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News and Events 2009

News Contents

Events


  • The Elizabeth Spreadbury Lecture
    Weds 25th Mar, 4.30pm, Harrie Massey Lecture Theatre
    Rolf Heuer (Director General of CERN), 'The Large Hadron Collider -  Shedding light on the Dark Universe'
    This lecture is open to members of the public.
  • Physics Colloquium
    Weds 18th Feb 2009, 4pm Harrie Massey Lecture Theatre
    Léon Sanche (University of Sherbrooke), ‘Low Electron Induced Processes in Dielectrics, Icy Satelllites, Stratospheric Clouds, Nanolithograogy and Radiotherapy’.
  • AMOPP Open Day
  • Weds 21st Jan 2009
  • This is an open day for prospective PhD students.


  • MSL workshop; 'Accessing large length and time scales with accurate quantum methods'
  • Mon 12th and Tues 13th Jan 2009.
  • The two-day workshop has been organised to celebrate the career and 65th birthday of Professor Mike Gillan, Professor of Physics and Director of the Materials Simulation Laboratory at UCL, and recipient of the 2006 Institute of Physics Dirac Medal for outstanding contributions to Theoretical Physics.

  • Computational AstroChemistry - a New Era?
    Tues 6th & WedS 7th Jan 2009.

    The huge expansion in the UK's HEI computing power and the recent STFC High Performance Computing award to UCL and Manchester to support Astrochemical data modelling for the JCMT Spectral Line Survey Programme and Herschel Guaranteed Programme Observations have set the scene for a large expansion in the amount and complexity of astrochemical modelling that can now be undertaken.

Call for Fellowship Applications

Please follow the link to apply through the department for a Research Fellowship


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Professor Jonathan Tennyson, Head of Department has been elected to a Fellowship of the Royal Society (FRS).

This great honour recognises not just the enormous technical advances Jonathan has led in high-accuracy calculations of the properties of molecules, but also the influence that his work continues to have across a wide range of physics and astronomy.

To read the award citation please see http://royalsociety.org/publication.asp?id=8521


Excited-state positronium formation from helium, argon and xenon


D.J. Murtagh, D.A. Cooke, G. Laricchia,

Physical Review letters, 102, 133202 (2009)

Paper selected as 'Editors' suggestion'

Positronium is the quasi-stable bound-state of a positron and an electron. It is readily formed in encounters of positrons with matter and its own interactions with atoms and molecules, including its fragmentation and even its combination with another positronium atom, are amenable to experimental investigations. Interest in positronium encompasses the quest for the understanding of fundamental matter/antimatter interactions, tests of collision physics theories and of bound-state QED calculations, the analysis of energetic events occurring in the galactic centre (where it is estimated 93% of all annihilations occur through the decay of Ps) and problems of medical relevance.

Now a team at UCL have measured for the first time the probability for its formation in an excited (2P) state in collisions of positrons with helium, argon and xenon atoms. They measured coincidences between the remnant-ion and the Lyman-alpha photon from positronium and found maximum values to increase from approximately 0.06 ± 0.01 in helium, to 0.12 ± 0.04 in argon and 0.26 ± 0.09 in xenon. These results might have repercussions also in the development of beams of positronium and evaluation of its survival probability in dense media.

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Detection of the transit of the planetary companion to HD 80606

Stephen Fossey, Ingo Waldmann and David Kipping


Paper accepted for publication in Monthly Notices of the RAS Letters.
A preprint is available at www.arxiv.org 

These findings have also been featured in the 'The Times' newspaper at http://www.timesonline.co.uk/tol/news/uk/science/article6135796.ece and on the BBC website- see http://news.bbc.co.uk/1/hi/sci/tech/8020594.stm



We have made one of the first detections of the transit of the extrasolar planet HD 80606b. The planet is unusual in that it has a highly eccentric orbit, which in itself may hold clues as to its origin and orbital evolution. The key observations were made using UCL's observatory (the University of London Observatory) in Mill Hill, NW London, with the direct participation of UCL undergraduates.

