In this paper we examine thoroughly the Higgs boson to Ç AE decay via processes involving R parity violating couplings. By means of full one-loop diagrammatic calculations, we found that even if known experimental constraints, particularly including the stringent sub-eV neutrino mass bounds, give strong restrictions on some of the R parity violating parameters, the branching ratio could still achieve notable value in the admissible parameter space. Hence, the flavor violating leptonic decay is of interest to future experiments. We present here key results of our analysis. Based on the analysis, we give some comments on h 0 ! e Ç AE and h 0 ! e Ç AE also.
The ab initio density
matrix renormalization group
(DMRG) method has been well-established and has become one of the
most accurate numerical methods for the precise electronic structure
solution of large active spaces. In the past few years, to capture
the missing dynamic correlation, various post-DMRG approaches have
been proposed through the combination of DMRG and multireference quantum
chemical methods or density functional theory. With this in mind,
this work provides a brief overview of ab initio DMRG
principles and the new developments within post-DMRG methods. For
clarity, post-DMRG methods are classified into two main categories
depending on whether high-order n-electron reduced
density matrices are used, and their merits and disadvantages are
properly discussed. Finally, we conclude by discussing unsolved bottlenecks
and giving development perspectives of post-DMRG approaches, which
are expected to yield quantitative descriptions of complex electronic
structures in large strongly correlated molecules and materials.
The accurate electronic structure calculation for strongly correlated chemical systems requires an adequate description for both static and dynamic electron correlation, and is a persistent challenge for quantum chemistry. In order to account for static and dynamic electron correlations accurately and efficiently, in this work we propose a new method by integrating the density matrix renormalization group (DMRG) method and multi-reference second-order Epstein-Nesbet perturbation theory (ENPT2) with a selected configuration interaction (SCI) approximation. Compared to previous DMRG-based dynamic correlation methods, the DMRG-ENPT2 method extends the range of applicability, allowing us to efficiently calculate systems with very large active spaces beyond 30 orbitals. We demonstrate this by performing calculations on H 2 S with an active space of (16e, 15o), hexacene with an active space of (26e, 26o) and trinuclear Manganese cluster with an active space of (47e, 43o).
In this letter, we report on lepton flavor violating Higgs decay into µ ∓ τ ± in the framework of the generic supersymmetric standard model without R-parity and list interesting combinations of R-parity violating parameters. We impose other known experimental constraints on the parameters of the model and show our results from the R-parity violating parameters. In our analysis, the branching ratio of h 0 → µ ∓ τ ± can exceed 10 −5 within admissible parameter space.
It is thought that the spacetime geometry around black hole candidates is described by the Kerr solution, but an observational confirmation is still missing. Today, the continuum-fitting method and the analysis of the iron Kα line cannot unambiguously test the Kerr paradigm because of the degeneracy among the parameters of the system, in the sense that it is impossible with current X-ray data to distinguish a Kerr black hole from a non-Kerr object with different values of the model parameters. In this paper, we study the possibility of testing the Kerr nature of black hole candidates with X-ray spectropolarimetric measurements. Within our simplified model that does not include the effect of returning radiation, we find that it is impossible to test the Kerr metric and the problem is still the strong correlation between the spin and possible deviations from the Kerr geometry. Moreover, the correlation is very similar to that of the other two techniques, which makes the combination of different measurements not very helpful. Nevertheless, our results cannot be taken as conclusive and, in order to arrive at a final answer, the effect of returning radiation should be properly taken into account.
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