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Anna Escofet

Publications and source records attributed to Anna Escofet.

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Geometric realizations of the Lie superalgebra D(2,1;a)

For every parabolic subgroup $P$ of a Lie supergroup $G$, the homogeneous superspace $G/P$ carries a $G$-invariant supergeometry. We address the question whether $\mathfrak{g}=\text{Lie}(G)$ is the maximal supersymmetry of this supergeometry in the case of the exceptional Lie superalgebra $D(2,1;a)$. For each choice of parabolic $\mathfrak{p}\subset\mathfrak{g}$, we consider the corresponding negatively graded Lie subalgebra $\mathfrak{m}\subset\mathfrak{g}$, and compute its Tanaka--Weisfeiler prolongations, with reduction of the structure group when required, thus realizing $D(2,1;a)$ via symmetries of supergeometries. This gives 6 inequivalent supergeometries: one of these is a vector superdistribution, two are given by cone fields of supervarieties, and the remaining three are higher order structure reductions (a novel feature). We describe those supergeometries and realize $D(2,1;a)$ supersymmetry explicitly in each case.

math.DG

Gauss-Bonnet modified gravity models with bouncing behavior

The following issue is addressed: how the addition of a Gauss-Bonnet term (generically coming from most fundamental theories, as string and M theories), to a viable model, can change the specific properties, and even the physical nature, of the corresponding cosmological solutions? Specifically, brand new original dark energy models are obtained in this way with quite interesting properties, which exhibit, in a unified fashion, the three distinguished possible cosmological phases corresponding to phantom matter, quintessence, and ordinary matter, respectively. A model, in which the equation of state parameter, $w$, is a function of time, is seen to lead either to a singularity of the Big Rip kind or to a bouncing solution which evolves into a de Sitter universe with $w=-1$. Moreover, new Gauss-Bonnet modified gravity models with bouncing behavior in the early stages of the universe evolution are obtained and tested for the validity and stability of the corresponding solutions. They allow for a remarkably natural, unified description of a bouncing behavior at early times and accelerated expansion at present.

gr-qc