The observation of a transit of HD 80606b - its passage in front of the star as seen from Earth - enables a precise determination of its radius, which turns out to be close to that of Jupiter; from its now-resolved mass of 3.9 Jupiter masses, the density of HD 80606b is found to be the amongst the highest of the known transiting planets.

We can also resolve precisely the inclination of the orbit, which turns out to be in a near-grazing configuration (see figure), and the orbital eccentricity is tightly constrained by our data.

Dr. Greg Laughlin, who co-ordinated a global observing campaign on HD 80606b via his web site www.oklo.org, noted on his site, "It's certainly been a long time since an observational astronomical discovery of this magnitude has been made from within the London City Limits."

HD 80606b has the longest period (111 days) for a transiting planet yet discovered, and its orbit is also the most eccentric - it orbits its parent star more like a comet, moving in a couple of months from just inside the 'habitable zone' of its parent star, before plunging close to the star to experience an 800-fold increase in irradiation. This unusual orbit may be due to the influence of other planets in the system, or due to the parent star being part of a binary star system.

The observations at ULO were carried out by UCL undergraduates in a collaboration set up by Dr. Steve Fossey. A 10-hour series of observations was conducted on the night of Feb 13/14, when the transit occurred, by Ingo Waldmann, Maria Duffy, Stephen Fawcett, Yilmaz Gul and Cherry Ng, all undergraduate students taking degrees in the Dept of Physics and Astronomy at UCL, supervised by Steve Fossey.

Ingo Waldmann, a 4th-year Natural Sciences MSci student at UCL, obtained and reduced the observations as part of his final-year project. The final author is Dave Kipping, a postgraduate student at UCL, who developed an eccentric-orbit modelling code which enabled a precise analyis of the transit light curve.

The detection was made using two of ULO's smaller telescopes which are well set up for this kind of photometry - a 35-cm Celestron and a 25-cm Meade telescope. Careful observation, and rigorous calibration and data-reduction procedures, enable us to contribute important results in observational astrophysics, even from London. Our results have provided some of the most precise measurements of the transit yet obtained by astronomers.

Independent detections of the transit of HD 80606b have also been reported  by Moutou et al. and Garcia-Melendo & McCullough (see www.exoplanet.eu for details).


ULO website: www.ulo.ucl.ac.uk

Links to other articles relating to this research

http://www.ulo.ucl.ac.uk/news/index.html#hd80606b-news-reports


For further details on this discovery please see UCL News http://www.ucl.ac.uk/news/news-articles/0903/09030301

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Fig 1:
The geometry of the transit (courtesy of Greg Laughlin (UCSC) www.oklo.org

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FIG 2:
Light curves of exoplanet HD80606b captured at ULO. On the time axis, HJD 2454876.5 corresponds to midnight on Feb 13/14 2009.  (The Meade light curve has been shifted vertically by -0.023 units for clarity.) The brightening of the star by about 1% as the planet completes its transit is clearly detected.


The Computational Power of Correlations

Janet Anders and Dan Browne

Physical Review Letters 102, 050502 (2009)

In this Letter, Anders and Browne study the intrinsic computational power of the correlated outputs of quantum measurements, a phenomenon previously exploited in measurement-based quantum computation (MBQC). Exploiting computational complexity theory, they provide a classification of the computational power of research states for measurement-based quantum computation. This allows the identification of a classical computational analogue of MBQC. Remarkably, this leads, for the first time, to a unified formulation of the Bell inequalities and the Greenberger Horne-Zeilinger effect, two of the most well- studied examples of quantum Physics' incompatibility with a local realistic model of nature. This research opens up the possibility of a more systematic study of the quantum correlations of many-particle systems and gives new insights into the mechanisms through which measurement-based quantum computation obtains its power.

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Nuclear & Particle Physics by Brian Martin

Nuclear & Particle Physics is an introduction to the subject and provides a readable and up-to-date overview of both the theoretical and experimental aspects of nuclear and particle physics, with an emphasis on the phenomenological interpretation of experimental phenomena.

