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How to break the uniqueness of W1,ploc(Ω)Wloc1,p(Ω) -solutions for very singular elliptic problems by non-local terms
(Zeitschrift für angewandte Mathematik und Physik, 2019)
A posteriori error estimates for elliptic problems with Dirac measure terms in weighted spaces
(Edp Sciences, 2014-02)
In this article we develop a posteriori error estimates for second order linear elliptic problems with point sources in two- and three-dimensional domains. We prove a global upper bound and a local lower bound for the error ...
Qualitative properties of ground states for singular elliptic equations with weights
(2006)
In a series of papers the question of uniqueness of radial ground states of the equation Delta u + f(u) = 0 and of various related equations has been studied. It is remarkable that throughout this work (except in very ...
Qualitative properties of ground states for singular elliptic equations with weights
(SPRINGER, 2006-01)
In a series of papers the question of uniqueness of radial ground states of the equation Delta u + f(u) = 0 and of various related equations has been studied. It is remarkable that throughout this work (except in very ...
Functional implications of a singular penguin scapula (Aves, Sphenisciformes) from the Eocene of Antarctica
(Università degli Studi di Milano, 2012-03)
Penguins have peculiar modifications in their skeletal anatomy as a consequence of their extremely specialized diving habit. Morphological specialization is particularly evident in the forelimb. However, the kinematics of ...
A general Trotter-Kato formula for a class of evolution operators
(ACADEMIC PRESS INC ELSEVIER SCIENCE, 2009)
In this article we prove new results concerning the existence and various properties of an evolution system U(A+B)(t, s)0 <= s <= t <= T generated by the sum -(A(t) + B(t)) of two linear, time-dependent, and generally ...
Testing phenomenological and theoretical models of dark matter density profiles with galaxy clusters
(Oxford University PressOxford, 2013)
We use the stacked gravitational lensingmass profile of four high-mass (M 1015M ) galaxy
clusters around z≈0.3 from Umetsu et al. to fit density profiles of phenomenological [Navarro–
Frenk–White (NFW), Einasto, S´ersic, ...