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Dive into the research topics where Greg Landsberg is active.

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Featured researches published by Greg Landsberg.


Physics of the Dark Universe | 2015

Simplified models for dark matter searches at the LHC

J. Abdallah; H.M. Araújo; Alexandre Arbey; A. Ashkenazi; Alexander Belyaev; J. Berger; Celine Boehm; A. Boveia; A. J. Brennan; Jim J Brooke; O. L. Buchmueller; Matthew S. Buckley; Giorgio Busoni; Lorenzo Calibbi; S. Chauhan; Nadir Daci; Gavin Davies; Isabelle De Bruyn; Paul de Jong; Albert De Roeck; Kees de Vries; D. Del Re; Andrea De Simone; Andrea Di Simone; C. Doglioni; Matthew J. Dolan; Herbi K. Dreiner; John Ellis; Sarah Catherine Eno; E. Etzion

This document outlines a set of simplified models for dark matter and its interactions with Standard Model particles. It is intended to summarize the main characteristics that these simplified models have when applied to dark matter searches at the LHC, and to provide a number of useful expressions for reference. The list of models includes both s-channel and t-channel scenarios. For s-channel, spin-0 and spin-1 mediation is discussed, and also realizations where the Higgs particle provides a portal between the dark and visible sectors. The guiding principles underpinning the proposed simplified models are spelled out, and some suggestions for implementation are presented.


Physical Review D | 2001

Higgs boson decays to CP-odd scalars at the Fermilab Tevatron and beyond

Bogdan A. Dobrescu; Greg Landsberg; K. Matchev

In extended Higgs models, the Higgs boson may decay into a pair of light CP-odd scalars, with distinctive collider signatures. We study the ensuing Higgs signals at the upgraded Fermilab Tevatron, considering the subsequent decays of the scalars into pairs of gluons or photons. For CP-odd scalars lighter than a few GeV, the Higgs boson manifests itself as a diphoton resonance and can be discovered up to masses of a few hundred GeV. For heavier CP-odd scalars the reach extends at most up to M{sub h}{approx}120GeV. We also discuss the capabilities of the CERN LHC and lepton colliders in these channels.


Physics of the Dark Universe | 2015

Interplay and Characterization of Dark Matter Searches at Colliders and in Direct Detection Experiments

S. Malik; Christopher McCabe; H.M. Araújo; Alexander Belyaev; Céline Bœhm; Jim J Brooke; O. L. Buchmueller; Gavin Davies; Albert De Roeck; Kees de Vries; Matthew J. Dolan; John Ellis; Malcolm Fairbairn; Henning Flaecher; L. Gouskos; Valentin V. Khoze; Greg Landsberg; Dave M Newbold; Michele Papucci; T. J. Sumner; Marc Thomas; Steven Worm

In this White Paper we present and discuss a concrete proposal for the consistent interpretation of Dark Matter searches at colliders and in direct detection experiments. Based on a specific implementation of simplified models of vector and axial-vector mediator exchanges, this proposal demonstrates how the two search strategies can be compared on an equal footing.


Journal of Physics G | 2006

Black holes at future colliders and beyond

Greg Landsberg

One of the most dramatic consequences of low-scale (~1 TeV) quantum gravity in models with large or warped extra dimension(s) is copious production of mini-black holes at future colliders and in ultra-high-energy cosmic ray collisions. Hawking radiation of these black holes is expected to be constrained mainly to our three-dimensional world and results in rich phenomenology. In this topical review we discuss the current status of astrophysical observations of black holes and selected aspects of mini-black-hole phenomenology, such as production at colliders and in cosmic rays, and black-hole decay properties, Hawking radiation as a sensitive probe of the dimensionality of extra space, as well as an exciting possibility of finding new physics in the decays of black holes.


Modern Physics Letters A | 2012

Vanishing Dimensions and Planar Events at the LHC

Luis Anchordoqui; De-Chang Dai; Malcolm Fairbairn; Greg Landsberg; Dejan Stojkovic

We propose that the effective dimensionality of the space we live in depends on the length scale we are probing. As the length scale increases, new dimensions open up. At short scales the space is lower dimensional; at the intermediate scales the space is three-dimensional; and at large scales, the space is effectively higher dimensional. This setup allows for some fundamental problems in cosmology, gravity, and particle physics to be attacked from a new perspective. The proposed framework, among the other things, offers a new approach to the cosmological constant problem and results in striking collider phenomenology and may explain elongated jets observed in cosmic-ray data.


