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Liverpool, United Kingdom

Liverpool John Moores University is a new university located in the city of Liverpool, England. The university is named after businessman and philanthropist John Moores, and was previously called Liverpool Mechanics' School of Arts and later Liverpool Polytechnic before gaining university status in 1992, thus becoming Liverpool John Moores University.The university is a member of the University Alliance, a mission group of British universities established in 2007. It is also a member of the European University Association and the North West Universities Association. At present, LJMU serves more than 24,000 students comprising 20,410 undergraduate students and 4,270 postgraduate students, making it the largest university in Liverpool by student population – as well as the twentieth largest in the United Kingdom. Wikipedia.


Wainwright M.,Liverpool John Moores University
Journal of Antimicrobial Chemotherapy | Year: 2012

Given the problem of increasing antimicrobial-especially antibacterial-drug resistance and the paucity of new agents, it is sensible to consider alternative approaches to infection control to aid in conservation. Photoantimicrobials are highly active agents, regardless of the conventional drug resistance status of the intended organism. Their use in infection control, via topical or local treatment protocols, has thus far received far from proper assessment and requires a wider audience. © The Author 2012. Published by Oxford University Press on behalf of the British Society for Antimicrobial Chemotherapy. All rights reserved. Source


Lees A.,Liverpool John Moores University
Journal of sports sciences | Year: 2010

Kicking is the defining action of soccer, so it is appropriate to review the scientific work that provides a basis of our understanding of this skill. The focus of this review is biomechanical in nature and builds on and extends previous reviews and overviews. While much is known about the biomechanics of the kicking leg, there are several other aspects of the kick that have been the subject of recent exploration. Researchers have widened their interest to consider the kick beginning from the way a player approaches the ball to the end of ball flight, the point that determines the success of the kick. This interest has encapsulated characteristics of overall technique and the influences of the upper body, support leg and pelvis on the kicking action, foot-ball impact and the influences of footwear and soccer balls, ball launch characteristics and corresponding flight of the ball. This review evaluates these and attempts to provide direction for future research. Source


Richter M.,Liverpool John Moores University
Ear and Hearing | Year: 2016

A common element of the psychophysiological research on listening effort is the focus on listening demand as determinant of effort. The article discusses preceding studies and theorizing on effort to show that the link between listening demand and listening effort is moderated by various variables. Moreover, I will present a recent study that examined the joint effect of listening demand and success importance on effort-related cardiovascular reactivity in an auditory discrimination task. Results for pre-ejection period reactivity-an indicator of sympathetic activity-supported the hypothesis that the relationship between listening demand and listening effort is moderated by other variables: Pre-ejection period reactivity was higher in the high-demand-highsuccess-importance condition than in the other three conditions. This new finding as well as the findings of previous research on effort suggest that a broader perspective on the determinants of listening effort is warranted. © Copyright 2016 Wolters Kluwer Health. Source


Longmore S.N.,Liverpool John Moores University
Monthly Notices of the Royal Astronomical Society: Letters | Year: 2015

To explain the observed anomalies in stellar populations within globular clusters, many globular cluster formation theories require two independent episodes of star formation. A fundamental prediction of these models is that the clusters must accumulate large gas reservoirs as the raw material to form the second stellar generation. We show that young clusters containing the required gas reservoir should exhibit the following observational signatures: (i) a dip in the measured luminosity profile or an increase in measured reddening towards the cluster centre, with AV > 10 mag within a radius of a few pc; (ii) bright (sub)mm emission from dust grains; (iii) bright molecular line emission once the gas is dense enough to begin forming stars. Unless the initial mass function is anomalously skewed towards low-mass stars, the clusters should also show obvious signs of star formation via optical emission lines (e.g. Hα) after the stars have formed. These observational signatures should be readily observable towards any compact clusters (radii of a few pc) in the nearby Universe with masses ≳106 M⊙ and ages ≲100 Myr. This provides a straightforward way to directly test globular cluster formation models which predict large gas reservoirs are required to form the second stellar generation. The fact that no such observational evidence exists calls into question whether such a mechanism happens regularly for young massive clusters in galaxies within a few tens of Mpc. © 2015 The Authors. Source


Parker R.J.,Liverpool John Moores University
Monthly Notices of the Royal Astronomical Society | Year: 2014

The initial density of individual star-forming regions (and by extension the birth environment of planetary systems) is difficult to constrain due to the 'density degeneracy problem': an initially dense region expands faster than a more quiescent region due to two-body relaxation and so two regions with the same observed present-day density may have had very different initial densities. We constrain the initial densities of seven nearby star-forming regions by folding in information on their spatial structure from the Q-parameter and comparing the structure and present-day density to the results of N-body simulations. This in turn places strong constraints on the possible effects of dynamical interactions and radiation fields from massive stars on multiple systems and protoplanetary discs.We apply our method to constrain the initial binary population in each of these seven regions and show that the populations in only three-the Orion Nebula Cluster, σ Oph, and Corona Australis-are consistent with having evolved from the Kroupa universal initial period distribution and a binary fraction of unity. © 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. Source

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