Macroinstability and Perturbation in Turbulent Stirred Tank Flows

Impeller stirred tank reactors (STRs) are commonly used in the chemical processing industries for a variety of mixing and blending technologies. In this research, a numerical study of flow and mixing inside turbulently agitated STRs are carried out. An immersed boundary method (IBM) is utilized to represent moving impeller geometries in the background of multi-block structured curvilinear fluid. The IBM This curvilinear-IBM methodology is further combined with the large eddy simulation (LES) technique to address the issue of modeling unsteady turbulent flows in the STR. Verification of the combined IBM-LES implementation strategy in curvilinear coordinates is done through comparisons with the measurements of laminar and turbulent flows in baffled STRs with pitched blade impellers. Flow structures are studied inside a dished bottom pitched-blade baffled for different impeller rotational speeds in the turbulent regime to observe the formation of trailing edge vortices which are associated with higher levels of turbulent kinetic energy relative to the remaining flowfield. Instabilities occurring at a frequency lower than the frequency of impeller rotation are identified from the time signal of velocity components. The role of these low frequency macro-instabilities (MI) is explored by observing changes in the three-dimensional circulation pattern within the STR. Significant amount of kinetic energy is observed to be associated with the dynamics of the trailing edge vortices during MI cycles. Flow inside an unbaffled Rushton impeller STR is perturbed using time-dependent impeller rotational speeds at a dominant MI frequency. Perturbation increased the mean radial width of the impeller jet-stream and enhanced overall turbulent kinetic energy compared to the constant rotational speed cases. Large-scale periodic velocity fluctuations due to perturbations produced large strain rates favoring higher turbulence production. Fluctuations in power consumptions are shown to correlate with the perturbation amplitude. Study on the mixing of a passive scalar inside STR showed that the growth rate of unmixed tracer is influenced by the MI oscillations. Perturbation of the STR flow resulted into significant reduction of mixing time. The spatio-temporal behavior of the large-scale mixing structures revealed that fast mixing is promoted due to the break-up of unmixed segregated zones during a perturbation cycle

The effect of peculiar velocities on the epoch of reionization (EoR) 21-cm signal

We have used semi-numerical simulations of reionization to study the behaviour of the power spectrum of the EoR 21-cm signal in redshift space. We have considered two models of reionization, one which has homogeneous recombination (HR) and the other incorporating inhomogeneous recombination (IR). We have estimated the observable quantities --- quadrupole and monopole moments of HI power spectrum at redshift space from our simulated data. We find that the magnitude and nature of the ratio between the quadrupole and monopole moments of the power spectrum ($P^s_2 /P^s_0$) can be a possible probe for the epoch of reionization. We observe that this ratio becomes negative at large scales for $x_{HI} \leq 0.7$ irrespective of the reionization model, which is a direct signature of an inside-out reionization at large scales. It is possible to qualitatively interpret the results of the simulations in terms of the fluctuations in the matter distribution and the fluctuations in the neutral fraction which have power spectra and cross-correlation $P_{\Delta \Delta}(k)$, $P_{xx}(k)$ and $P_{\Delta x}(k)$ respectively. We find that at large scales the fluctuations in matter density and neutral fraction is exactly anti-correlated through all stages of reionization. This provides a simple picture where we are able to qualitatively interpret the behaviour of the redshift space power spectra at large scales with varying $x_{HI}$ entirely in terms of a just two quantities, namely $x_{HI}$ and the ratio $P_{xx}/P_{\Delta \Delta}$. The nature of $P_{\Delta x}$ becomes different for HR and IR scenarios at intermediate and small scales. We further find that it is possible to distinguish between an inside-out and an outside-in reionization scenario from the nature of the ratio $P^s_2 /P^s_0$ at intermediate length scales.Comment: 11 pages, 6 figures. Accepted for publication in MNRAS. Replaced to match the accepted version. Added one appendix to quantify the possible uncertainties in the estimation of the multipole moments of redshift space power spectru

A smart contract system for decentralized borda count voting

In this article, we propose the first self-tallying decentralized e-voting protocol for a ranked-choice voting system based on Borda count. Our protocol does not need any trusted setup or tallying authority to compute the tally. The voters interact through a publicly accessible bulletin board for executing the protocol in a way that is publicly verifiable. Our main protocol consists of two rounds. In the first round, the voters publish their public keys, and in the second round they publish their randomized ballots. All voters provide Non-interactive Zero-Knowledge (NIZK) proofs to show that they have been following the protocol specification honestly without revealing their secret votes. At the end of the election, anyone including a third-party observer will be able to compute the tally without needing any tallying authority. We provide security proofs to show that our protocol guarantees the maximum privacy for each voter. We have implemented our protocol using Ethereum's blockchain as a public bulletin board to record voting operations as publicly verifiable transactions. The experimental data obtained from our tests show the protocol's potential for the real-world deployment