Events Archive

Jan
30
2014
Driving nanomagnets by spin-polarized currents offers exciting prospects in magnetoelectronics, but the response of the magnet to such currents remains poorly understood. For a single domain ferromagnet, I will show that an averaged equation describing the diffusion of energy on a graph captures the low-damping dynamics of these systems. In particular, I compute the mean times of thermally assisted magnetization reversals in the finite temperature system, giving explicit expressions for the effective energy barriers conjectured to exist. I will then outline the problem of extending the analysis to...
Jan
27
2014
The spectrum of cosmic rays includes the most energetic particles ever observed. The mechanism of their acceleration and their sources are, however, still mostly unknown. Observing astrophysical neutrinos can help solve this problem. Because neutrinos are produced in hadronic interactions and are neither absorbed nor deflected, they will point directly back to their source. This talk will cover searches for high-energy neutrinos (> 100 TeV) at the IceCube neutrino observatory, which have recently produced the first evidence for a flux beyond standard expectations from neutrinos generated in the Earth's atmosphere. This includes the detection of two events with energies above...
Jan
23
2014
A new observational era in gravitational wave astronomy is poised to begin in this decade, with the upcoming start of Advanced LIGO and Advanced Virgo.  These instruments will be capable of the direct detection of gravitational wave transients, which will yield new insights into the engines powering some of the most energetic astrophysical events: the coalescence of neutron star and/or black hole binary systems, core-collapse supernovae, and isolated neutron star instabilities. I will present the path towards this detection using the second generation of gravitational wave interferometers, and summarize the open analysis challenges, prospects for astrophysical inference and the...
Jan
06
2014
Computational modeling of eukaryotic cells moving on substrates is an extraordinarily complex task: many physical processes, such as actin polymerization, action of motors, formation of adhesive contacts concomitant with both substrate deformation and recruitment of actin etc., as well as regulatory pathways are intertwined. Moreover, highly nontrivial cell responses emerge when the substrate becomes deformable and/or heterogeneous. Here we extended a computational model for motile cell fragments, based on an earlier developed phase field approach, to account for...
Dec
02
2013
Cosmic rays are microscopic, charged particles that permanently bombard Earth from outer space. 100 years after their discovery their origin is still a mystery. It is also not clear how cosmic rays can obtain energies that are sometimes billion times larger than what can be produced in the most powerful particle accelerator on Earth, the LHC, where the Higgs particle was discovered last year. Possible particle accelerators that nature provides are very exotic sites in the universe like exploding stars, massive black holes, gamma-ray bursts, and pulsars. To find out more about these...
Nov
23
2013
To accept Special Relativity we give up Absolute Time. What do we give up to accept Quantum Theory?  After all these years Heisenberg's 1925 discovery paper for Quantum Theory is still opaque, in contrast to  Einstein's for Special Relativity. In hindsight, to accept Quantum Theory we must give up the Classical Principle, which is hardly ever even stated, for the Quantum Principle.  Today this is naturally inferred from a well-known polarization study of Malus in 1805.  Problems  like "spooky...

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