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Physics Colloquia
Fridays at 1200hrs
In Newman F
12 October 2007
| The role of the cryosphere in the climate system
Jeff Ridley, the Met Office
Predictions of sea level rise require an understanding the behaviour
of the cryosphere with changing climatic forces and the feedbacks on
the climate system. The cold high latitude ocean is a crucial sink for
atmospheric carbon, and controls the overturning of the deep
ocean. This talk describes how climate models may be used to ascertain
the contribution of ice sheets and glaciers to sea level rise, and
their potential to shut down the ocean conveyor. The impact of natural
variability in regional atmospheric and ocean circulation on high
latitude processes is compared with that of climate feedbacks from sea
ice and cloud. The reduction of uncertainties in sea level rise
prediction requires the development of new physical processes.
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19 October 2007
| From transit spectroscopy to direct detection: a roadmap to exoplanet characterization
Giovanna Tinetti, University College London
In the past decade, more than 250 planets orbiting other stars
(extrasolar planets) were discovered using indirect detection
techniques. Most recent observations of primary and secondary eclipses
with Hubble Space Telescope and Spitzer of transiting extrasolar giant
planets (EGPs), suggest that emitted and transmitted spectra of EGPs
can be used to infer many properties of their atmospheres and internal
structure, including chemical element abundances, cloud/haze optical
properties, temperature-pressure profiles, density and
evolution. Larger and technologically more challenging concept
missions have been proposed to directly detect exoplanets in the near
future. These projects are expected to provide our first opportunity
to study spectroscopically the global characteristics of Super-Earths
and Earth-size planets beyond our solar system, and even search for
signs of habitability and life. To understand our ability to
characterize Giant and Terrestrial exoplanets, we have generated
synthetic planetary spectra (emitted, reflected and transmitted) of
these exotic environments, using a set of chemistry, climate and
radiative transfer models. This presentation will focus on the
detectability of spectral signatures of crucial atmospheric molecules
and surface characteristics with present and future observations.
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26 October 2007
| QED in a Pencil Trace
Kostya Novoselov, University of Manchester
When one writes by a pencil, thin flakes of graphite are left on a
surface. Some of them are only one angstrom thick and can be viewed as
individual atomic planes cleaved away from the bulk. This strictly two
dimensional material called graphene was presumed not to exist in the
free state and remained undiscovered until the last year. In fact,
there exists a whole class of such two-dimensional crystals. In
grapheme, electrons move with little scattering over huge (submicron)
distances as if they were completely insensitive to the environment
only a couple of angstroms away. Moreover, electron transport in
graphene is governed by the Dirac equation so that they mimic
relativistic particles with zero rest mass.
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2 November 2007
| Geometry, light, and a wee bit of magic
Ulf Leonhardt, University of St. Andrews
Invisibility devices, quantum levitation and optical black holes have
something in common: they use the fact that dielectric media act as
effective geometries, changing the way light perceives space and
time. In this lecture, these connections will be elucidated.
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9 November 2007
| Water at model membranes: structure, dynamics and biomolecular sensing
Mischa Bonn, FOM Institute AMOLF, Amsterdam.
The interaction of lipids with water drives the self-assembly process
of biological membranes. It has been a challenge to elucidate the
detailed role of water in biomolecular processes, including those
occurring at the membrane surface. We use surface-specific vibrational
spectroscopies to study the properties of the one molecular layer
water directly interacting with model membranes. Our results reveal
marked differences between membrane-bound water and other types of
interfacial water.
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16 November 2007
| Evidence that Drug Molecules Eat Their Way Through Membranes
Oscar Ces, Imperial College London.
To get to their site of action drug molecules must cross multiple cell
membrane barriers. At present they are believed to do so by one of two
major mechanisms: active or passive translocation. Passive
translocation involves diffusion, with the concentration gradient
across membranes acting as the driving force. Active transport on the
other hand is mediated by special carrier proteins and is of
particular relevance to larger drug molecules. These mechanisms
however are not yet fully understood and do not account for many
experimental observations. This presentation highlights our
observation that one of the largest classes of pharmaceutical drug
molecules, the cationic amphiphilic drugs, or CADs, do so via a novel
mechanism driven by a catalytic reaction that degrades the
membrane. Our results demonstrate that the entire process, from drug
adsorption to drug release within micelles occurs on a timescale of
seconds, compatible with in vivo drug diffusion rates. Given the rate
at which this occurs it is probable that this process is a significant
mechanism for drug transport.
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23 November 2007
| Measuring the electric dipole moment of the neutron - a very small measurement with very big consequences
David Wark, Imperial College London/Rutherford Appleton Laboratory
First pointed out in the 60s, in order to get from a Big Bang of pure
energy to our current universe (which is strongly dominated by matter)
the laws of physics must be different for particles and antiparticles
(a phenomenon called CP violation). IF CP violation exists beyond the
Standard Model, it is quite likely to induce a static electric dipole
moment in the neutron. This talk will discuss this theoretical
background and then concentrate on efforts to observe such an effect
using ultra-cold neutrons. This involves cooling neutrons to a
fraction of a degree Kelvin, at which point they travel at walking
pace, can be controlled with water valves and bath plugs, and stored
in a bottle like milk. The neutrons are then used to make an "atomic
clock", and measurements of shifts in the frequency of that clock when
subjected to a high electric field hold out the promise of finally
giving an answer to the question: Why is the Universe made of matter?
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30 November 2007
| Gravitational Lensing as a Universal Astrophysical Tool: Giant Arcs, Multiple Quasars and Extrasolar Planets
Joachim Wambsganss, Astronomisches Rechen Institut, Heidelberg
Deflection of light by gravity was predicted by Einstein's Theory of
General Relativity and observationally confirmed in 1919. Only in
1979, gravitational lensing became an observational science when the
first doubly imaged quasar was discovered. Today lensing is a booming
part of astrophysics and cosmology. A whole suite of lensing phenomena
have been investigated since: multiple quasars, giant luminous arcs,
quasar microlensing, galactic microlensing, Einstein rings, arclets,
weak gravitational lensing and cosmic shear. The most recent lensing
application is the detection of extrasolar planets. Lensing has
contributed significant new results in areas as different as the
cosmological distance scale, mass determination of galaxy clusters,
physics of quasars, searches for dark matter in galaxy halos,
structure of the Milky Way, stellar atmospheres and exoplanets. A
guided tour through some of these lensing applications will illustrate
that gravitational lensing has established itself as a very useful
universal astrophysical tool.
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ALL
WELCOME
For more details contact
Euan Hendry.
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