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Dipesh Bhandari

Publications and source records attributed to Dipesh Bhandari.

4 recordsLinked to original sources

Making Surfaces Biharmonic by Conformal Reparametrization in Anti-de Sitter Three-Space

Harmonic immersions of surfaces are minimal, while biharmonic maps form a fourth-order extension of harmonic-map theory. Because every harmonic map is automatically biharmonic, the basic existence problem is to find \emph{proper} biharmonic maps, namely biharmonic maps that are not harmonic. This paper asks a more geometric question: when can a fixed nondegenerate surface in three-dimensional anti-de Sitter space be made proper biharmonic by changing only the conformal metric on its domain? Equivalently, how much of biharmonicity is determined by the immersed surface, and how much can be created by conformal reparametrization? Writing the induced metric as $g=\lambda^2\bar g$ and introducing the weighted mean curvature $u=\lambda^2H$, we first reduce the map equation to a normal scalar equation coupled to a tangential first-order constraint. The resulting system reveals a sharp rigidity--existence dichotomy. A nonminimal spacelike constant-mean-curvature solution must have constant dilation and is locally the totally umbilical hyperbolic plane of curvature $-2/L^2$. Once the constant-mean-curvature assumption is removed, however, there is an open set of local analytic solutions for which both $H$ and $\lambda$ vary. A moving-frame invariant then identifies the ambient one-parameter symmetry and separates elliptic, hyperbolic, and index-three parabolic orbit types. In the parabolic class the geometric system reduces to a scalar third-order analytic equation, from which we reconstruct explicit local spacelike and real-principal timelike families in null coordinates. The paper therefore locates the rigid branch, proves that the rigidity can be escaped, and gives an explicit mechanism for producing the resulting non-CMC surfaces.

math.DG

Hyperbolic Completion of Newton's Off-Center Orbit Problem: $SO(2,1)$ Symmetry, Inversion Duality, and Magnetic Classification

Which central forces produce circular trajectories whose geometric center differs from the force center? We solve the hyperbolic version of this problem for $$ V(r)=-\frac{\alpha}{(R^2-r^2)^2},\qquad \alpha>0, $$ whose singular circle $r=R$ separates the configuration space into two components. At zero energy, the Jacobi metric is proportional to the Poincar\'e disk metric. Hence every nonradial orbit is an arc of a Euclidean circle orthogonal to $r=R$, while radial orbits lie on lines through the origin. We construct a Runge--Lenz-type vector which, together with angular momentum, defines an on-shell $\mathfrak{so}(2,1)$ moment map. Circular inversion preserves this structure and relates the exterior and punctured-interior flows up to time reparametrization. Although $(r=R)$ is infinitely distant in the Jacobi metric, it is reached in finite Newtonian time. A magnetic deformation corresponds to a constant intrinsic field on the hyperbolic plane and yields an exact circle--horocycle--hypercycle transition at $Q^2=8m\alpha R^2$, with inversion acting as the charge-reversing duality $Q\leftrightarrow -Q$. We also relate the hyperbolic continuum threshold to the Hardy threshold of an inverse-square boundary model.

math-ph

A Kac-Weyl Character Identity

An explicit quantization of Chern-Simons theory leads to an identity between sums of the Kac-Weyl characters. One can use this identity to prove inequalities that constrain the fusion coefficients $N_{\mu\nu}^l$ in the case of RCFTs that descend from current algebras. It also leads to a statement regarding the conjugacy symmetry of the sums of squares of fusion coefficients for current algebras admitting complex representations.

math-ph

Newton's Off-Center Circular Orbits and the Magnetic Monopole

Introducing a radially dependent magnetic field into Newton's off-center circular orbits potential so as to preserve the $E=0$ dynamical symmetry leads to a unique choice of field that can be identified as the inclusion of a magnetic monopole in the inverse stereographically projected problem. One finds also a phenomenological correspondence with that of the linearly damped Kepler model. The presence of the monopole field deforms the symmetry algebra by a central extension, and the quantum mechanical version of this algebra reveals a number of zero modes equal to that counted using the index theorem of elliptic operators.

math-ph