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Large Scale Structure

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lightbulbAbout this topic
Large Scale Structure refers to the distribution and organization of matter in the universe on scales larger than galaxy clusters, encompassing the arrangement of galaxies, galaxy clusters, and cosmic filaments. It studies the formation, evolution, and dynamics of these structures, providing insights into the underlying cosmological principles and the nature of dark matter and dark energy.
lightbulbAbout this topic
Large Scale Structure refers to the distribution and organization of matter in the universe on scales larger than galaxy clusters, encompassing the arrangement of galaxies, galaxy clusters, and cosmic filaments. It studies the formation, evolution, and dynamics of these structures, providing insights into the underlying cosmological principles and the nature of dark matter and dark energy.

Key research themes

1. How can machine learning and topological data analysis improve the extraction and modeling of the Cosmic Web's large-scale structure?

This research area focuses on developing sophisticated algorithms that can identify, extract, and probabilistically model the filamentary and web-like structures formed by galaxies and matter in the universe, known as the Cosmic Web. Traditional astrophysical statistics, such as correlation functions, often fail to capture the complexity of these large-scale arrangements. New computational methods aim to overcome challenges posed by high-dimensional data, noise, and hierarchical structures inherent in cosmological simulations and observations.

Key finding: Introduced the 1-DREAM toolbox that uses five machine learning methods, including Ant Colony and swarm intelligence algorithms, to extract one-dimensional filamentary structures from cosmological N-body simulations. It... Read more
Key finding: Developed the theoretical Hyperstructure Program providing a formal mathematical framework for forming higher-level structures (H-structures) through iterative binding, observation of emergent properties, local-to-global... Read more
Key finding: Proposed a formal multi-scale spatial data model and introduced the binary tolerance tree (BVT) to support multi-scale data storage and retrieval, which is essential for representing hierarchical structures like those seen in... Read more

2. What role do multi-field dynamics and complex bias modeling play in advancing theoretical descriptions and observational constraints of large-scale structure formation?

This theme investigates the incorporation of multi-field scalar dark energy models and advanced biasing schemes in understanding the growth of cosmic structures. It covers both theoretical frameworks, such as multi-field dark energy models with curved field space trajectories and effective field theory (EFT) approaches to structure formation, and the precise measurement of bias parameters up to cubic order in Eulerian and Lagrangian frameworks. These developments address inadequacies in single-field or local bias models and refine parameter estimation for cosmological data sets.

Key finding: Demonstrated that multi-field dark energy models following non-geodesic trajectories in field space allow cosmic acceleration on potentials too steep for single-field scenarios, thus evading swampland constraints. Such models... Read more
Key finding: Formulated a unified effective field theory framework that consistently connects inflationary initial conditions to large-scale structure formation, enabling model-independent computation of both primordial and late-time... Read more
Key finding: Introduced an extension of the quadratic field method to estimate cubic order bias parameters from halo fields in simulations, improving the modeling of one-loop halo power spectra. Significant detections of local and... Read more

3. How do observational cosmology techniques, including CMB measurements and 21 cm cosmology, interact with large-scale structure studies to constrain fundamental parameters like optical depth and the growth of structure?

This area explores the interplay between cosmic microwave background (CMB) analyses, large-scale structure observations, and novel probes such as the 21 cm hydrogen line to improve constraints on critical cosmological parameters, particularly the optical depth to reionization (τ) and amplitude of matter fluctuations (As). Combining these complementary datasets aims to overcome parameter degeneracies, refine the timeline of reionization, and enhance the precision of growth rate measurements, thereby advancing our understanding of the universe's evolution and underlying physics.

by Ms Aya
Key finding: Showed that 21 cm cosmology can independently and precisely predict the optical depth τ by leveraging power spectrum observations combined with semi-analytic reionization modeling and global 21 cm measurements. This breaks... Read more
Key finding: Although primarily an engineering-focused study, it demonstrated a non-invasive magnetomechanical technique for inferring dynamic strain in large steel structures. Analogously, innovative measurement methods with minimal... Read more
Key finding: Provided a conceptual foundation for multi-level and hierarchical structure formation processes, such as those underlying cosmic reionization bubbles and large-scale matter clustering, relevant when linking observables across... Read more

