1,343 research outputs found

    How effective is stretching in maintaining range of movement for children with cerebral palsy?

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    YesBackground: Cerebral Palsy (CP) is the most common childhood disorder affecting four percent of children born in the UK. It is common for children with CP to have reduced range of movement (ROM) due to spasticity and contractures. Stretching is commonly used in physiotherapy programmes to manage this. Aim: This critical review aims to evaluate the evidence base behind the use of stretching for children with CP. Methods: A systematic literature search of AMED, CINAHL, MEDLINE and Cochrane Library Trials was conducted. Returned searches were assessed against strict criteria according to a predefined PICOS (Population, Intervention, Comparison, Outcome, Study). These studies were then critically appraised to assess the validity, reliability and clinical relevance. Findings: There is evidence supporting the use of stretching in children with CP. However there is also some evidence to suggest very little or no positive change. All of the included studies have methodological limitations, which questions the validity of the results. Conclusions/Recommendations: The research suggests some positive outcomes for the use of stretching in CP, studies that did not find positive outcomes found no adverse effects; however further research in the area is required to validate the effectiveness of stretching to maintain ROM in children with CP

    Very Cold Gas and Dark Matter

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    We have recently proposed a new candidate for baryonic dark matter: very cold molecular gas, in near-isothermal equilibrium with the cosmic background radiation at 2.73 K. The cold gas, of quasi-primordial abundances, is condensed in a fractal structure, resembling the hierarchical structure of the detected interstellar medium. We present some perspectives of detecting this very cold gas, either directly or indirectly. The H2_2 molecule has an "ultrafine" structure, due to the interaction between the rotation-induced magnetic moment and the nuclear spins. But the lines fall in the km domain, and are very weak. The best opportunity might be the UV absorption of H2_2 in front of quasars. The unexpected cold dust component, revealed by the COBE/FIRAS submillimetric results, could also be due to this very cold H2_2 gas, through collision-induced radiation, or solid H2_2 grains or snowflakes. The Îł\gamma-ray distribution, much more radially extended than the supernovae at the origin of cosmic rays acceleration, also points towards and extended gas distribution.Comment: 16 pages, Latex pages, crckapb macro, 3 postscript figures, uuencoded compressed tar file. To be published in the proceeedings of the "Dust-Morphology" conference, Johannesburg, 22-26 January, 1996, D. Block (ed.), (Kluwer Dordrecht
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