The Lancaster, Manchester, Sheffield Consortium for Fundamental Physics: Particle Physics, From the Universe to the LHC
Lead Research Organisation:
University of Manchester
Department Name: Physics and Astronomy
Abstract
Particle physics is all about understanding the elementary building blocks of nature and their interactions. Over the years, physicists have developed the Standard Model of particle physics, which is extremely successful in describing a very wide range of natural phenomena from things as basic as how light works and why atoms form through to the complicated workings inside stars and the synthesis of nuclei in the first few minutes after the Big Bang. However, we know that the Standard Model is not the whole story for it leaves many questions unanswered. Our proposal focuses on these unanswered questions and the way that scientists hope to address them in the coming years using experiments like the Large Hadron Collider (LHC) or observations like those that will be made using the Planck satellite.
The discovery at the LHC of a Higgs boson is a major milestone in our quest to understand the origin of mass. It is certainly not, however, the whole story. The LHC experiments are working hard to measure the properties of the particle they have discovered. They are also searching for new particles such as those predicted by supersymmetry. If supersymmetry is discovered then it offers the hope to explain the origin of the Dark Matter that makes up a large fraction of the material that is known to exist in the Universe. The scientists in our consortium will explore the theory of supersymmetry and dark matter. We will use data from experiments like the LHC to identify which of the many possible variants of supersymmetry are allowed by the data and to suggest new ways to explore those models in experiments. Any "new physics" produced at the LHC will be produced as a result of smashing two protons into each other, a very complicated environment, usually in association with "jets" of other particles. Members of our consortium will explore how we can make use of these jets to learn more about the associated new physics: the better we understand the environment in which new physics occurs, the more we are able to learn about the new physics itself. This is a complicated business that often necessitates computer simulations of particle collisions. Our members are experts in these simulations and have plans on how the make them more accurate, which is necessary if we are to make the most of the exciting data from the LHC.
The Standard Model of particle physics is also insufficient when it comes to explaining the early history of the Universe, when it was hot and dense. The evidence is now very strong that the history began with an era of accelerating expansion, called inflation. We are experts on inflation and its consequences. Inflation makes the Universe featureless, except for tiny quantum fluctuations that cause the density of matter and energy in the Universe to vary with position. These initially small variations grow to become observable effects. One effect is the formation of the billions of galaxies that populate the night sky. Another is to leave a tiny imprint on the cosmic microwave background radiation (CMB), a faint hum of microwave radiation in which the Universe is bathed. The CMB is being studied in exquisite detail by the Planck satellite, which was launched in 2009. We are at the forefront of interpreting the Planck data in the hope of pinning down which of the various theories of the early universe are ruled out and which remain viable. The deficiencies of the Standard Model extend still further for it does not explain the amount nor even the existence of ordinary matter. Our scientists will use this to constrain possible physics beyond the Standard Model and to do that they need to master the dynamics of the Universe shortly after the end of inflation. Last but not least, we hope to understand better the mysterious "Dark Energy" that drives the current and future acceleration of the Universe: one possibility is that it is because Einstein's theory of gravity is not quite right and that is something we will explore.
The discovery at the LHC of a Higgs boson is a major milestone in our quest to understand the origin of mass. It is certainly not, however, the whole story. The LHC experiments are working hard to measure the properties of the particle they have discovered. They are also searching for new particles such as those predicted by supersymmetry. If supersymmetry is discovered then it offers the hope to explain the origin of the Dark Matter that makes up a large fraction of the material that is known to exist in the Universe. The scientists in our consortium will explore the theory of supersymmetry and dark matter. We will use data from experiments like the LHC to identify which of the many possible variants of supersymmetry are allowed by the data and to suggest new ways to explore those models in experiments. Any "new physics" produced at the LHC will be produced as a result of smashing two protons into each other, a very complicated environment, usually in association with "jets" of other particles. Members of our consortium will explore how we can make use of these jets to learn more about the associated new physics: the better we understand the environment in which new physics occurs, the more we are able to learn about the new physics itself. This is a complicated business that often necessitates computer simulations of particle collisions. Our members are experts in these simulations and have plans on how the make them more accurate, which is necessary if we are to make the most of the exciting data from the LHC.
