Research in Theoretical Astronomy 2009-2014

Lead Research Organisation: University of Cambridge
Department Name: Institute of Astronomy

Abstract

The Institute of Astronomy, Cambridge, is one of the worlds leading research Institutes in Astronomy. It comprises 19 academic staff, 51 postdoctoral research assistants and 52 PhD students, about half of whom work on theoretical astronomy. This grant application is asking for a renewal of the main theoretical rolling grant at the IoA. Over the next five years we will pursue a broad range of theoretical research on the following problems: (i) The Planck satellite is a third generation space satellite dedicated to measuring the temperature and polarization anisotropies in the cosmic microwave background. Planck is scheduled for launch at the end of 2008, some 15 years after it was first proposed to ESA. The years covered by the grant coincide with the peak period for the scientific exploitation of this satellite. PDRA support is requested to work with the Co-Investigators on core science projects. In particular, we are responsible for leading the key analysis of cosmological parameters from Planck and wish to investigate constraints on models of cosmic inflation. Cambridge has a leading role in the Clover polarization experiment and we wish to involve PDRAs in the scientific interpretation of that experiment. (ii) The cosmic microwave background radiation provides us with a picture of the Universe when it was 400,000 years old. At that time, the Universe was filled with a near uniform mixture of hydrogen , helium, dark matter and radiation. We will investigate how the first non-linear structures emerged from this stochastic background. Over the grant period the main emphasis of the research will be to perform hydrodynamic simulations including radiative transfer to model the thermal state of the intergalactic medium and spatially extended Lyalpha emission. We will also extend previous work on the matter power spectrum from the Ly alpha forest to constrain neutrino masses, in combination with data from Planck. (iii) The discovery of large numbers of extrasolar planets has led to enormous interest in theoretical work on the formation of planets. Over the grant period we will pursue a research programme building on expertise in protoplanetary and debris disk evolution. The work will be centred on linking the protoplanetary phase, when discs were gas rich and possible sites of ongoing gaseous planet formation, through to the debris disc phase, when discs were gas poor, dusty structures, with planetesimal bels as possible sites for terrestrial planet formation. (iv) Accretion discs are present in a wide variety of astronomical systems . In particular, accretion onto compact objects such as black holes, neutron stars and white dwarfs produce observational signatures that provide the main scientific justification for X-ray satellites and gravitational wave detectors. Magnetic fields are central to understanding the evolution of accretion discs. We will perform state-of-the-art numerical simulations of magnetised accretion discs to understand their role in accretion disc dynamics and to compute observational signatures. (v) Understanding stellar evolution is essential for the interpretation of all astrophysical systems, from stars in our own Galaxy to the formation of the first non-linear structures in the Universe. Over the next five years we will develop improved models of massive stars as the progenitors of supernovae and gamma-ray bursts. We will also develop fully three-dimensional numerical models of stellar evolution in binary systems, in collaboration with colleagues at Livermore. (vi) Finally, we will pursue two research themes to understand feedback processes in the cores of clusters of galaxies. We will investigate the physics of `emission line filaments', which are still not understood and we will use large numerical simulations to assess the impact of baryonic physics on the use of clusters as cosmological probes (e.g. testing the nature of dark energy.

Publications

10 25 50
publication icon
Booth M (2009) The history of the Solar system's debris disc: observable properties of the Kuiper belt in Monthly Notices of the Royal Astronomical Society

publication icon
Mustill A (2009) Debris disc stirring by secular perturbations from giant planets in Monthly Notices of the Royal Astronomical Society

publication icon
Martin R (2009) The shape of an accretion disc in a misaligned black hole binary in Monthly Notices of the Royal Astronomical Society

publication icon
Church R (2009) Mass transfer in eccentric binaries: the new oil-on-water smoothed particle hydrodynamics technique in Monthly Notices of the Royal Astronomical Society

publication icon
Barnes L (2009) A joint model for the emission and absorption properties of damped Lya absorption systems in Monthly Notices of the Royal Astronomical Society

publication icon
Eldridge J (2009) A new-age determination for ?2 Velorum from binary stellar evolution models in Monthly Notices of the Royal Astronomical Society: Letters

publication icon
Ferrario L (2009) The origin of magnetism on the upper main sequence in Monthly Notices of the Royal Astronomical Society: Letters

publication icon
Viel M (2009) Cosmological and astrophysical constraints from the Lyman a forest flux probability distribution function in Monthly Notices of the Royal Astronomical Society: Letters

publication icon
Wickramasinghe D (2009) Accretion induced collapse of white dwarfs in binary systems and their observational properties in Journal of Physics: Conference Series

