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Research Progress on Downstream Mechanisms of Glucose Metabolic Reprogramming and Its Role in the Occurrence and Progression of Type 2 Diabetes Mellitus
Chan Wu
,Maoying Wei
,Aijing Li
,Qingyi Zhu
,Jingyi Guo
,Anning Sun
,Xin Gu
,Yincheng Li
,Yanbing Gong
Posted: 20 May 2026
Numerical Simulation of Shock Wave Propagation Through Multiple Raindrops
Lingquan Li
,Jianglan Li
,Zhouteng Ye
,Jia Yan
,Linchuan Tian
,Xiaoquan Yang
Posted: 20 May 2026
WindPower-SAFusion: A Sparse-Attention and Multi-Scale Fusion Model for Wind Power Forecasting
Xuegong Zhang
,Yarou Li
,Zhuo Shao
,Huzi Qiu
,Jiatai Shi
,Jing Wang
,Dongdong Zhang
,Xuejing Zhao
Posted: 20 May 2026
A Descartes Companion Identity at Q = 2/3 and a Geometric Light-Fermion Mass Cascade
Andrew M. Brilliant
Posted: 20 May 2026
Biological Control of Fusarium verticillioides P03 in Maize by Bacillus cereus sensu lato B25 Involves Coordinated Host–Bacterium Responses
Jesús Eduardo Cazares-Álvarez
,Karem María Figueroa-Brambila
,Alejandro Miguel Figueroa-López
,Francisco Roberto Quiroz-Figueroa
,Ignacio Eduardo Maldonado-Mendoza
Posted: 20 May 2026
Comparative Performance Analysis of Vector Control, Fuzzy Logic Control, and Adaptive Quantum Fuzzy Logic for Induction Motor Drives in Hybrid Renewable Energy Systems
Mouhamadou Moustapha Diop
,Adam W. Skorek
,Modou Diop
Posted: 20 May 2026
Faithfulness-Aware Decoding via Constrained Optimization for Multi-Document Summarization: Framework, Diagnosis, and Empirical Analysis
Suhrid Pandey
,Sameer Kumar Singh
Posted: 20 May 2026
Soil Heterogeneity and Nutrient Response in Smallholder Maize Systems in Uganda: Implications for Balanced Fertilizer Recommendations
Yam Kanta Gaihre
,Kayuki C. Kaizzi
,John Wendt
,Latha Nagarajan
,Kodjovi S. Ezui
,Upendra Singh
,Joel Muyinza
,Angella Nansamba
,Ongua Fanuel
,Nabwami Ethel Joyce
+2 authors
Posted: 20 May 2026
Gaps in Contemporary International Political Economy Research: An Analytical Review of Structural Challenges, Technological Transformations, and Institutional Reconfigurations
Safran Safar Almakaty
Posted: 20 May 2026
Molecular Mechanisms of Zika Virus Entry into Host Cells
Haolong Cong
,Zhao Xin
,Wenhui Li
,Rong Lei
,Zhao Wenjun
,Xiaodong Han
Posted: 20 May 2026
Cross-Platform Performance and Security Evaluation of Post-Quantum Cryptographic Algorithms on Resource-Constrained Devices
Daiana-Larisa Lucaciu
,Daniela Elena Popescu
Posted: 20 May 2026
Neoformations and Tumors of the Hand and Wrist: WALANT Applied to 209 Cases
Giuseppe D'Antonio
,Alberto Rinaldi
,Francesco Schilardi
,Laura Langone
,Vanita Castafaro
,Veronica Longanesi
,Federico Pilla
Posted: 20 May 2026
The Silent Brand: How Perceived Greenhushing Shapes Green Purchase Intention Through Brand Trust, Perceived Risk, and Consumer Green Skepticism
Kha Duy Nguyen
,Le Thao Vy
Posted: 20 May 2026
A Hybrid Empirical-AI Model for Multi-Product Yield Prediction and Optimization from Cocoa Residues: A Stochastic Approach for Sustainable Valorization
Juan Carlos Vesga Ferreira
,Alexander Florez Martinez
,Brayan Elias Vargas Niño
Posted: 20 May 2026
An Archaeometric Study of the Porcelain Chinese Sherds Found at the Santana Convent in Lisbon – Part 2 – A Comparison with Coeval Chinese Samples of Well-Known Provenance
Luis F. Vieira Ferreira
,Ana Maria Rego
,Rosa Varela Gomes
,Mário Varela Gomes
,Shanshan Li
,Manuel F. C. Pereira
Posted: 20 May 2026
Receiver–Spectral Closure of Copy-Time Quantum Information: Finite Algebra, Gauge, Flavour, Global-Spectral Precision Predictions, and Hydrodynamic Reconstruction
Mohamed Sacha
Posted: 20 May 2026
A Simple Model for Self-Propelled Liquid Surfers
Ayase Kawamura
,Yuki Araya
,Hiroyuki Kitahata
,Shinpei Tanaka
Posted: 20 May 2026
A Linear Algebraic Proof of the Gauss-Markov Theorem Under Generalized Conditions: Theory and Empirical Application to Clustered Clinical Data
Justice Yaw Effah
,Gifty Duah
,Eric Nyarko
,Natasha Adjoa Anderson
,Miriam Appiah
Posted: 20 May 2026
New Prediction for Gravitational Wave Background from Topological Phase Transitions in the Early Universe