All papers in Large Scale Structure

This technical note proposes that the observed cosmic acceleration can arise without invoking a cosmological constant. In the Information-Induced Collapse Model (IICM), informational congestion acts as an effective fluid that reproduces... more
We discuss optical associations, spectral energy distributions and photometric redshifts for SWIRE sources in the ELAIS-N1 area and the Lockman Validation Field. The band-merged IRAC (3.6, 4.5, 5.8 and 8.0 µm) and MIPS (24, 70, 160 µm)... more
To study the relevance of mergers for the fueling of QSOs, we are currently conducting an HST imaging campaign of a sample of QSO host galaxies classified as ellipticals in the literature. Here, we present results from a study of the... more
We investigate a scalar field modulated by a spiral-time function as a candidate for a unified dark component, dynamically interpolating between Dark Matter (DM) and Dark Energy (DE). The model proposes that oscillatory regimes reproduce... more
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This work addresses one of the central challenges in modern physics: the reconciliation of quantum theory with general relativity. In standard approaches, Planck-scale vacuum fluctuations destabilize spacetime and render gravity... more
This work investigates flow structures in Couette-Poiseuille (C-P) flows with the adverse pressure gradient (APG) adjusted to create zero mean skin friction on the stationary wall. The vortical structures are identified as regions with a... more
This work is part of the ongoing CFT Framework Project, a program dedicated to the normalization of physics. The present paper develops the mathematical foundations of the Constitutive Flux (CF) Framework, which interprets spacetime as a... more
We present the large-scale correlation function measured from a spectroscopic sample of 46,748 luminous red galaxies from the Sloan Digital Sky Survey. The survey region covers 0.72h -3 Gpc 3 over 3816 square degrees and 0.16 < z < 0.47,... more
The angular distribution of galaxies encodes a wealth of information about large scale structure. Ultimately, the Sloan Digital Sky Survey (SDSS) will record the angular positions of order 10 8 galaxies in five bands, adding significantly... more
This paper reframes black holes not only as gravitational singularities but as integral components of a cosmic recycling system. Termed the Universal Grinder hypothesis, this model suggests that black holes consume matter, reduce it into... more
We introduce a new framework for cosmic acceleration: the Scalar-Cost Dark Energy model. In this approach, dark energy arises not from a cosmological constant but from an energetic cost associated with the expansion of spacetime. This... more
We study the phenomenology associated to non-minimally coupled dark matter. In particular, we consider the model where the non-minimal coupling arises from the formation of relativistic Bose-Einstein condensates in high density regions of... more
We investigate a scalar field modulated by a spiral-time function as a candidate for a unified dark component, dynamically interpolating between Dark Matter (DM) and Dark Energy (DE). The model proposes that oscillatory regimes reproduce... more
We collected data on radial velocities and distances of galaxies to elucidate structure and kinematics of the filament attached to the Virgo cluster from south. In the region RA = [12. h 5-13. h 5], Dec. = [-20 • ,0 • ] there are 171... more
The Cosmic Microwave Background (CMB) radiation represents one of the most significant discoveries in modern astrophysics, serving as a relic radiation from the early universe and providing empirical support for the Big Bang model. Its... more
This paper gives a compilation of physical mechanisms which have been proposed to explain the spectral red-shift of distant astronomical objects. Over sixty selected mechanisms are listed for the purpose of quantitative comparisons. Some... more
Comparison with the Standard Model. It is important to emphasize how the U(3) ZPE scalar field theory approach differs from the Standard Model (SM) in its treatment of divergences. The SM achieves its extraordinary precision through the... more
by gui la
he ETCQ framework proposes that dark energy is not a mysterious cosmological constant but the elastic response of a fundamental "frame" of space. Instead of acting at the Planck scale, this frame has a critical coherence length of about... more
We discuss the performances of a trigger implemented for the planned neutrino telescope NEMO. This trigger seems capable to discriminate between the signal and the strong background introduced by atmospheric muons and by the β decay of... more
Several models have been proposed to explain the cosmological constant as a consequence of alterations in the distance-redshift relation caused by the universe's inhomogeneities. We modelled the universe as a spherical galactic mass with... more
“The MBF scaling law (ρ^0.27) has now been derived from a minimal chameleon-modulus sector in string compactification. This suggests MBF scaling is truly universal, with the potential to turn otherwise parameter-dependent theories into... more
We develop a falsifiable framework in which the phenomenon attributed to "dark matter" arises from resonant overlap shadows cast by the baryonic sector, of which only ~15% is directly visible (luminous stars, gas, dust). Here a shadow... more
