Particle acceleration
View article: Predicted Resonant Re-Excitation of Interstellar Comet 3I/ATLAS During the Jupiter Flyby of March 16, 2026
Predicted Resonant Re-Excitation of Interstellar Comet 3I/ATLAS During the Jupiter Flyby of March 16, 2026 Open
This paper presents the Harmonic Curvature Model (HCM) forecast for the interstellar comet 3I/ATLAS during its 0.358 AU encounter with Jupiter. By modeling the nucleus as a damped toroidal resonator coupled to a scalar field, the author pr…
View article: Intangible Field Theory: Unification of Galactic Dynamics, Cosmology and Particle Physics from a Single Density Parameter
Intangible Field Theory: Unification of Galactic Dynamics, Cosmology and Particle Physics from a Single Density Parameter Open
Intangible Field Theory (IFT) proposes that space is permeated by a field of mutually repulsive particles (I field) with density ρ₀ = 2.4 × 10⁻²⁷ kg/m³. From this single hypothesis, the framework derives: E = mc², relativistic mass, time d…
View article: Intangible Field Theory: Unification of Galactic Dynamics, Cosmology and Particle Physics from a Single Density Parameter
Intangible Field Theory: Unification of Galactic Dynamics, Cosmology and Particle Physics from a Single Density Parameter Open
Intangible Field Theory (IFT) proposes that space is permeated by a field of mutually repulsive particles (I field) with density ρ₀ = 2.4 × 10⁻²⁷ kg/m³. From this single hypothesis, the framework derives: E = mc², relativistic mass, time d…
View article: Predicted Resonant Re-Excitation of Interstellar Comet 3I/ATLAS During the Jupiter Flyby of March 16, 2026
Predicted Resonant Re-Excitation of Interstellar Comet 3I/ATLAS During the Jupiter Flyby of March 16, 2026 Open
This paper presents the Harmonic Curvature Model (HCM) forecast for the interstellar comet 3I/ATLAS during its 0.358 AU encounter with Jupiter. By modeling the nucleus as a damped toroidal resonator coupled to a scalar field, the author pr…
View article: Simulation Study of Binary Mergers of Galaxy Clusters I: Properties of Merger Shocks and Radio Emission
Simulation Study of Binary Mergers of Galaxy Clusters I: Properties of Merger Shocks and Radio Emission Open
We investigate binary mergers of galaxy clusters and the resulting radio relics using three-dimensional simulations. The initial setup consists of two idealized, spherical subclusters with a mass ratio below three, each permeated by turbul…
View article: Practical predictions for the effects of acceleration on decay
Practical predictions for the effects of acceleration on decay Open
We make predictions of the effects of acceleration on decay rate for three benchmark processes spanning alpha, beta and isomeric decay. These processes are observed to require lower acceleration than that required by previously studied pro…
View article: Practical predictions for the effects of acceleration on decay
Practical predictions for the effects of acceleration on decay Open
We make predictions of the effects of acceleration on decay rate for three benchmark processes spanning alpha, beta and isomeric decay. These processes are observed to require lower acceleration than that required by previously studied pro…
View article: Simulation Study of Binary Mergers of Galaxy Clusters I: Properties of Merger Shocks and Radio Emission
Simulation Study of Binary Mergers of Galaxy Clusters I: Properties of Merger Shocks and Radio Emission Open
We investigate binary mergers of galaxy clusters and the resulting radio relics using three-dimensional simulations. The initial setup consists of two idealized, spherical subclusters with a mass ratio below three, each permeated by turbul…
View article: A Quantum-Geometric Interpretation of Cosmic Acceleration from Temporal Asynchrony
A Quantum-Geometric Interpretation of Cosmic Acceleration from Temporal Asynchrony Open
This preprint introduces SynchronoGeometry, a quantum-geometric framework that interprets cosmic acceleration as a manifestation of temporal asynchrony. The central innovation is treating time not as a fixed background parameter but as a d…
View article: A Quantum-Geometric Interpretation of Cosmic Acceleration from Temporal Asynchrony
A Quantum-Geometric Interpretation of Cosmic Acceleration from Temporal Asynchrony Open
This preprint introduces SynchronoGeometry, a quantum-geometric framework that interprets cosmic acceleration as a manifestation of temporal asynchrony. The central innovation is treating time not as a fixed background parameter but as a d…
