21,112 research outputs found
Energy transfer calculations for two C-phycocyanins based on refined x-ray crystal structure coordinates of chromophores
Nonequivalent ensembles and metastability
This paper reviews a number of fundamental connections that exist between
nonequivalent microcanonical and canonical ensembles, the appearance of
first-order phase transitions in the canonical ensemble, and thermodynamic
metastable behavior.Comment: 4 pages, RevTeX, 1 figure. Contribution to the Proceedings of the
31st Workshop of the International School of Solid State Physics
``Complexity, Metastability and Nonextensivity'', held at the Ettore Majorana
Foundation and Centre for Scientific Culture, Erice, Sicily, Italy, July
2004. Edited by C. Tsallis, A. Rapisarda and C. Beck. To be published by
World Scientific, 200
Picosecond time-resolved energy transfer kinetics within C-phycocyanin and allophycocyanin aggregates
Coherent anti-Stokes Raman spectroscopy of phycobilisomes, phycocyanin and allophycocyanin from Mastigocladus laminosus
Energy transfer in 'native' and chemically modified C-phyocyanin trimers and the constituent subunits
Energy transfer in C-phycocyanin in different states of aggregation studied by picosecond time-resolved fluorescence
Investigating Bar Structure of Disc Galaxies via PRIMAL: A PaRtIcle-by-particle M2M ALgorithm
We have modified our particle-by-particle adaptation of the made-to-measure
(M2M) method, with the aim of modelling the Galactic disc from upcoming
Galactic stellar survey data. In our new particle-by-particle M2M algorithm,
PRIMAL, the observables of the target system are compared with those of the
model galaxy at the position of the target stars, i.e. particles. The mass of
the model particles are adjusted to reproduce the observables of the target
system, and the gravitational potential is automatically adjusted by the
changing mass of the particles. This paper builds upon our previous work,
introducing likelihood-based velocity constraints in PRIMAL. In this paper we
apply PRIMAL to barred disc galaxies created by a N-body simulation in a known
dark matter potential, with no error in the observables. This paper
demonstrates that PRIMAL can recover the radial profiles of the surface
density, velocity dispersion in the radial and perpendicular directions, and
the rotational velocity of the target discs, along with the apparent bar
structure and pattern speed of the bar, especially when the reference frame is
adjusted so that the bar angle of the target galaxy is aligned to that of the
model galaxy at every timestep.Comment: 13 pages, 10 figures, Accepted 2013 April 16. Received 2013 April 8;
in original form 2013 February
- …
