22,511 research outputs found

    Ethnic minority business in the uk: a review of research and policy development

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    Part of a series produced to support a ESRC/CRE/DTI/emda workshop on ethnic minority entrepreneurship. This paper comprised a review of research literature on ethnic minority enterprise and an overview of UK policy developments

    On sign changes for almost prime coefficients of half-integral weight modular forms

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    For a half-integral weight modular form f=n=1af(n)nk12qnf = \sum_{n=1}^{\infty} a_f(n)n^{\frac{k-1}{2}} q^n of weight k=l+12k = l +\frac{1}{2} on Γ0(4)\Gamma_0(4) such that af(n)a_f(n) (nn \in N\mathbb{N}) are real, we prove for a fixed suitable natural number rr that af(n)a_f(n) changes sign infinitely often as nn varies over numbers having at most rr prime factors, assuming the analog of the Ramanujan conjecture for half-integral weight forms.Comment: To appear in Mathematik

    Falling through the black hole horizon

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    We consider the fate of a small classical object, a "stick", as it falls through the horizon of a large black hole (BH). Classically, the equivalence principle dictates that the stick is affected by small tidal forces, and Hawking's quantum-mechanical model of BH evaporation makes essentially the same prediction. If, on the other hand, the BH horizon is surrounded by a "firewall", the stick will be consumed as it falls through. We have recently extended Hawking's model by taking into account the quantum fluctuations of the geometry and the classical back-reaction of the emitted particles. Here, we calculate the strain exerted on the falling stick for our model. The strain depends on the near-horizon state of the Hawking pairs. We find that, after the Page time when the state of the pairs deviates significantly from maximal entanglement (as required by unitarity), the induced strain in our semiclassical model is still parametrically small. This is because the number of the disentangled pairs is parametrically smaller than the BH entropy. A firewall does, however, appear if the number of disentangled pairs near the horizon is of order of the BH entropy, as implicitly assumed in previous discussions in the literature.Comment: 25 pages, 3 figure
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