Classical and Quantum Gravity | 2012

NR/HEP: roadmap for the future

Vitor Cardoso; Leonardo Gualtieri; Carlos Herdeiro; Ulrich Sperhake; Paul M. Chesler; Luis Lehner; S. Park; Harvey S. Reall; Carlos F. Sopuerta; Daniela Alic; Oscar J. C. Dias; Roberto Emparan; Valeria Ferrari; Steven B. Giddings; Mahdi Godazgar; Ruth Gregory; Veronika E. Hubeny; Akihiro Ishibashi; Greg Landsberg; Carlos O. Lousto; David Mateos; Vicki Moeller; Hirotada Okawa; Paolo Pani; M. Andy Parker; Frans Pretorius; Masaru Shibata; Hajime Sotani; Toby Wiseman; Helvi Witek

Physic in curved spacetime describes a multitude of phenomena, ranging from astrophysics to high-energy physics (HEP). The last few years have witnessed further progress on several fronts, including the accurate numerical evolution of the gravitational field equations, which now allows highly nonlinear phenomena to be tamed. Numerical relativity simulations, originally developed to understand strong-field astrophysical processes, could prove extremely useful to understand HEP processes such as trans-Planckian scattering and gauge–gravity dualities. We present a concise and comprehensive overview of the state-of-the-art and important open problems in the field(s), along with a roadmap for the next years.


arXiv: High Energy Physics - Experiment | 2016

Recommendations on presenting LHC searches for missing transverse energy signals using simplified

A. Boveia; William Shepherd; Francesco D'Eramo; Steven Worm; D. Salek; Lian-Tao Wang; Andrea De Simone; Kathryn Zurek; Valentin V. Khoze; Giorgio Busoni; Tristan Du Pree; Albert De Roeck; Matthew J. Dolan; Greg Landsberg; P. Harris; Stephen Mrenna; Steven Lowette; Kai Schmidt-Hoberg; Marie-Helene Genest; Jan Heisig; S. Malik; Suchita Kulkarni; V. Ippolito; Antonio Riotto; P. Pani

This document summarises the proposal of the LHC Dark Matter Working Group on how to present LHC results on


Physical Review Letters | 2002

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Greg Landsberg

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European Physical Journal C | 1995

-channel models of dark matter

D. Alde; Freddy Binon; M. Boutemeur; C. Bricman; S. V. Donskov; M. Gouanere; A. V. Inyakin; V.A. Kachanov; G. V. Khaustov; Edward E.A. Knapp; A. A. Kondashov; A. V. Kulik; Greg Landsberg; A. A. Lednev; V. A. Lishin; J.-P. Peigneux; S. A. Polovnikov; V.A. Polyakov; M. Poulet; Yu.D. Prokoshkin; S. A. Sadovsky; V.D. Samoylenko; P.M. Shagin; A. V. Shtannikov; A. V. Singovsky; Jean-Pierre Stroot; V. P. Sugonyaev

-channel simplified dark matter models and to compare them to direct (indirect) detection experiments.


Journal of High Energy Physics | 2016

Discovering new physics in the decays of black holes.

JiJi Fan; Savvas M. Koushiappas; Greg Landsberg

If the scale of quantum gravity is near a TeV, the CERN Large Hadron Collider (LHC) will be producing one black hole (BH) about every second, thus qualifying as a BH factory. With the Hawking temperature of a few hundred GeV, these rapidly evaporating BHs may produce new, undiscovered particles with masses approximately 100 GeV. The probability of producing a heavy particle in the decay depends on its mass only weakly, in contrast with the exponentially suppressed direct production. Furthermore, backgrounds in the BH sample can be made small. Using the Higgs boson as an example, we show that it may be found at the LHC on the first day of its operation, even with incomplete detectors.

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Edward E.A. Knapp

Los Alamos National Laboratory

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M. Poulet

Stony Brook University

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Freddy Binon

Université libre de Bruxelles

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