2,108 research outputs found

    AGN Feedback models: Correlations with star formation and observational implications of time evolution

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    We examine the correlation between the star formation rate (SFR) and black hole accretion rate (BHAR) across a suite of different AGN feedback models, using the time evolution of a merger simulation. By considering three different stages of evolution, and a distinction between the nuclear and outer regions of star formation, we consider 63 different cases. Despite many of the feedback models fitting the M-\sigma\ relationship well, there are often distinct differences in the SFR-BHAR correlations, with close to linear trends only being present after the merger. Some of the models also show evolution in the SFR-BHAR parameter space that is at times directly across the long-term averaged SFR-BHAR correlation. This suggests that the observational SFR-BHAR correlation found for ensembles of galaxies is an approximate statistical trend, as suggested by Hickox et al. Decomposing the SFR into nuclear and outer components also highlights notable differences between models and there is only modest agreement with observational studies examining this in Seyfert galaxies. For the fraction of the black hole mass growth from the merger event relative to the final black hole mass, we find as much as a factor of three variation among models. This also translates into a similar variation in the post-starburst black hole mass growth. Overall, we find that while qualitative features are often similar amongst models, precise quantitative analysis shows there can be quite distinct differences.Comment: Accepted to MNRAS. Comments welcom

    Development and Application of Porphyrin-Maquette Complexes: Towards Artificial Photosynthesis

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    This study looks at developing an artificial reaction centre with photogenerated electron transfer. Naturally occurring photosynthetic reaction centres utilise proteins to house photoactive material, which is coupled with redox enzymes for catalytic reactions to produce chemical fuels. Photosynthetic systems provide inspiration for designing new means to produce renewable energy, whereby sunlight can produce fuels in the form of chemical energy. Artificially designed proteins with synthetically produced porphyrins can potentially be employed to mimic the natural photosynthetic reaction centre for light-induced charge separation. This charge separation is fundamental for conversion of light energy to other forms of energy
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