View article: Article 4: Resistance to Acceleration in COED Geometry: Topological Friction and the Hierarchy of Cosmic Speeds (ver. 2)
Article 4: Resistance to Acceleration in COED Geometry: Topological Friction and the Hierarchy of Cosmic Speeds (ver. 2) Open
Based on the refined COED model presented in Article 3 (Version 3), we investigate the dynamics of accelerated motion in discrete space-time. We show that when a wave packet accelerates, additional resistance arises from the need to reconf…
View article: Rotating twisted magnetosphere of magnetars: approximate analytical solutions
Rotating twisted magnetosphere of magnetars: approximate analytical solutions Open
An approximate analytical solution for the rotating twisted magnetosphere of magnetars is presented. The poloidal flux is approximated by the self-similar twisted dipole field. The toroidal field is obtained by the minimum torque model. Un…
View article: Article 4: Resistance to Acceleration in COED Geometry: Topological Friction and the Hierarchy of Cosmic Speeds (ver. 2)
Article 4: Resistance to Acceleration in COED Geometry: Topological Friction and the Hierarchy of Cosmic Speeds (ver. 2) Open
Based on the refined COED model presented in Article 3 (Version 3), we investigate the dynamics of accelerated motion in discrete space-time. We show that when a wave packet accelerates, additional resistance arises from the need to reconf…
View article: Mission 043: TFD Neutrino Mass from SN1987A – Causal Derivation and Comparison with KATRIN
Mission 043: TFD Neutrino Mass from SN1987A – Causal Derivation and Comparison with KATRIN Open
Mission 043 documents the first causal derivation of the effective electron‑antineutrino mass from astrophysical observations of Supernova SN1987A within the framework of Tension Field Dynamics (TFD). Based on the observed 3‑hour time diff…
View article: Mission 043: TFD Neutrino Mass from SN1987A – Causal Derivation and Comparison with KATRIN
Mission 043: TFD Neutrino Mass from SN1987A – Causal Derivation and Comparison with KATRIN Open
Mission 043 documents the first causal derivation of the effective electron‑antineutrino mass from astrophysical observations of Supernova SN1987A within the framework of Tension Field Dynamics (TFD). Based on the observed 3‑hour time diff…
View article: A Nanosatellite-Sized Detector for Sub-MeV Charged Cosmic Ray Fluxes in Low Earth Orbit: The Low-Energy Module (LEM) Onboard the NUSES Space Mission
A Nanosatellite-Sized Detector for Sub-MeV Charged Cosmic Ray Fluxes in Low Earth Orbit: The Low-Energy Module (LEM) Onboard the NUSES Space Mission Open
NUSES is a planned space mission aiming to test new observational and technological approaches related to the study of low-energy cosmic rays, gamma rays, and high-energy astrophysical neutrinos. Two scientific payloads will be hosted onbo…
View article: Modeling Particle Acceleration and MWL Emission of a PeVatron Microquasar V4641 Sgr
Modeling Particle Acceleration and MWL Emission of a PeVatron Microquasar V4641 Sgr Open
The Large High Altitude Air Shower Observatory (LHAASO) has recently reported five Galactic microquasars as Ultra-High-Energy (UHE) $γ$-ray emitters (> 100 TeV). Among these sources, the microquasar V4641 Sgr exhibits $γ$-ray emission up t…
View article: Numerically Solving the Particle Kinetic Equation to Study the Effect of Non-Thermal Cooling on1 Particle Spectra in Relativistic Jets
Numerically Solving the Particle Kinetic Equation to Study the Effect of Non-Thermal Cooling on1 Particle Spectra in Relativistic Jets Open
Blazars exhibit broadband non-thermal emission characterized by a double-hump Spectral Energy Distribution¹⁷(SED) attributed to Synchrotron and Synchrotron Self-Compton (SSC) processes (P. Padovani et al. 2017; G.18Risaliti & M. Elvis 2004…
View article: Numerically Solving the Particle Kinetic Equation to Study the Effect of Non-Thermal Cooling on1 Particle Spectra in Relativistic Jets
Numerically Solving the Particle Kinetic Equation to Study the Effect of Non-Thermal Cooling on1 Particle Spectra in Relativistic Jets Open
Blazars exhibit broadband non-thermal emission characterized by a double-hump Spectral Energy Distribution¹⁷(SED) attributed to Synchrotron and Synchrotron Self-Compton (SSC) processes (P. Padovani et al. 2017; G.18Risaliti & M. Elvis 2004…
View article: Generation of giga-electron-volt proton beams by micronozzle acceleration
