Theoretical Particle Physics at the University of Sussex

Lead Research Organisation: University of Sussex
Department Name: Sch of Mathematical & Physical Sciences

Abstract

The proposed research in the Theoretical Particle Physics group at the University of Sussex focuses on three themes: Fundamental forces in extreme conditions. One of the major problems in modern theoretical physics is the extrapolation of physical laws to new length or energy scales. We wish to push our understanding to ever more extreme situations such the collisions of heavy nuclei, the centres of neutron stars, or the very early universe. Our research will develop our theoretical tools and extrapolate the theories of the strong interactions (QCD) and gravity to regimes of high density, of high temperature, and high energy. Particle astrophysics and cosmology Perhaps the most active area of research in the past decade has been at the interface between particle physics and cosmology. In order to understand the history of the universe we must understand physical laws in the first moments of the Big Bang, when temperatures and particle energies were huge. Conversely, by detailed observations of the universe today we can trace back the conditions and make deductions about physical laws at high energies. Our research will tackle three of the three questions about the universe: why is there more matter than antimatter; is there any evidence out there for strings or string theory; and why is the expansion of the universe accelerating. The Terascale and Beyond The Terascale is the frontier of particle physics, where we collide elementary particles with velocities so close to that of light that their effective mass grows by a factor of a billion. At this frontier there are new discoveries to be made, new theories of physics to test. One of the recurring themes in particle physics is the proposition that the universe has more than three space dimensions: there may be more hidden from us either because they are curled up so small we don't notice them, or because we are trapped on a three-dimensional 'surface' in a higher dimensional space. We will work out how to test these these theories at the latest and biggest particle physics laboratory - the Large Hadron Collider, which will start running this year.

Publications

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Archer P (2011) Flavour physics in the soft wall model in Journal of High Energy Physics

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Archer P (2010) Electroweak constraints on warped geometry in five dimensions and beyond in Journal of High Energy Physics

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Basbøll A (2011) Anomaly mediation and cosmology in Journal of High Energy Physics

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Bond A (2017) Theorems for asymptotic safety of gauge theories in The European Physical Journal C

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Bond AD (2017) Asymptotic Safety Guaranteed in Supersymmetry. in Physical review letters

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Borsanyi S (2008) Semiclassical decay of topological defects in Physical Review D

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Borsányi S (2009) Classical field theory with fermions in Nuclear Physics A

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Borsányi S (2009) Low-cost fermions in classical field simulations in Physical Review D

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Falls K (2018) On de Sitter solutions in asymptotically safe $\boldsymbol {f(R)}$ theories in Classical and Quantum Gravity

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Falls K (2018) Asymptotic safety of quantum gravity beyond Ricci scalars in Physical Review D

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Gerwick E (2011) Asymptotic safety and Kaluza-Klein gravitons at the LHC in Physical Review D

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Hindmarsh M (2008) Perturbations and moduli space dynamics of tachyon kinks in Physical Review D

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Hindmarsh M (2011) Covariant closed string coherent states. in Physical review letters

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Hindmarsh M (2014) Improving cosmic string network simulations in Physical Review D

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Hindmarsh M (2016) New Solutions for Non-Abelian Cosmic Strings. in Physical review letters

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Hindmarsh M (2014) Dark matter from decaying topological defects in Journal of Cosmology and Astroparticle Physics

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Hindmarsh M (2012) f ( R ) gravity from the renormalization group in Physical Review D

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Hindmarsh M (2008) Oscillons and domain walls in Physical Review D

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Hindmarsh M (2016) Breaking symmetry, breaking ground in Journal of Physics A: Mathematical and Theoretical

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Hindmarsh M (2009) Abelian Higgs cosmic strings: Small-scale structure and loops in Physical Review D

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Hindmarsh M (2009) Inhomogeneous tachyon condensation in Journal of High Energy Physics

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Hindmarsh M (2011) Asymptotically safe cosmology in Journal of Cosmology and Astroparticle Physics

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Huber S (2008) Gravitational wave production by collisions: more bubbles in Journal of Cosmology and Astroparticle Physics

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Litim D (2011) Ising exponents from the functional renormalization group in Physical Review D

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Litim D (2017) Critical O ( N ) models in the complex field plane in Physical Review D

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Litim DF (2011) Renormalization group and the Planck scale. in Philosophical transactions. Series A, Mathematical, physical, and engineering sciences

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Litim, Daniel F. And Plehn, Tilman (2007) Virtual gravitons at the LHC

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Lizarraga J (2016) New CMB constraints for Abelian Higgs cosmic strings in Journal of Cosmology and Astroparticle Physics

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Lizarraga J (2014) Can topological defects mimic the BICEP2 B-mode signal? in Physical review letters

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Salmi P (2012) Radiation and relaxation of oscillons in Physical Review D

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Saltas I (2011) The dynamical equivalence of modified gravity revisited in Classical and Quantum Gravity

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Skliros D (2011) String vertex operators and cosmic strings in Physical Review D

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Skliros D (2008) Large radius Hagedorn regime in string gas cosmology in Physical Review D

 
Description We made detailed predictions for the Planck satellite of the Cosmic Microwave Background signal produced by cosmic strings. These predictions were used by the Planck collaboration, who found stringent upper limits on the string mass per unit length.

