Theoretical Particle Physics Research
Lead Research Organisation:
University of Oxford
Department Name: Oxford Physics
Abstract
Our overall aim is to elucidate the nature of matter and its fundamental interactions via a variety of phenomenological and theoretical studies. Of crucial importance will be the new results coming from the Large Hadron Collider (LHC) at CERN. The proposed research will improve our ability to predict the effects of the strong interactions (QCD) on the processes that will be studied at the LHC and develop efficient methods to determine the properties of any new states of matter discovered there. Both analytical and numerical methods will be used to study the properties of hadrons, strongly interacting bound states of quarks. Our research will seek to determine what lies beyond the Standard Model of the strong, weak and electromagnetic interactions, with the ultimate goal of providing a fully unified theory, including gravity. The most promising candidate theories will be studied, including Grand and superstring unification and theories with additional space dimensions. Laboratory, astrophysical and cosmological implications will be analysed to determine the most sensitive experimental tests of these theories. We hope these studies will lead to a complete understanding of the origin of mass, including an understanding of the quark, charged lepton and neutrino masses, mixing angles and CP violation, as well as of the nature of dark matter. In addition to having direct relevance to the LHC program, our research will have relevance to present and future neutrino and astroparticle experiments and to astrophysical and cosmological studies. In particular a concerted effort will be made to understand the nature of the dark matter and optimise strategies for detecting both direct and indirect signals. The implications of particle physics models for early universe processed such as inflation will also be studied.
Organisations
Publications
Nason P
(2014)
$$W^+W^-$$ W + W - , $$WZ$$ W Z and $$ZZ$$ Z Z production in the POWHEG-BOX-V2
in The European Physical Journal C
Aartsen M
(2015)
A COMBINED MAXIMUM-LIKELIHOOD ANALYSIS OF THE HIGH-ENERGY ASTROPHYSICAL NEUTRINO FLUX MEASURED WITH ICECUBE
in The Astrophysical Journal
Mertsch P
(2014)
A hadronic explanation of the lepton anomaly
in Journal of Physics: Conference Series
Buchbinder E
(2014)
A heterotic standard model with B - L symmetry and a stable proton
in Journal of High Energy Physics
Ambjørn J
(2014)
A restricted dimer model on a two-dimensional random causal triangulation
in Journal of Physics A: Mathematical and Theoretical
Collaboration T
(2012)
A search for anisotropy in the arrival directions of ultra high energy cosmic rays recorded at the Pierre Auger Observatory
in Journal of Cosmology and Astroparticle Physics
Abreu P
(2011)
Advanced functionality for radio analysis in the Offline software framework of the Pierre Auger Observatory
in Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Gray J
(2013)
All complete intersection Calabi-Yau four-folds
in Journal of High Energy Physics
Aartsen M
(2016)
All-flavour search for neutrinos from dark matter annihilations in the Milky Way with IceCube/DeepCore
in The European Physical Journal C
Abbasi R
(2013)
All-particle cosmic ray energy spectrum measured with 26 IceTop stations
in Astroparticle Physics
Aartsen M
(2017)
All-sky Search for Time-integrated Neutrino Emission from Astrophysical Sources with 7 yr of IceCube Data
in The Astrophysical Journal
Mertsch P
(2014)
AMS-02 data confront acceleration of cosmic ray secondaries in nearby sources
in Physical Review D
IceCube Collaboration
(2012)
An absence of neutrinos associated with cosmic-ray acceleration in ?-ray bursts.
in Nature
Aartsen M
(2016)
AN ALL-SKY SEARCH FOR THREE FLAVORS OF NEUTRINOS FROM GAMMA-RAY BURSTS WITH THE ICECUBE NEUTRINO OBSERVATORY
in The Astrophysical Journal
Gauld R
(2014)
An explicit Z '-boson explanation of the B ? K * µ + µ - anomaly
in Journal of High Energy Physics
Abbasi R
(2013)
An improved method for measuring muon energy using the truncated mean of dE/dx
in Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Abreu P
(2012)
Antennas for the detection of radio emission pulses from cosmic-ray induced air showers at the Pierre Auger Observatory
in Journal of Instrumentation
Giasemidis G
(2013)
Aspects of dynamical dimensional reduction in multigraph ensembles of CDT
in Journal of Physics: Conference Series
March-Russell J
(2012)
Asymmetric dark matter via spontaneous co-genesis
in Journal of Cosmology and Astroparticle Physics
Baryakhtar M
(2013)
Axion mediation
in Journal of High Energy Physics
Abbasi R
(2012)
Background studies for acoustic neutrino detection at the South Pole
in Astroparticle Physics
Fields B
(2014)
Big-Bang Nucleosynthesis
Fields B
(2014)
Big-Bang Nucleosynthesis
in Chin.Phys.
Collaboration T
(2013)
Bounds on the density of sources of ultra-high energy cosmic rays from the Pierre Auger Observatory
in Journal of Cosmology and Astroparticle Physics
Goertz F
(2012)
Bounds on warped extra dimensions from a Standard Model-like Higgs boson
in Physics Letters B
Description | Our overall aim is to elucidate the nature of matter and its fundamental interactions via a variety of phenomenological and theoretical studies. It was anticipated in the proposal that new results coming from the Large Hadron Collider (LHC) at CERN would be of crucial importance and the proposed research was intended to improve our ability to predict the effects of the strong interactions (QCD) on the processes that will be studied at the LHC and develop efficient methods to determine the properties of any new states of matter discovered there. This expectation was more than adequately fulfilled with the discovery of the Higgs boson - responsible for giving mass to all known fundamental particles in the Standard Model of the strong, weak and electromagnetic interactions. Our research also seeks to determine what lies beyond the Standard Model, with the ultimate goal of providing a fully unified theory, including gravity. Experimental progress here has not been as dramatic, in fact the Standard Model has been amazingly successful at explaining all laboratory measurements. Nevertheless there must be new physics, if only to account for the observed universe with its asymmetry between matter and antimatter, preponderance of dark over luminous matter, and inhomogeneities which grow under gravity into the large-scale structure of galaxies, clusters and superclusters ... none of which can be explained in the framework of the Standard Model. We have continued to make progress in studying promising candidate theories, including unified theories and theories with additional space dimensions. |
Exploitation Route | Our work forms part of a collective effort by theoretical physicists all over the world - each generation builds on the work of those who came before. |
Sectors | Education |
URL | http://www2.physics.ox.ac.uk/research/particle-theory |
Description | An innovative website to explain `Why String Theory?' (http://whystringtheory.com/) has received over 100,000 unique visitors. |
Sector | Education |
Impact Types | Cultural |
Description | Consolidated grant |
Amount | £717,699 (GBP) |
Funding ID | ST/P000770/1 |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 10/2017 |
End | 09/2020 |