Mussafirs of the 21st Century: British South Asian Muslim women, higher education and the changing notions of ‘Britishness’

The South Asian Muslim community in Britain is one that has become increasingly ‘visible’ with what it means to be ‘British Muslim’ remaining a pertinent issue. Given that the British South Asian community is set to grow, it is necessary to engage with this community in order to understand how discourses around gender, ethnicity and identity affect how this community develops. The aim of this research was to engage with specific members of the British South Asian Muslim community, that of women and mothers. In undertaking this research aspects of identity, belonging and citizenship were explored, with particular emphasis placed on discourses around ‘identity’. Drawing on narratives expressed in focus groups and interviews this research analysed and explored the influences of higher education in shaping attitudes towards citizenship and belonging. Higher education was revealed to have a positive impact on Muslim women’s’ lives, whilst identities and the notions of ‘Britishness’ were increasingly areas of intense negotiation

Cosmological solutions with charged black holes

RB aknowledges support from the Higher Education Commission (HEC) of Pakistan, which provided funding to visit QMUL while this work was performed. TC and JD are supported by the STFC

Solution of the Einstein-Maxwell Equations with Anisotropic Negative Pressure as a Potential Model of a Dark Energy Star

We have obtained a new class of solutions for the Einstein-Maxwell field equations for static spherically symmetric spacetimes by considering the negative anisotropic pressures, which represents a potential model of a dark energy star. We take the equation of state pr = −ρ, where pr is the radial pressure and ρ is the density. We have also checked that for these solutions metric coefficients, mass density, radial pressure, transverse pressure, electric field, and current density are well defined for suitable values of the parameters involved in the solution. These exact solutions can be used to develop models of dark energy stellar interiors satisfying all physical constraints except for the causality condition, which cannot be satisfied for the equation of state considered here, and which is arguably not an applicable physical constraint for dark matter/energy.The accepted manuscript in pdf format is listed with the files at the bottom of this page. The presentation of the authors' names and (or) special characters in the title of the manuscript may differ slightly between what is listed on this page and what is listed in the pdf file of the accepted manuscript; that in the pdf file of the accepted manuscript is what was submitted by the author

Cross-correlations between economic policy uncertainty and precious and industrial metals: A multifractal cross-correlation analysis

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