University of Kentucky

About: University of Kentucky is a education organization based out in Lexington, Kentucky, United States. It is known for research contribution in the topics: Population & Poison control. The organization has 43933 authors who have published 92195 publications receiving 3256087 citations. The organization is also known as: UK.

The evolution of self-control

Abstract: Cognition presents evolutionary research with one of its greatest challenges. Cognitive evolution has been explained at the proximate level by shifts in absolute and relative brain volume and at the ultimate level by differences in social and dietary complexity. However, no study has integrated the experimental and phylogenetic approach at the scale required to rigorously test these explanations. Instead, previous research has largely relied on various measures of brain size as proxies for cognitive abilities. We experimentally evaluated these major evolutionary explanations by quantitatively comparing the cognitive performance of 567 individuals representing 36 species on two problem-solving tasks measuring self-control. Phylogenetic analysis revealed that absolute brain volume best predicted performance across species and accounted for considerably more variance than brain volume controlling for body mass. This result corroborates recent advances in evolutionary neurobiology and illustrates the cognitive consequences of cortical reorganization through increases in brain volume. Within primates, dietary breadth but not social group size was a strong predictor of species differences in self-control. Our results implicate robust evolutionary relationships between dietary breadth, absolute brain volume, and self-control. These findings provide a significant first step toward quantifying the primate cognitive phenome and explaining the process of cognitive evolution.

Comparative localization of serotonin1A, 1C, and 2 receptor subtype mRNAs in rat brain.

Abstract: Serotonin (5-HT) mediates its effects on neurons in the central nervous system through a number of different receptor types. To gain better insight as to the localization of 5-HT responsive cells, the distribution of cells expressing mRNAs encoding the three 5-HT receptor subtypes 1A, 1C, and 2 was examined in rat brain with in situ hybridization using cRNA probes. 5-HT1A receptor mRNA labeling was most pronounced in the olfactory bulb, anterior hippocampal rudiment, septum, hippocampus (dentate gyrus and layers CA1-3), entorhinal cortex, interpeduncular nucleus, and medullary raphe nuclei. 5-HT1C receptor mRNA labeling was the most abundant and widespread of the three 5-HT receptor subtypes examined. Hybridization signal was densest in the choroid plexus, anterior olfactory nucleus, olfactory tubercle, piriform cortex, septum, subiculum, entorhinal cortex, claustrum, accumbens nucleus, striatum, lateral amygdala, paratenial and paracentral thalamic nuclei, subthalamic nucleus, substantia nigra, and reticular cell groups. 5-HT2 receptor mRNA was localized to the olfactory bulb, anterior hippocampal rudiment, frontal cortex, piriform cortex, entorhinal cortex, claustrum, pontine nuclei, and cranial nerve motor nuclei including the oculomotor, trigeminal motor, facial, dorsal motor nucleus of the vagus, and hypoglossal nuclei. The distributions of mRNAs for the three different 5-HT receptor subtypes overlap with regions that bind various 5-HT receptor-selective ligands and are present in nearly all areas known to receive serotonergic innervation. The results of this study demonstrate that neurons which express these 5-HT receptor subtypes are very widespread in the central nervous system, yet possess unique distributions within the rat brain. Moreover, previously unreported regions of 5-HT receptor subtype expression were observed, particularly with the 5-HT2 receptor riboprobe in the brainstem. Finally, several brain areas contain multiple 5-HT receptor subtype mRNAs, which leads to the possibility that individual cells may express more than one 5-HT receptor subtype.

The Search for a Better Treatment for Recurrent Clostridium difficile Disease: Use of High-Dose Vancomycin Combined with Saccharomyces boulardii

Abstract: Recurrent Clostridium difficile disease (CDD) is a difficult clinical problem because antibiotic therapy often does not prevent further recurrences. In a previous study, the biotherapeutic agent Saccharomyces boulardii was used in combination with standard antibiotics and was found to be effective in reducing subsequent recurrences of CDD. In an effort to further refine a standard regimen, we tested patients receiving a regimen of a standard antibiotic for 10 days and then added either S. boulardii (1 g/day for 28 days) or placebo. A significant decrease in recurrences was observed only in patients treated with high-dose vancomycin (2 g/day) and S. boulardii (16.7%), compared with those who received high-dose vancomycin and placebo (50%; ). No serious adverse reactions were observed in these patients. ComP p .05

The AGN-obscuring Torus: The End of the ``Doughnut'' Paradigm?

Abstract: Unified schemes of active galactic nuclei (AGNs) require an obscuring dusty torus around the central engine. The compact sizes (only a few parsecs) determined in recent high-resolution observations require that the obscuring matter be clumpy and located inside the region where the black hole gravity dominates over the galactic bulge. This location is in line with the scenario depicting the torus as the region of the clumpy wind coming off the accretion disk in which the clouds are dusty and optically thick. We study here the outflow scenario within the framework of hydromagnetic disk winds, incorporating the cloud properties determined from detailed modeling of the IR emission from clumpy tori. We find that torus clouds were likely detected in recent water maser observations of NGC 3079. In the wind scenario, the AGN main dynamic channel for release of accreted mass seems to be switching at low luminosities from torus outflow to radio jets. The torus disappears when the bolometric luminosity decreases below ~1042 ergs s-1 because the accretion onto the central black hole can no longer sustain the required cloud outflow rate. This disappearance seems to have been observed in both LINERs and radio galaxies. With further luminosity decrease, suppression of cloud outflow spreads radially inward from the disk's dusty, molecular region into its atomic, ionized zone, resulting in the disappearance of the broad emission-line region at lower luminosities yet to be determined.