena · Physics 2015-05-19 D. R. Ballantyne , M. Schumann , B. Ford

We extract the total width of the top quark, Gamma_t, from the partial decay width Gamma(t -> W b) measured using the t-channel cross section for single top quark production and from the branching fraction B(t -> W b) measured in ttbar…

High Energy Physics - Experiment · Physics 2016-08-14 V. M. Abazov , B. Abbott , M. Abolins , B. S. Acharya , M. Adams , T. Adams , G. D. Alexeev , G. Alkhazov , A. Altona , G. Alverson , G. A. Alves , L. S. Ancu , M. Aoki , Y. Arnoud , M. Arov , A. Askew , B. Åsman , O. Atramentov , C. Avila , J. BackusMayes , F. Badaud , L. Bagby , B. Baldin , D. V. Bandurin , S. Banerjee , E. Barberis , P. Baringer , J. Barreto , J. F. Bartlett , U. Bassler , V. Bazterra , S. Beale , A. Bean , M. Begalli , M. Begel , C. Belanger-Champagne , L. Bellantoni , S. B. Beri , G. Bernardi , R. Bernhard , I. Bertram , M. Besançon , R. Beuselinck , V. A. Bezzubov , P. C. Bhat , V. Bhatnagar , G. Blazey , S. Blessing , K. Bloom , A. Boehnlein , D. Boline , T. A. Bolton , E. E. Boos , G. Borissov , T. Bose , A. Brandt , O. Brandt , R. Brock , G. Brooijmans , A. Bross , D. Brown , J. Brown , X. B. Bu , D. Buchholz , M. Buehler , V. Buescher , V. Bunichev , S. Burdinb , T. H. Burnett , C. P. Buszello , B. Calpas , E. Camacho-Pérez , M. A. Carrasco-Lizarraga , B. C. K. Casey , H. Castilla-Valdez , S. Chakrabarti , D. Chakraborty , K. M. Chan , A. Chandra , G. Chen , S. Chevalier-Théry , D. K. Cho , S. W. Cho , S. Choi , B. Choudhary , T. Christoudias , S. Cihangir , D. Claes , J. Clutter , M. Cooke , W. E. Cooper , M. Corcoran , F. Couderc , M. -C. Cousinou , A. Croc , D. Cutts , M. Ćwiok , A. Das , G. Davies , K. De , S. J. de Jong , E. De La Cruz-Burelo , F. Déliot , M. Demarteau , R. Demina , D. Denisov , S. P. Denisov , S. Desai , K. DeVaughan , H. T. Diehl , M. Diesburg , A. Dominguez , T. Dorland , A. Dubey , L. V. Dudko , D. Duggan , A. Duperrin , S. Dutt , A. Dyshkant , M. Eads , D. Edmunds , J. Ellison , V. D. Elvira , Y. Enari , S. Eno , H. Evans , A. Evdokimov , V. N. Evdokimov , G. Facini , T. Ferbel , F. Fiedler , F. Filthaut , W. Fisher , H. E. Fisk , M. Fortner , H. Fox , S. Fuess , T. Gadfort , A. Garcia-Bellido , V. Gavrilov , P. Gay , W. Geist , W. Geng , D. Gerbaudo , C. E. Gerber , Y. Gershtein , G. Ginther , G. Golovanov , A. Goussiou , P. D. Grannis , S. Greder , H. Greenlee , Z. D. Greenwood , E. M. Gregores , G. Grenier , Ph. Gris , J. -F. Grivaz , A. Grohsjean , S. Grnendahl , M. W. Grünewald , F. Guo , J. Guo , G. Gutierrez , P. Gutierrez , A. Haasc , S. Hagopian , J. Haley , L. Han , K. Harder , A. Harel , J. M. Hauptman , J. Hays , T. Head , T. Hebbeker , D. Hedin , H. Hegab , A. P. Heinson , U. Heintz , C. Hensel , I. Heredia-De La Cruz , K. Herner , G. Hesketh , M. D. Hildreth , R. Hirosky , T. Hoang , J. D. Hobbs , B. Hoeneisen , M. Hohlfeld , S. Hossain , Z. Hubacek , N. Huske , V. Hynek , I. Iashvili , R. Illingworth , A. S. Ito , S. Jabeen , M. Jaffré , S. Jain , D. Jamin , R. Jesik , K. Johns , M. Johnson , D. Johnston , A. Jonckheere , P. Jonsson , J. Joshi , A. Justed , K. Kaadze , E. Kajfasz , D. Karmanov , P. A. Kasper , I. Katsanos , R. Kehoe , S. Kermiche , N. Khalatyan , A. Khanov , A. Kharchilava , Y. N. Kharzheev , D. Khatidze , M. H. Kirby , J. M. Kohli , A. V. Kozelov , J. Kraus , A. Kumar , A. Kupco , T. Kurča , V. A. Kuzmin , J. Kvita , S. Lammers , G. Landsberg , P. Lebrun , H. S. Lee , S. W. Lee , W. M. Lee , J. Lellouch , L. Li , Q. Z. Li , S. M. Lietti , J. K. Lim , D. Lincoln , J. Linnemann , V. V. Lipaev , R. Lipton , Y. Liu , Z. Liu , A. Lobodenko , M. Lokajicek , P. Love , H. J. Lubatti , R. Luna-Garciae , A. L. Lyon , A. K. A. Maciel , D. Mackin , R. Madar , R. Magaña-Villalba , S. Malik , V. L. Malyshev , Y. Maravin , J. Martínez-Ortega , R. McCarthy , C. L. McGivern , M. M. Meijer , A. Melnitchouk , D. Menezes , P. G. Mercadante , M. Merkin , A. Meyer , J. Meyer , N. K. Mondal , G. S. Muanza , M. Mulhearn , E. Nagy , M. Naimuddin , M. Narain , R. Nayyar , H. A. Neal , J. P. Negret , P. Neustroev , S. F. Novaes , T. Nunnemann , G. Obrant , J. Orduna , N. Osman , J. Osta , G. J. Otero y Garzón , M. Owen , M. Padilla , M. Pangilinan , N. Parashar , V. Parihar , S. K. Park , J. Parsons , R. Partridgec , N. Parua , A. Patwa , B. Penning , M. Perfilov , K. Peters , Y. Peters , G. Petrillo , P. Pétroff , R. Piegaia , J. Piper , M. -A. Pleier , P. L. M. Podesta-Lermaf , V. M. Podstavkov , M. -E. Pol , P. Polozov , A. V. Popov , M. Prewitt , D. Price , S. Protopopescu , J. Qian , A. Quadt , B. Quinn , M. S. Rangel , K. Ranjan , P. N. Ratoff , I. Razumov , P. Renkel , P. Rich , M. Rijssenbeek , I. Ripp-Baudot , F. Rizatdinova , M. Rominsky , C. Royon , P. Rubinov , R. Ruchti , G. Safronov , G. Sajot , A. Sánchez-Hernández , M. P. Sanders , B. Sanghi , A. S. Santos , G. Savage , L. Sawyer , T. Scanlon , R. D. Schamberger , Y. Scheglov , H. Schellman , T. Schliephake , S. Schlobohm , C. Schwanenberger , R. Schwienhorst , J. Sekaric , H. Severini , E. Shabalina , V. Shary , A. A. Shchukin , R. K. Shivpuri , V. Simak , V. Sirotenko , P. Skubic , P. Slattery , D. Smirnov , K. J. Smith , G. R. Snow , J. Snow , S. Snyder , S. Söldner-Rembold , L. Sonnenschein , A. Sopczak , M. Sosebee , K. Soustruznik , B. Spurlock , J. Stark , V. Stolin , D. A. Stoyanova , E. Strauss , M. Strauss , D. Strom , L. Stutte , P. Svoisky , M. Takahashi , A. Tanasijczuk , W. Taylor , M. Titov , V. V. Tokmenin , D. Tsybychev , B. Tuchming , C. Tully , P. M. Tuts , L. Uvarov , S. Uvarov S. Uzunyan , R. Van Kooten , W. M. van Leeuwen , N. Varelas , E. W. Varnes , I. A. Vasilyev , P. Verdier , L. S. Vertogradov , M. Verzocchi , M. Vesterinen , D. Vilanova , P. Vint , P. Vokac , H. D. Wahl , M. H. L. S. Wang , J. Warchol , G. Watts , M. Wayne , M. Weberg , L. Welty-Rieger , M. Wetstein , A. White , D. Wicke M. R. J. Williams , G. W. Wilson , S. J. Wimpenny , M. Wobisch , D. R. Wood , T. R. Wyatt , Y. Xie , C. Xu , S. Yacoob , R. Yamada , W. -C. Yang , T. Yasuda , Y. A. Yatsunenko , Z. Ye , H. Yin , K. Yip , H. D. Yoo , S. W. Youn , J. Yu , S. Zelitch , T. Zhao , B. Zhou , J. Zhu , M. Zielinski , D. Zieminska , L. Zivkovic