publication icon
Raymond S (2009) PLANET-PLANET SCATTERING LEADS TO TIGHTLY PACKED PLANETARY SYSTEMS in The Astrophysical Journal

publication icon
Greaves J (2009) Debris discs around nearby solar analogues in Monthly Notices of the Royal Astronomical Society

publication icon
Wright J (2009) A THIRD GIANT PLANET ORBITING HIP 14810 in The Astrophysical Journal

publication icon
Moeckel N (2009) Does subcluster merging accelerate mass segregation in local clusters? in Monthly Notices of the Royal Astronomical Society

publication icon
Stancliffe R (2009) Modelling the binary progenitor of Supernova 1993J in Monthly Notices of the Royal Astronomical Society

publication icon
Beckwith K (2009) TRANSPORT OF LARGE-SCALE POLOIDAL FLUX IN BLACK HOLE ACCRETION in The Astrophysical Journal

publication icon
Clarke C (2009) Limits on the location of planetesimal formation in self-gravitating protostellar discs in Monthly Notices of the Royal Astronomical Society: Letters

publication icon
Brown M (2009) Impact of modulation on CMB B -mode polarization experiments in Monthly Notices of the Royal Astronomical Society

publication icon
Lestrade J (2009) Search for cold debris disks around M-dwarfs. II in Astronomy & Astrophysics

publication icon
Kennedy G (2009) STELLAR MASS DEPENDENT DISK DISPERSAL in The Astrophysical Journal

publication icon
Veras D (2009) FORMATION, SURVIVAL, AND DETECTABILITY OF PLANETS BEYOND 100 AU in The Astrophysical Journal

publication icon
Smartt S (2009) The death of massive stars - I. Observational constraints on the progenitors of Type II-P supernovae in Monthly Notices of the Royal Astronomical Society

publication icon
Hanson D (2009) CMB lensing and primordial non-Gaussianity in Physical Review D

publication icon
Dodson-Robinson S (2009) THE FORMATION MECHANISM OF GAS GIANTS ON WIDE ORBITS in The Astrophysical Journal

publication icon
Martin R (2009) Supernova kicks and misaligned Be star binaries in Monthly Notices of the Royal Astronomical Society

publication icon
Eldridge J (2009) Spectral population synthesis including massive binaries in Monthly Notices of the Royal Astronomical Society

publication icon
Payne M (2009) Outward migration of terrestrial embryos in binary systems Terrestrial embryo migration around binaries in Monthly Notices of the Royal Astronomical Society

publication icon
Efstathiou G (2009) B-mode detection with an extended planck mission in Journal of Cosmology and Astroparticle Physics

publication icon
Efstathiou G (2009) Impact of Galactic polarized emission on B -mode detection at low multipoles in Monthly Notices of the Royal Astronomical Society

publication icon
Clarke C (2009) Pseudo-viscous modelling of self-gravitating discs and the formation of low mass ratio binaries in Monthly Notices of the Royal Astronomical Society

publication icon
Sijacki D (2009) Growing the first bright quasars in cosmological simulations of structure formation in Monthly Notices of the Royal Astronomical Society

publication icon
Moeckel N (2009) BONDI-HOYLE-LYTTLETON ACCRETION ONTO A PROTOPLANETARY DISK in The Astrophysical Journal

publication icon
Moeckel N (2009) Limits on initial mass segregation in young clusters in Monthly Notices of the Royal Astronomical Society

publication icon
Hanson D (2010) Weak lensing of the CMB in General Relativity and Gravitation

publication icon
Efstathiou G (2010) Large-angle correlations in the cosmic microwave background Large-angle correlations of the CMB in Monthly Notices of the Royal Astronomical Society

publication icon
Hurley J (2010) Formation of binary millisecond pulsars by accretion-induced collapse of white dwarfs in Monthly Notices of the Royal Astronomical Society

publication icon
Wickramasinghe D (2010) Does GD 356 have a terrestrial planetary companion? in Monthly Notices of the Royal Astronomical Society

publication icon
Kotarba H (2010) SIMULATING MAGNETIC FIELDS IN THE ANTENNAE GALAXIES in The Astrophysical Journal

publication icon
Engel H (2010) NGC 6240: merger-induced star formation and gas dynamics in Astronomy & Astrophysics

publication icon
Owen J (2010) Radiation-hydrodynamic models of X-ray and EUV photoevaporating protoplanetary discs in Monthly Notices of the Royal Astronomical Society

 
Description Fundamental contributions to a wide range of problems in theoretical astronomy
Exploitation Route Via publication in academic journals
Sectors Aerospace, Defence and Marine,Other