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Nakul Aggarwal

Publications and source records attributed to Nakul Aggarwal.

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Pruning-induced phases in fully-connected neural networks: the eumentia, the dementia, and the amentia

Modern neural networks are heavily overparameterized, and pruning, which removes redundant neurons or connections, has emerged as a key approach to compressing them without sacrificing performance. However, while practical pruning methods are well developed, whether pruning induces sharp phase transitions in the neural networks and, if so, to what universality class they belong, remain open questions. To address this, we study fully-connected neural networks trained on MNIST, independently varying the dropout (i.e., removing neurons) rate at both the training and evaluation stages to map the phase diagram. We identify three distinct phases: eumentia (the network learns), dementia (the network has forgotten), and amentia (the network cannot learn), sharply distinguished by the power-law scaling of the cross-entropy loss with the training dataset size. {In the eumentia phase, the algebraic decay of the loss, as documented in the machine learning literature as neural scaling laws, is from the perspective of statistical mechanics the hallmark of quasi-long-range order.} We demonstrate that the transition between the eumentia and dementia phases is accompanied by scale invariance, with a diverging length scale that exhibits hallmarks of a Berezinskii-Kosterlitz-Thouless-like transition; the phase structure is robust across different network widths and depths. Our results establish that dropout-induced pruning provides a concrete setting in which neural network behavior can be understood through the lens of statistical mechanics.

cond-mat.dis-nn

Observational Constraints on Chaplygin Gas Models in Non-Minimally Coupled Power Law $f(Q)$ Gravity with Quasars

In the framework of $f(Q)$ gravity, where gravity emerges from non-metricity $Q$, we explore the cosmological implications of its non-minimal coupling to matter. Inspired by the recent success of Chaplygin gas models in explaining dark energy, we consider a background fluid composed of baryonic matter, radiation, and a family of Chaplygin gas variants namely Generalized Chaplygin Gas (GCG), Modified Chaplygin Gas (MCG), and Variable Chaplygin Gas (VCG). We constrain these models with three recent observational datasets: Observational Hubble Data (OHD), Baryonic Acoustic Oscillation (BAO) measurements, and Quasi-Stellar Objects (QSO) data. For the QSO dataset, we propose an analytical expression for errors in comoving distance to circumvent the reliance on Monte Carlo simulations. Using kinematic diagnostics such as the deceleration and jerk parameters and Om diagnostic, we assess deviations of the proposed models from $\Lambda$CDM. Our joint analysis of the three datasets reveals that the transition redshift from a decelerated to an accelerated expansion of the universe for the GCG, MCG and VCG models is $0.620^{+0.018}_{-0.017}$, $0.537^{+0.017}_{-0.017}$ and $0.470^{+0.012}_{-0.012}$ respectively, indicating a departure from $\Lambda$CDM.

gr-qc

Discovering Factorization Surface of Quantum Spin Chains with Machine Learning

Entanglement in quantum many-body systems is required for a variety of quantum information tasks, making it crucial to identify the parameter space in which the ground state is fully separable, known as the factorization surface (FS). Nonetheless, the tuning parameters indicating FS for several quantum spin models remain unknown. We employ symbolic regression (SR), a supervised learning technique, to determine a closed-form expression in the parameter regime corresponding to FS of quantum many-body Hamiltonians. We verify the effectiveness of this method by examining the analytically tractable models, namely a nearest-neighbor (NN) quantum transverse XY model with additional Kaplan-Shekhtman-Entin-Aharony interactions, for which the FS is well-known. We construct an accurate expression for the FS of the XYZ model by providing the parameter set through the SR algorithm in which the ground state is derived by matrix product state formalism. With a satisfactory level of accuracy, we estimate the FS for the long-range XY model, and the NN XY model with Dzyaloshinskii-Moriya type asymmetric interaction for which the factorization surface is not known.

quant-ph

Phase-Binarized Spintronic Oscillators for Combinatorial Optimization, and Comparison with Alternative Classical and Quantum Methods

Solving combinatorial optimization problems efficiently through emerging hardware by converting the problem to its equivalent Ising model and obtaining its ground state is known as Ising computing. Phase-binarized oscillators (PBO), modeled through the Kuramoto model, have been proposed for Ising computing, and various device technologies have been used to experimentally implement such PBOs. In this paper, we show that an array of four dipole-coupled uniform-mode spin Hall nano oscillators (SHNOs) can be used to implement such PBOs and solve the NP-Hard combinatorial problem MaxCut on 4-node complete weighted graphs. We model the spintronic oscillators through two techniques: an approximate model for coupled magnetization dynamics of spin oscillators, and Landau Lifshitz Gilbert Slonckzweski (LLGS) equation-based more accurate magnetization dynamics modeling of such oscillators. Next, we compare the performance of these room-temperature-operating spin oscillators, as well as generalized PBOs, with two other alternative methods that solve the same MaxCut problem: a classical approximation algorithm, known as Goemans-Williamson's (GW) algorithm, and a Noisy Intermediate Scale Quantum (NISQ) algorithm, known as Quantum Approximation Optimization Algorithm (QAOA). For four types of graphs, with graph size up to twenty nodes, we show that approximation ratio (AR) and success probability (SP) obtained for generalized PBOs (Kuramoto model), as well as spin oscillators, are comparable to that for GW and much higher than that of QAOA for almost all graph instances. Moreover, unlike GW, the time to solution (TTS) for generalized PBOs and spin oscillators does not grow with graph size for the instances we have explored. This can be a major advantage for PBOs in general and spin oscillators specifically for solving these types of problems, along with the accuracy of solutions they deliver.

physics.app-ph

Constraining Generalized Chaplygin Gas in Non-Minimally Coupled $f(Q)$ Cosmology using Quasars and $H(z)$ Data

In the current framework of Einstein's equations in general relativity (GR), gravity is described by the spacetime curvature. However, there are other descriptions where the origin of gravity can be understood through torsion and non-metricity $Q$. In this work, we discuss a modified theory of gravity namely $f(Q)$ gravity, which considers a non-linear extension of $Q$. In particular, we study the case where it is non-minimally coupled to matter. Motivated by the recent success of Chaplygin gas models in the explanation of dark energy, we assume a pressureless baryonic matter and a generalized Chaplygin gas as the background fluid. We constrain the proposed model using two different datasets: one for Hubble measurements and the other for quasars (which we calibrated) with Markov-Chain Monte Carlo (MCMC) methods. We employ kinematic tools such as deceleration and jerk parameters to determine deviations of the proposed model from $\Lambda$CDM. We establish that the transition redshift $z_T$ in the deceleration parameter $q$ is $0.607$ and $0.204$ with the two datasets respectively, therefore describing the universe's acceleration.

gr-qc