scholarly journals Dirac equation as a quantum walk over the honeycomb and triangular lattices

2018 ◽  
Vol 97 (6) ◽  
Author(s):  
Pablo Arrighi ◽  
Giuseppe Di Molfetta ◽  
Iván Márquez-Martín ◽  
Armando Pérez
2015 ◽  
Vol 2 (3) ◽  
pp. 243-252 ◽  
Author(s):  
Giuseppe Di Molfetta ◽  
Lauchlan Honter ◽  
Ben B. Luo ◽  
Tatsuaki Wada ◽  
Yutaka Shikano

2017 ◽  
Vol 17 (9&10) ◽  
pp. 810-824 ◽  
Author(s):  
Pablo Arrighi ◽  
Stefno Facchini

A discrete-time Quantum Walk (QW) is essentially an operator driving the evolution of a single particle on the lattice, through local unitaries. Some QWs admit a continuum limit, leading to familiar PDEs (e.g. the Dirac equation). Recently it was discovered that prior grouping and encoding allows for more general continuum limit equations (e.g. the Dirac equation in (1+ 1) curved spacetime). In this paper, we extend these results to arbitrary space dimension and internal degree of freedom. We recover an entire class of PDEs encompassing the massive Dirac equation in (3 + 1) curved spacetime. This means that the metric field can be represented by a field of local unitaries over a lattice.


2015 ◽  
Vol 2 (3) ◽  
pp. 253-254
Author(s):  
Giuseppe Di Molfetta ◽  
Lauchlan Honter ◽  
Ben B. Luo ◽  
Tatsuaki Wada ◽  
Yutaka Shikano

Symmetry ◽  
2020 ◽  
Vol 12 (1) ◽  
pp. 128 ◽  
Author(s):  
Quentin Aristote ◽  
Nathanaël Eon ◽  
Giuseppe Di Molfetta

We present the single-particle sector of a quantum cellular automaton, namely a quantum walk, on a simple dynamical triangulated 2 - manifold. The triangulation is changed through Pachner moves, induced by the walker density itself, allowing the surface to transform into any topologically equivalent one. This model extends the quantum walk over triangular grid, introduced in a previous work, by one of the authors, whose space-time limit recovers the Dirac equation in (2+1)-dimensions. Numerical simulations show that the number of triangles and the local curvature grow as t α e − β t 2 , where α and β parametrize the way geometry changes upon the local density of the walker, and that, in the long run, flatness emerges. Finally, we also prove that the global behavior of the walker, remains the same under spacetime random fluctuations.


2013 ◽  
Vol 58 (6) ◽  
pp. 523-533 ◽  
Author(s):  
V.M. Simulik ◽  
◽  
I.Yu. Krivsky ◽  
I.L. Lamer ◽  
◽  
...  

Author(s):  
І. І. Гайсак ◽  
В. С. Морохович

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