The symmetric tensor spherical harmonics (STSH’s) on the N‐sphere (S N ), which are defined as the totally symmetric, traceless, and divergence‐free tensor eigenfunctions of the Laplace–Beltrami (LB) ...

UC, Berkeley. astro-ph and hep-ex and hep-ph and hep-th. ABRACADABRA and CERN-LHC-CMS ...

We construct a potential for Higgs doublets and triplets that preserves ϱ = M 2 w / M 2 w cos 2 θ w =1, allowing the triplets to make the dominant contribution to W and Z boson masses.

We establish the conditions under which a conservation law associated with a non-invertible operator may be realized as a symmetry in quantum mechanics. As established by Wigner, all quantum ...

We present a lattice computation of ππ–scattering in the I = 1 channel with N f = 2 dynamical quark flavours obtained with ensembles bracketing the physical value of the pion mass. Employing a global ...

Data sets were collected with the BESIII detector at the BEPCII collider at the center-of-mass energy of √s = 3.650 GeV during May 2009 and at √s = 3.773 GeV from January 2010 to May 2011. By ...

Current quantum computers are limited by errors, but have not yet achieved the scale required to benefit from active error correction in large computations. ...

Élie Cartan’s “généralisation de la notion de courbure” (1922) arose from a creative evaluation of the geometrical structures underlying both, Einstein’s theory of gravity and the Cosserat brothers ...

It is widely believed that the complete gravitational collapse of a body always results in a black hole (i.e., “naked singularities” can never be produced) a ...

So far, many exotic predictions of Einstein's equations have been corroborated, with one exception: wormholes (WHs). In this work, we analyze an exact solution to the Einstein-Maxwell-Dilaton or ...

Trento U.. astro-ph and gr-qc and hep-ph ...