Generation of giga-electron-volt proton beams by micronozzle acceleration Open
Our proposed ion acceleration scheme, micronozzle acceleration (MNA), generates proton beams with extremely high kinetic energies on the giga-electron-volt (GeV) order. The underlying physics and performance of MNA are studied with two-dim…
View article: A Unified, Parameter-Free Derivation of Inertia, Vacuum Energy, and Mass( Cosmic to Quantum)
A Unified, Parameter-Free Derivation of Inertia, Vacuum Energy, and Mass( Cosmic to Quantum) Open
Modern theoretical physics faces several disconnected anomalies: the unexplained acceleration scale in galactic dynamics, the vacuum energy density, the hierarchical structure of particle masses, and the lack of a geometric reason for Stan…
View article: A Unified, Parameter-Free Derivation of Inertia, Vacuum Energy, and Mass( Cosmic to Quantum)
A Unified, Parameter-Free Derivation of Inertia, Vacuum Energy, and Mass( Cosmic to Quantum) Open
Modern theoretical physics faces several disconnected anomalies: the unexplained acceleration scale in galactic dynamics, the vacuum energy density, the hierarchical structure of particle masses, and the lack of a geometric reason for Stan…
View article: Disentangling the Geometric and Fluid Natures of Cosmic Acceleration
Disentangling the Geometric and Fluid Natures of Cosmic Acceleration Open
The observed cosmic acceleration represents one of the most profound mysteries in modern cosmology, challenging the standard model of particle physics and general relativity. This phenomenon can be theoretically approached from two primary…
View article: Disentangling the Geometric and Fluid Natures of Cosmic Acceleration
Disentangling the Geometric and Fluid Natures of Cosmic Acceleration Open
The observed cosmic acceleration represents one of the most profound mysteries in modern cosmology, challenging the standard model of particle physics and general relativity. This phenomenon can be theoretically approached from two primary…
View article: Deep insights into Abell 2163: unveiling the treasure trove of ICM plasma physics
Deep insights into Abell 2163: unveiling the treasure trove of ICM plasma physics Open
Nonthermal emission observed in galaxy clusters provides a direct probe into the plasma physics of the intra-cluster medium (ICM) under extreme conditions. We report the first detailed analysis of the giant radio halo in the merging galaxy…
View article: The Solar Close Observations and Proximity Experiments (SCOPE) mission
The Solar Close Observations and Proximity Experiments (SCOPE) mission Open
The Solar Close Observations and Proximity Experiments (SCOPE) mission will send a spacecraft into the solar atmosphere at a low altitude of just 5 R_sun from the solar center. It aims to elucidate the mechanisms behind solar eruptions and…
View article: Deep insights into Abell 2163: unveiling the treasure trove of ICM plasma physics
Deep insights into Abell 2163: unveiling the treasure trove of ICM plasma physics Open
Nonthermal emission observed in galaxy clusters provides a direct probe into the plasma physics of the intra-cluster medium (ICM) under extreme conditions. We report the first detailed analysis of the giant radio halo in the merging galaxy…
View article: Impact of Cosmic Ray Distribution on the Growth and Saturation of Bell Instability
Impact of Cosmic Ray Distribution on the Growth and Saturation of Bell Instability Open
Cosmic rays (CRs) streaming in weakly magnetized plasmas can drive large-amplitude magnetic fluctuations via nonresonant streaming instability (NRSI), or Bell instability. Using one-dimensional kinetic simulations, we investigate how mono-…
View article: Local Particle Acceleration in an ICME-in-Sheath Structure Observed by Solar Orbiter
Local Particle Acceleration in an ICME-in-Sheath Structure Observed by Solar Orbiter Open
Local particle acceleration in the shock sheath region formed during the interaction between multiple coronal mass ejections (CMEs) is a complicated process that is still under investigation. On 2024 March 23, the successive eruption of tw…
View article: Self-similar Cosmic-Ray Transport in High-resolution Magnetohydrodynamic Turbulence
Self-similar Cosmic-Ray Transport in High-resolution Magnetohydrodynamic Turbulence Open
We study the propagation of cosmic rays (CRs) through a simulation of magnetohydrodynamic (MHD) turbulence at an unprecedented resolution of 10,240 3 . We drive turbulence that is subsonic and super-Alfvénic, characterized by δB rms / B 0 …