TeV-scale dark matter is well motivated by notions of naturalness as the new physics threshold is expected to emerge in the TeV regime. We extend the Standard Model by adding an arbitrary SU(2) dark matter multiplet in non-chiral…

High Energy Physics - Phenomenology · Physics 2022-11-23 Ramtin Amintaheri

Light Dark Matter (DM), defined here as having a mass between 1 MeV and about 1 GeV, is an interesting possibility both theoretically and phenomenologically, at one of the frontiers of current progress in the field of DM searches. Its…

High Energy Physics - Phenomenology · Physics 2022-07-06 Marco Cirelli , Nicolao Fornengo , Bradley J. Kavanagh , Elena Pinetti

It is shown that, for a nontrivial radiative decay channel of the 17-keV neutrino, the photons would distort the microwave background radiation through ionization of the universe. The constraint on the branching ratio of such decays from…

Astrophysics · Physics 2009-10-22 Biman B. Nath

We show that the late-decaying particle scenario may be realized in the supersymmetric singlet majoron model with the majoron scale $10-200$ TeV. The smajoron decaying into two neutrinos is the late-decaying particle with the mass $0.1-1$…

High Energy Physics - Phenomenology · Physics 2009-10-28 E. J. Chun

We review the experimental limits on mass of excited fundamental particles and contact interaction energy scale parameters $\Lambda$ for QCD, QED and electroweak reactions. In particular we have focused on the QED reaction $ \EEGG $ at the…

High Energy Physics - Phenomenology · Physics 2009-11-07 Irina Dymnikova , Juergen Ulbricht , Jiawei Zhao

We calculate the scattering rate of sub-GeV dark matter in solid-state targets for spin-dependent dark matter -- nucleon interactions. For dark matter particles with mass below 100 MeV, the scattering occurs predominantly through incoherent…

High Energy Physics - Phenomenology · Physics 2025-06-16 Stefania Gori , Simon Knapen , Tongyan Lin , Pankaj Munbodh , Bethany Suter

We provide a model in which both the inflaton and the curvaton are obtained from within the minimal supersymmetric Standard Model, with known gauge and Yukawa interactions. Since now both the inflaton and curvaton fields are successfully…

High Energy Physics - Phenomenology · Physics 2012-03-14 Anupam Mazumdar , Seshadri Nadathur

Inflating curvaton can create curvature perturbation when the curvaton density is slowly varying. Using the delta-N formalism, we discuss the evolution of the curvature perturbation during curvaton inflation and find analytic formulation of…

High Energy Physics - Phenomenology · Physics 2013-06-26 Seishi Enomoto , Kazunori Kohri , Tomohiro Matsuda

Gravitational positivity bounds are constraints on a renormalizable theory in the presence of a massless graviton, under the assumption that the gravitational theory is ultraviolet-completed by a perturbative string theory. We derive these…

High Energy Physics - Phenomenology · Physics 2026-04-14 Kimiko Yamashita