We performed the first systematic study of constraints on theories with extra curved space dimensions, showing how precision W and Z data imposes new limits on the size of the extra dimensions.

We computed quantum gravity corrections to Yang-Mills theories, which describe the strong force, showing that asymptotic freedom (the tendency of the force to get weaker the closer the particles are together) is not substantially affected by gravity corrections.
Exploitation Route The findings continue to generate academic through citations. The non-academic impacts are through talks to schools.
Sectors Education

 
Description Helsinki Visiting Professorship 
Organisation University of Helsinki
Department Department of Physics
Country Finland 
Sector Academic/University 
PI Contribution Collaboration on theory papers, co-supervision of student research.
Collaborator Contribution Collaboration on theory papers HPC resources 20% salary, travel expenses
Impact @article{Hindmarsh:2013xza, author = "Hindmarsh, Mark and Huber, Stephan J. and Rummukainen, Kari and Weir, David J.", title = "{Gravitational waves from the sound of a first order phase transition}", journal = "Phys.Rev.Lett.", volume = "112", pages = "041301", doi = "10.1103/PhysRevLett.112.041301", year = "2014", eprint = "1304.2433", archivePrefix = "arXiv", primaryClass = "hep-ph", reportNumber = "HIP-2013-07-TH", SLACcitation = "%%CITATION = ARXIV:1304.2433;%%", } @article{Figueroa:2012kw, author = "Figueroa, Daniel G. and Hindmarsh, Mark and Urrestilla, Jon", title = "{Exact Scale-Invariant Background of Gravitational Waves from Cosmic Defects}", journal = "Phys.Rev.Lett.", number = "10", volume = "110", pages = "101302", doi = "10.1103/PhysRevLett.110.101302", year = "2013", eprint = "1212.5458", archivePrefix = "arXiv", primaryClass = "astro-ph.CO", SLACcitation = "%%CITATION = ARXIV:1212.5458;%%", } @article{Hindmarsh:2014rka, author = "Hindmarsh, Mark and Rummukainen, Kari and Tenkanen, Tuomas V. I. and Weir, David J.", title = "{Improving cosmic string network simulations}", journal = "Phys.Rev.", volume = "D90", pages = "043539", doi = "10.1103/PhysRevD.90.043539", year = "2014", eprint = "1406.1688", archivePrefix = "arXiv", primaryClass = "hep-lat", reportNumber = "HIP-2014-10-TH", SLACcitation = "%%CITATION = ARXIV:1406.1688;%%", }
Start Year 2012
 
Description Particle Physics Masterclass (Sussex) 
Form Of Engagement Activity Participation in an open day or visit at my research institution
Part Of Official Scheme? No
Geographic Reach Regional
Primary Audience Schools
Results and Impact Acitivities sparked many questions and discussion.

In a survey of year 1 UGs this year, one reported attending the PPMC and being favourably influenced by outreach towards physics and Sussex.
Year(s) Of Engagement Activity 2013,2014
 
Description School visit (Tunbridge Wells) 
Form Of Engagement Activity A talk or presentation
Part Of Official Scheme? No
Geographic Reach Regional
Primary Audience Schools
Results and Impact Questions and discussion.

School asked if current A Level pupils could visit University of Sussex physics department.
Year(s) Of Engagement Activity 2014
 
Description Talk (WP Sussex) 
Form Of Engagement Activity A talk or presentation
Part Of Official Scheme? Yes
Type Of Presentation Keynote/Invited Speaker
Geographic Reach Regional
Primary Audience Schools
Results and Impact 15 pupils attended a talk on my research ("The Sound of the Big Bang")

too early to say
Year(s) Of Engagement Activity 2014
 
Description Talk (public, Sussex) 
Form Of Engagement Activity A talk or presentation
Part Of Official Scheme? No
Type Of Presentation Keynote/Invited Speaker
Geographic Reach Local
Primary Audience Public/other audiences
Results and Impact 300 people (public, colleagues, university students, and school students) attended my professorial inaugural lecture "Gone in a Yoctosecond: a Rough Guide to the Big Bang").

Stream available on Sussex web: http://www.sussex.ac.uk/newsandevents/sussexlectures/2013
Year(s) Of Engagement Activity 2013