Experiential investigation of nonlinear acoustic field structure in two and three dimensions

Author(s):  
Devkan Kaleci ◽  
Ali Sahin ◽  
Baki Karabocu
2000 ◽  
Vol 46 (3) ◽  
pp. 274-283 ◽  
Author(s):  
O. P. Galkin ◽  
E. A. Kharchenko ◽  
L. V. Shvachko

2014 ◽  
Vol 28 ◽  
pp. 1460168 ◽  
Author(s):  
OLIVER PORTH ◽  
SERGUEI S. KOMISSAROV ◽  
RONY KEPPENS

Pulsar wind nebulae (PWN) provide a unique test-bed for the study of highly relativistic processes right at our astronomical doorstep. In this contribution we will show results from the first 3D RMHD simulations of PWN. Of key interest to our study is the long standing "sigma-problem" that challenges MHD models of Pulsars and their nebulae now for 3 decades. Earlier 2D MHD models were very successful in reproducing the morphology of the inner Crab nebula showing a jet, torus, concentric wisps and a variable knot. However, these models are limited to a purely toroidal field geometry which leads to an exaggerated compression of the termination shock and polar jet — in contrast to the observations. In three dimensions, the toroidal field structure is susceptible to current driven instabilities; hence kink instability and magnetic dissipation govern the dynamics of the nebula flow. This leads to a resolution of the sigma-problem once also the pulsar's obliqueness (striped wind) is taken into account. In addition, we present polarized synchrotron maps constructed from the 3D simulations, showing the wealth of morphological features reproduced in 2D is preserved in the 3D case.


2016 ◽  
Vol 80 (10) ◽  
pp. 1197-1202 ◽  
Author(s):  
I. N. Didenkulov ◽  
A. I. Martyanov ◽  
N. V. Pronchatov-Rubtsov

2021 ◽  
Vol 11 (1) ◽  
Author(s):  
M. Arif Hasan ◽  
Keith Runge ◽  
Pierre A. Deymier

AbstractThe possibility of achieving and controlling scalable classically entangled, i.e., inseparable, multipartite states, would fundamentally challenge the advantages of quantum systems in harnessing the power of complexity in information science. Here, we investigate experimentally the extent of classical entanglement in a $$16$$ 16 acoustic qubit-analogue platform. The acoustic qubit-analogue, a.k.a., logical phi-bit, results from the spectral partitioning of the nonlinear acoustic field of externally driven coupled waveguides. Each logical phi-bit is a two-level subsystem characterized by two independently measurable phases. The phi-bits are co-located within the same physical space enabling distance independent interactions. We chose a vector state representation of the $$16$$ 16 -phi-bit system which lies in a $${2}^{16}$$ 2 16 -dimensional Hilbert space. The calculation of the entropy of entanglement demonstrates the possibility of achieving inseparability of the vector state and of navigating the corresponding Hilbert space. This work suggests a new direction in harnessing the complexity of classical inseparability in information science.


Sign in / Sign up

Export Citation Format

Share Document