The Standard Model of particle physics is also insufficient when it comes to explaining the early history of the Universe, when it was hot and dense. The evidence is now very strong that the history began with an era of accelerating expansion, called inflation. We are experts on inflation and its consequences. Inflation makes the Universe featureless, except for tiny quantum fluctuations that cause the density of matter and energy in the Universe to vary with position. These initially small variations grow to become observable effects. One effect is the formation of the billions of galaxies that populate the night sky. Another is to leave a tiny imprint on the cosmic microwave background radiation (CMB), a faint hum of microwave radiation in which the Universe is bathed. The CMB is being studied in exquisite detail by the Planck satellite, which was launched in 2009. We are at the forefront of interpreting the Planck data in the hope of pinning down which of the various theories of the early universe are ruled out and which remain viable. The deficiencies of the Standard Model extend still further for it does not explain the amount nor even the existence of ordinary matter. Our scientists will use this to constrain possible physics beyond the Standard Model and to do that they need to master the dynamics of the Universe shortly after the end of inflation. Last but not least, we hope to understand better the mysterious "Dark Energy" that drives the current and future acceleration of the Universe: one possibility is that it is because Einstein's theory of gravity is not quite right and that is something we will explore.
Planned Impact
See the attached "Pathways to Impact" document for details.
This project has impact beyond the international scientific community mainly through the training of highly skilled graduate students and postdoctoral researchers and through extensive "outreach" activities of various kinds aimed at engaging directly with the general public, school children, teachers, policy makers and the media. Undergraduate teaching is also impacted beneficially by our research.
This project has impact beyond the international scientific community mainly through the training of highly skilled graduate students and postdoctoral researchers and through extensive "outreach" activities of various kinds aimed at engaging directly with the general public, school children, teachers, policy makers and the media. Undergraduate teaching is also impacted beneficially by our research.
Organisations
Publications
Dev P
(2014)
New Production Mechanism for Heavy Neutrinos at the LHC
in Physical Review Letters
Biswas T
(2014)
Atick-Witten Hagedorn conjecture, near scale-invariant matter and blue-tilted gravity power spectrum
in Journal of High Energy Physics
Dev P
(2014)
Constraining non-thermal and thermal properties of Dark Matter
in Frontiers in Physics
Ambrus V
(2015)
Rotating fermions inside a cylindrical boundary
Van De Bruck C
(2015)
Disformally coupled inflation
Choudhury A
(2015)
Less-simplified models of dark matter for direct detection and the LHC
Dasgupta M
(2015)
On jet substructure methods for signal jets
in Journal of High Energy Physics
Ambru? V
(2015)
Renormalised fermion vacuum expectation values on anti-de Sitter space-time
in Physics Letters B
Conroy A
(2015)
Generalized quadratic curvature, non-local infrared modifications of gravity and Newtonian potentials
in Classical and Quantum Gravity
Roszkowski L
(2015)
Prospects for dark matter searches in the pMSSM
in Journal of High Energy Physics
Van De Bruck C
(2015)
Simplest extension of Starobinsky inflation
in Physical Review D
Dev P
(2015)
Flavour effects in Resonant Leptogenesis from semi-classical and Kadanoff-Baym approaches
in Journal of Physics: Conference Series
Kanti P
(2015)