Completely revised, this edition incorporates several new and greatly expanded sections, including additional material on:

• Penning trap measurements of nuclear masses

• nuclear beta decay

• time reversal invariance and tests via measurements of electric dipole moments

• nuclear weapons

• experimental searches for the Higgs boson

• neutrino physics, including oscillation experiments and experiments on neutrinoless double beta decay

• CP violation in the decays of B mesons and consequences for the standard model

• particle astrophysics

There is also a new Appendix on gauge invariance and the Higgs mechanism, tables of data for nuclear and particle physics and additional problems.

This is an invaluable text for all undergraduate physics and astronomy students taking courses in nuclear and particle physics.

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Honours


In the New Years Honours Dr Maggie Aderin (Science and Technology Studies and Visiting Research Fellow- Physics & Astronomy), was made a Member of the Order of the British Empire (MBE) for services to science.


Royal Astronomical Society  Awards

Dr Sarah Bridle and Prof. David Williams have been honoured by the Royal Astronomical Society (RAS) for their outstanding contribution to the field in the society’s allocation of medals for 2009.

Dr Sarah Bridle: The Fowler Award for Astronomy for early career achievements:

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'Dr Bridle has made important contributions to cosmology, in areas ranging from the cosmic microwave background radiation to gravitational lensing and surveys of the redshifts of galaxies. She has completed work on how to maximise the amount of information (and hence progress the field) obtained from the next generation of data sets that will come from instruments such as the Square Kilometre Array (the large radio observatory planned for the next decade). Dr Bridle is honoured in recognition of her status as a young scientist of proven achievement and great promise.'

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Prof. David Williams:

The Gold Medal for Astronomy
'Professor Williams has made seminal contributions to astronomy, particularly in the field of astrochemistry, applying it in progressive phases of star formation, from prestellar objects to protostars to the disks and planets found around young stars. He has also applied this technique in environments found at the end of the lives of stars, from planetary nebulae like the one that will emerge at the end of the Sun’s life to the ejecta from supernova explosions from more massive stars. Professor Williams effectively introduced the field of astrochemistry as a modern discipline to the UK and assembled a community that enabled it to blossom into a major research area.

Professor Williams led research groups in Manchester and London, produced more than 300 publications in refereed journals and numerous books and is a former President of the RAS. He is honoured in recognition of his role as a distinguished scientist, teacher and organiser'


Further details can be read on the UCL news page



Transit timing effects due to an exomoon

David M. Kipping

Monthly Notices of the Royal Astronomical Society, Vol. 392 Issue 1, pp 181 - 189

Also featured as a news item in Nature see http://www.nature.com/news/2009/120109/full/news.2009.16.html

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With over 300 exoplanets now known, the question as to whether such planets harbour moons as become increasingly asked. At the University College London, astronomers have now developed a new method for finding moons by watching the wobble of the host planet.

When an exoplanet transits, astronomers are afforded a brief snapshot of the planet's position and velocity. The presence of a moon around such a planet should cause the planet to wobble, resulting in both position and velocity varying over time. By watching multiple transits David Kipping, of the Dept. of Physics and Astronomy, has shown that these variations can be measured, producing a unique exomoon signature. Furthermore, this signal can be analyzed to determine both the mass and distance of the moon from the planet. The UCL-based work also finds that current telescopes could find Earth-mass moons today and Titan-mass moons in the next few years.

The paper has been accepted for publication in the Monthly Notices of the Royal Astronomical Society.

[Posted 16th Jan. 2009]

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Measurement-based quantum computation

H. J. Briegel, D. E. Browne, W. Dür, R. Raussendorf & M. Van den

Nest
Nature Physics 5, 19- 26 (2009).


Quantum computation offers a promising new kind of information processing, where the non-classical features of quantum mechanics are harnessed and exploited. A number of models of quantum computation exist. These models have been shown to be formally equivalent, but their underlying elementary concepts and the requirements for their practical realization can differ significantly. A particularly exciting paradigm is that of measurement-based quantum computation, where the processing of quantum information takes place by rounds of simple measurements on qubits prepared in a highly entangled state. In this progress article we review recent developments in measurement-based quantum computation with a view to both fundamental and practical issues, in particular the power of quantum computation, the protection against noise (fault tolerance) and steps towards experimental realization.

Finally, we highlight a number of connections between this field and other branches of physics and mathematics.

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