The phenomenon of resonant production of particles after inflation has received much attention in the past few years. In a new application of resonant production of particles, we consider the effect of a resonance during inflation. We... more
The past, present and future of cosmic microwave background (CMB) anisotropy research is discussed, with emphasis on the Boomerang and Maxima balloon experiments. These data are combined with large scale structure (LSS) information... more
We present results from our analysis of the Hydra I cluster observed in neutral atomic hydrogen (H ) as part of the Widefield ASKAP L-band Legacy All-sky Blind Survey (WALLABY). These WALLABY observations cover a 60-square-degree field of... more
This paper presents the Five-Dimensional Delay Field Model as a comprehensive Theory of Everything (TOE), unifying gravity, quantum mechanics, and the fundamental forces through a dynamical delay scalar field τ. Drawing from the detailed... more
General relativity and its extensions including torsion identify stress energy momentum as being proportional to the Einstein tensor, thus ensuring both symmetry and conservation. Here we visualize stress energy and momentum by... more
I introduce the Universal Algorithm (UA) as a geometric correction to Friedmann dynamics in a homogeneous and isotropic FLRW spacetime. The UA is modeled by a scalar term U (t) with the same dimension as H 2 , replacing Λ without invoking... more
The dynamics of particles in a gravitational field is investigated using Lagrange mechanics. Dynamic equations are obtained, including the rate of energy and momentum transfer to the gravitational field. The motion of particles in the... more
The Curvature-Activation Link (MRAH II) formalizes the idea that physical laws are not instantaneously absolute, but gradually activated in an environment-dependent manner. The activation field A ∈ [0, 1] quantifies law effectiveness: A →... more
In this work, I have formulated the chaotic inflation theory in the context of Starobinsky gravity, quadratic and quartic potential scenarios are considered. It is shown that the slow roll parameters at Hubble exit are dependent on theory... more
The Planck nominal mission cosmic microwave background (CMB) maps yield unprecedented constraints on primordial non-Gaussianity (NG). Using three optimal bispectrum estimators, separable template-fitting (KSW), binned, and modal, we... more
After many years of speculation, recent observations have confirmed the association of gamma-ray bursts with core-collapse supernova explosions from massive stars. This association carries with it important consequences. The burst... more
In DUST, the electromagnetic (EM) field propagates on a discrete hexagonal prime lattice (A 2). Discreteness perturbs the continuum EM mode density by a dimensionless, Brillouin-zone (BZ) averaged factor. We define the granularity factor
This paper presents a formalism for bimetric global and local time within the framework of teleparallel gravity, introducing dual metric-tetrad pairs to enforce time symmetry and account for torsional distortions. Global chronographic... more
The Higgs Gravitation-Sensitive Transition (HGST) model explores the idea that today’s cosmic acceleration can arise without a fundamental cosmological constant. Instead, the Standard-Model Higgs field undergoes a geometry-conditioned... more
This paper presents a comprehensive framework for estimating the population and properties of particles within the observable universe. The methodology synthesizes the Standard Model of Particle Physics with the Lambda-Cold Dark Matter... more
This paper presents a comprehensive framework for harmonic resonance architectures within black hole interior metrics, incorporating golden ratio couplings in a teleparallel gravity extension augmented by bimetric structures and... more
We study an effective 4-dimensional scalar-tensor field theory, originated from an underlying brane-bulk warped geometry, to explore the scenario of inflation. It is shown that the inflaton potential naturally emerges from the radion... more
The International X-ray Observatory (IXO) is a joint ESA-JAXA-NASA effort to address fundamental and timely questions in astrophysics: What happens close to a black hole? How did supermassive black holes grow? How does large scale... more
The success of the Magnetospheric Multiscale mission depends on the accurate measurement of the magnetic field on all four spacecraft. To ensure this success, two independently designed and built fluxgate magnetometers were developed,... more
This paper proposes a unified cosmological framework grounded in pressure driven gravity, in which gravitational effects arise from pressure gradients within a compressible, superfluid-like quantum vacuum. By modelling the vacuum as a... more
An optically accessible Taylor-Couette flow has been setup to enable experimental investigation of the influence of surface finish and roughness on the transfer of momentum between the wall and the bulk flow. Details of this facility and... more
The study of large scale structure (LSS) of the Universe has entered a precision era due to all-sky surveys and numerical simulations. The new data has provided a way to bring new methods to bear to analyze the cosmology as probed by... more
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