Ahmed Ali
Through this paper we analyze from first-principles, high-precision derivation of the spectral shape, characteristic amplitude, and unique observational signatures of the stochastic gravitational wave background (SGWB) generated during the primordial first-order topological phase transition that is a fundamental prediction of the Expanded Quantum String Theory with Gluonic Plasma (EQST-GP) framework. The transition corresponds to the spontaneous symmetry breaking \( SU(4) \to SU(3)_C \times U(1)_{\text{DM}} \) within the gluonic plasma confined to M5-brane world-volumes in the specific compactification geometry \( M_4 \times \text{CY}_3 \times S^1/\mathbb{Z}_2 \) with Euler characteristic \( \chi(\text{CY}_3) \approx -960 \). We move beyond generic parameterizations to perform a complete microphysical calculation. Starting from the finite-temperature effective potential for the symmetry-breaking scalar field \( \Phi \), where the coefficients \( D, T_0, E, \lambda \) in \( V_{\text{eff}}(\Phi, T) \approx D (T^2 - T_0^2) \Phi^2 - E T \Phi^3 + (\lambda/4) \Phi^4 \) are not free parameters but are explicitly computed from the underlying M-theory parameters: the M5-brane tension \( T_{M5} = (2\pi)^{-5} l_P^{-6} \), the volumes of the wrapped 2-cycles \( \text{Vol}(\Sigma_2) \), the stabilized values of the Kähler moduli $T_i$ from the KKLT-inspired potential \( V_{\text{up}}(\phi) \), and the thermal contributions of the confined \( SU(4) \) gluon degrees of freedom and the associated moduli fields. This derivation yields a highly specific set of phase transition parameters: a critical temperature \( T_c = 1.04^{+0.06}_{-0.05} \times 10^{16} \, \text{GeV} \), a nucleation temperature \( T_n = 0.971 \times 10^{16} \, \text{GeV} \) (corresponding to a Euclidean action \( S_3(T_n)/T_n = 138.2 \)), a transition strength parameter \( \alpha = 0.42 \pm 0.03 \) defined as the ratio of latent heat density to radiation energy density \( \alpha = \epsilon / \rho_{\text{rad}} \), and an inverse transition duration relative to Hubble \( \beta / H_* = 94.7 \). The bubble wall velocity \( v_w \), determined from the balance of the vacuum driving pressure against the friction from the strongly-coupled (2,0)-theory plasma on the M5-branes, is calculated to be \( v_w = 0.27 \, c \), characteristic of a deflagration mode. We then compute the gravitational wave spectrum \( \Omega_{\text{GW}}(f) h^2 \) from the three principal sources—scalar field bubble collisions \( (\Omega_\phi) \), sound waves in the post-collision plasma \( (\Omega_{\text{sw}}) \), and magnetohydrodynamic turbulence \( (\Omega_{\text{turb}}) \)—using the most advanced hydrodynamic simulations and envelope approximations, adapted for the specific relativistic degrees of freedom \( g_* = 187 \) of the EQST-GP plasma. The total spectrum exhibits a distinct, multi-peak fingerprint: a primary peak from sound waves at \( f_{\text{sw}} = 1.87 \times 10^{-3} \, \text{Hz} \) with amplitude \( \Omega_{\text{GW, sw}} h^2 = 6.31 \times 10^{-14} \), a secondary, broader peak from turbulence at \( f_{\text{turb}} \approx 3.2 \times 10^{-3} \, \text{Hz} \) with \( \Omega_{\text{GW, turb}} h^2 \approx 1.2 \times 10^{-14} \), and a high-frequency tail from bubble collisions. Crucially, we establish a detailed discrimination strategy demonstrating that the EQST-GP signal is distinguishable from inflationary tensor modes, cosmic string networks, and generic first-order phase transitions through multi-messenger consistency with predictions for ultra-heavy Majorana gluon dark matter, Hubble tension resolution, and fundamental constant derivation. We present a comprehensive detection blueprint for LISA, demonstrating that a signal-to-noise ratio $\text{SNR} > 8$ is achievable over a 4-year mission with optimal template-based analysis, and outline how cross-correlation with future CMB B-mode polarization measurements and 21-cm cosmology observations can further isolate this signal from astrophysical foregrounds.