Quantum Aspects of Black Holes
Kowalska K
(2015)
GUT-inspired SUSY and the muon g-2 anomaly: prospects for LHC 14 TeV
Ángeles-Martínez R
(2015)
Coulomb gluons and the ordering variable
in Journal of High Energy Physics
Dasgupta M
(2015)
Small-radius jets to all orders in QCD
in Journal of High Energy Physics
Ponglertsakul S
(2015)
Black hole solutions in Einstein-charged scalar field theory
Faraggi A
(2015)
Extra $$Z^{\prime }$$ Z ' s and $$W^{\prime }$$ W ' s in heterotic-string derived models
in The European Physical Journal C
Bhupal Dev P
(2015)
TeV-scale left-right symmetry and large mixing effects in neutrinoless double beta decay
in Physical Review D
Van De Bruck C
(2015)
Higgs Inflation with a Gauss-Bonnet term in the Jordan Frame
Breen C
(2015)
Vacuum polarization on the brane
Dolan S
(2015)
Bound states of the Dirac equation on Kerr spacetime
in Classical and Quantum Gravity
Dev P
(2015)
TeV Scale Lepton Number Violation and Baryogenesis
Bezrukov F
(2015)
Inflation, LHC and the Higgs boson
in Comptes Rendus. Physique
Bellm J
(2015)
Herwig 7.0 / Herwig++ 3.0 Release Note
Fischer N
(2015)
Measurement of observables sensitive to coherence effects in hadronic Z decays with the OPAL detector at LEP
in The European Physical Journal C
Chakrabortty J
(2015)
Di-photon resonance around 750 GeV: shedding light on the theory underneath
Chatterjee A
(2015)
Bound on largest r ? 0.1 from sub-Planckian excursions of inflaton
in Journal of Cosmology and Astroparticle Physics
Kent C
(2015)
The global rotating scalar field vacuum on anti-de Sitter space-time
in Physics Letters B
Van De Bruck C
(2015)
Stabilizing the Planck mass shortly after inflation
in Physical Review D
De Bruck C
(2015)
Disformal couplings and the dark sector of the universe
in Journal of Cosmology and Astroparticle Physics
Zenaiev O
(2015)
Impact of heavy-flavour production cross sections measured by the LHCb experiment on parton distribution functions at low x PROSA Collaboration
in The European Physical Journal C
Pilaftsis A
(2015)
Mass bounds on light and heavy neutrinos from radiative minimal-flavor-violation leptogenesis
in Physical Review D
Roszkowski L
(2015)
Axino dark matter with low reheating temperature
in Journal of High Energy Physics
Talaganis S
(2015)
Towards understanding the ultraviolet behavior of quantum loops in infinite-derivative theories of gravity
in Classical and Quantum Gravity
Ángeles-Martínez R
(2015)
Coulomb gluons and the ordering variable
Ambrus V
(2015)
Massless rotating fermions inside a cylinder
Van De Bruck C
(2015)
Stabilising the Planck mass shortly after inflation
Dayal P
(2015)
THE QUEST FOR CRADLES OF LIFE: USING THE FUNDAMENTAL METALLICITY RELATION TO HUNT FOR THE MOST HABITABLE TYPE OF GALAXY
in The Astrophysical Journal
Crispino L
(2015)
Scattering from charged black holes and supergravity
Bezrukov F
(2015)
Living beyond the edge: Higgs inflation and vacuum metastability
in Physical Review D
Crispino L
(2015)
Scattering from charged black holes and supergravity
in Physical Review D
Bhupal Dev P
(2015)
Corrigendum to "Flavour covariant transport equations: An application to resonant leptogenesis" [Nucl. Phys. B 886 (2014) 569]
in Nuclear Physics B
Bhupal Dev P
(2015)
Kadanoff-Baym approach to flavour mixing and oscillations in resonant leptogenesis
in Nuclear Physics B
Description | Progress on many fronts towards a better understanding of the universe, by developing theoretical models constrained by data from the LHC and cosmology experiments such as Planck. |
Exploitation Route | By continued research. |
Sectors | Education |
Description | Researchers supported by this award have been very active in outreach activities for the general public, schools and scientists from other fields. |
First Year Of Impact | 2014 |
Sector | Education |
Impact Types | Cultural,Societal |