Through this paper we analyze from first-principles, high-precision derivation of the spectral shape, characteristic amplitude, and unique observational signatures of the stochastic gravitational wave background (SGWB) generated during the primordial first-order topological phase transition that is a fundamental prediction of the Expanded Quantum String Theory with Gluonic Plasma (EQST-GP) framework. The transition corresponds to the spontaneous symmetry breaking \( SU(4) \to SU(3)_C \times U(1)_{\text{DM}} \) within the gluonic plasma confined to M5-brane world-volumes in the specific compactification geometry \( M_4 \times \text{CY}_3 \times S^1/\mathbb{Z}_2 \) with Euler characteristic \( \chi(\text{CY}_3) \approx -960 \). We move beyond generic parameterizations to perform a complete microphysical calculation. Starting from the finite-temperature effective potential for the symmetry-breaking scalar field \( \Phi \), where the coefficients \( D, T_0, E, \lambda \) in \( V_{\text{eff}}(\Phi, T) \approx D (T^2 - T_0^2) \Phi^2 - E T \Phi^3 + (\lambda/4) \Phi^4 \) are not free parameters but are explicitly computed from the underlying M-theory parameters: the M5-brane tension \( T_{M5} = (2\pi)^{-5} l_P^{-6} \), the volumes of the wrapped 2-cycles \( \text{Vol}(\Sigma_2) \), the stabilized values of the Kähler moduli $T_i$ from the KKLT-inspired potential \( V_{\text{up}}(\phi) \), and the thermal contributions of the confined \( SU(4) \) gluon degrees of freedom and the associated moduli fields. This derivation yields a highly specific set of phase transition parameters: a critical temperature \( T_c = 1.04^{+0.06}_{-0.05} \times 10^{16} \, \text{GeV} \), a nucleation temperature \( T_n = 0.971 \times 10^{16} \, \text{GeV} \) (corresponding to a Euclidean action \( S_3(T_n)/T_n = 138.2 \)), a transition strength parameter \( \alpha = 0.42 \pm 0.03 \) defined as the ratio of latent heat density to radiation energy density \( \alpha = \epsilon / \rho_{\text{rad}} \), and an inverse transition duration relative to Hubble \( \beta / H_* = 94.7 \). The bubble wall velocity \( v_w \), determined from the balance of the vacuum driving pressure against the friction from the strongly-coupled (2,0)-theory plasma on the M5-branes, is calculated to be \( v_w = 0.27 \, c \), characteristic of a deflagration mode. We then compute the gravitational wave spectrum \( \Omega_{\text{GW}}(f) h^2 \) from the three principal sources—scalar field bubble collisions \( (\Omega_\phi) \), sound waves in the post-collision plasma \( (\Omega_{\text{sw}}) \), and magnetohydrodynamic turbulence \( (\Omega_{\text{turb}}) \)—using the most advanced hydrodynamic simulations and envelope approximations, adapted for the specific relativistic degrees of freedom \( g_* = 187 \) of the EQST-GP plasma. The total spectrum exhibits a distinct, multi-peak fingerprint: a primary peak from sound waves at \( f_{\text{sw}} = 1.87 \times 10^{-3} \, \text{Hz} \) with amplitude \( \Omega_{\text{GW, sw}} h^2 = 6.31 \times 10^{-14} \), a secondary, broader peak from turbulence at \( f_{\text{turb}} \approx 3.2 \times 10^{-3} \, \text{Hz} \) with \( \Omega_{\text{GW, turb}} h^2 \approx 1.2 \times 10^{-14} \), and a high-frequency tail from bubble collisions. Crucially, we establish a detailed discrimination strategy demonstrating that the EQST-GP signal is distinguishable from inflationary tensor modes, cosmic string networks, and generic first-order phase transitions through multi-messenger consistency with predictions for ultra-heavy Majorana gluon dark matter, Hubble tension resolution, and fundamental constant derivation. We present a comprehensive detection blueprint for LISA, demonstrating that a signal-to-noise ratio $\text{SNR} > 8$ is achievable over a 4-year mission with optimal template-based analysis, and outline how cross-correlation with future CMB B-mode polarization measurements and 21-cm cosmology observations can further isolate this signal from astrophysical foregrounds.
Posted: 20 May 2026
International Digital System for Collective Food Security Support
Maxim Logachev
,Vitaliy Fomin
Posted: 20 May 2026
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