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๐Ÿ” steve bako ๐Ÿ“‚ Physics
Showing 3304 results for "steve bako" in Physics
Physics Preprint PDF DOI

Testing Scale-Dependent Modified Gravity with DESI DR1

D. Gonzalez, G. Niz, A. Aviles, C. Garcia-Quintero, H.E. Noriega, J. Aguilar, S. Ahlen, D. Bianchi, D. Brooks, T. Claybaugh, A. de la Macorra, A. de Mattia, P. Doel, S. Ferraro, J. E. Forero-Romero, E. Gaztanaga, S. Gontcho A Gontcho, G. Gutierrez, C. Hahn, K. Honscheid, D. Huterer, M. Ishak, R. Joyce, S. Juneau, R. Kehoe, D. Kirkby, M. Landriau, L. Le Guillou, M. E. Levi, M. Manera, A. Meisner, R. Miquel, S. Nadathur, W.J. Percival, I. Perez-Rafols, G. Rossi, L. Samushia, E. Sanchez, D. Schlegel, H. Seo, J. Silber, D. Sprayberry, G. Tarle, B. A. Weaver, R. Zhou (DESI Collaboration) ยท 2026

The Dark Energy Spectroscopic Instrument (DESI) provides an unprecedented opportunity to test deviations from general relativity (GR) that introduce a new physical scale within its redshift range. Usiโ€ฆ

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Physics Preprint PDF DOI

Kinematic Lensing Ratio: Reviving Weak Lensing Cosmography as a Geometric Dark Energy Probe

Qinxun Li (University of Utah) ยท 2026

We introduce the kinematic lensing ratio (KiLeR), a geometric dark-energy probe from weak lensing. Combining shear ratios with intrinsic galaxy shapes inferred from kinematics, KiLeR naturally mitigatโ€ฆ

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Physics Preprint PDF DOI

On the Relation Between Field-Level Posteriors, Correlators, and their Likelihoods

Massimo Pietroni, Fabian Schmidt ยท 2026

We develop a field-level posterior for cosmological data by marginalizing over initial conditions and noise in a general forward model. While our focus is on large-scale structure data, the results geโ€ฆ

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Physics Preprint PDF DOI

SVOM/VT: Preliminary Calibration Analysis

Zhu-Heng Yao, Yu-Lei Qiu, Jin-Song Deng, Li-Ping Xin, Chao Wu, Hua-Li Li, Jing Wang, Yi-Nuo Ma, Hong-Bo Cai, Xu-Hui Han, Jian-Yan Wei, Betrand Cordier ยท 2026

We present the in-orbit calibration of the Visible Telescope (VT), one of the key instruments aboard the Space Variable Objects Monitor (SVOM) mission for gamma-ray burst (GRB) studies. Using Gaia Datโ€ฆ

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Physics Preprint PDF DOI

A sound-horizon-free measurement of the Hubble constant from DESI DR2 baryon acoustic oscillations using artificial neural networks

Gaurav N. Gadbail, Kazuharu Bamba ยท 2026

We present a model-independent, sound-horizon-free measurement of the Hubble constant $H_0$ using baryon acoustic oscillation tracers from the Dark Energy Spectroscopic Instrument Data Release 2. The โ€ฆ

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Physics Preprint PDF DOI

From Big Bang Nucleosynthesis to Late-Time Acceleration in $f(Q,L_m)$ Gravity

Rajdeep Mazumdar, Kalyan Malakar, Kalyan Bhuyan ยท 2026

We perform a comprehensive investigation of the early-to-late time cosmic evolution within the framework of $f(Q,L_m)$ gravity, characterized by a non-minimal coupling between non-metricity and matterโ€ฆ

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Physics Preprint PDF DOI

Cosmological evolution of interacting dark energy with a CPL equation of state

Gerald Neumann, Nelson Videla, Dorian Araya ยท 2026

This paper examines interacting dark energy models within the Chevallier-Polarski-Linder (CPL) parametrization, emphasizing both theoretical structure and observational viability. Two commonly adoptedโ€ฆ

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Physics Preprint PDF DOI

Exploring Cosmic Evolution in R\'enyi Entropic Cosmology with Constraints from DESI DR2 BAO and GW Data

Rajdeep Mazumdar, Kalyan Malakar, Kalyan Bhuyan ยท 2026

We explore a cosmological model based on R\'enyi entropic corrections to the Friedmann equations and constrain it using DESI, P-BAO, CC, and gravitational-wave observations. Unlike earlier works, we oโ€ฆ

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Physics Preprint PDF DOI

The $f(Q, T)$ gravity and affine EoS: observational aspects

Romanshu Garg, G. P. Singh ยท 2026

In this paper, we investigate the cosmic expansion scenarios within the framework of $f(Q,T)$ gravity by using the affine equation of state (EoS) parameter. Specifically, we consider the linear form $โ€ฆ

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Multiscale Assessment of Tritium Behavior in Preliminary Fusion Pilot Plant Design Using Surrogate Models in TMAP8

Lin Yang, Pierre-Clement A. Simon, Emre Yildirim, Jose Trueba, Matthew Robinson, Masashi Shimada ยท 2026

The complexity and significance of multiscale phenomena in fusion energy systems make advanced modeling necessary for designing, optimizing, and safely deploying fusion plants. Tritium accountancy is โ€ฆ

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Physics Preprint PDF DOI

Model-independent consistency tests of DESI DR2 BAO and SN Ia

Hyeok Woo, William Luke Matthewson, Arman Shafieloo ยท 2026

Cosmic distances can be measured using two complementary probes: Type Ia supernovae (SN Ia), serving as standard candles, and baryon acoustic oscillations (BAO), serving as standard rulers. The luminoโ€ฆ

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Testing $\Lambda$CDM versus dynamical dark energy in one year: A DESI spectroscopic follow-up program for Rubin supernovae

Jannik Truong, Greg Aldering, Saul Perlmutter, David Rubin, David Schlegel ยท 2026

Combined cosmological probes currently indicate that best-fit values in the $w_0-w_a$ parametrization of dynamical dark energy deviate from $\Lambda$CDM by $\sim3\sigma$. In this work, we present a suโ€ฆ

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A barotropic alternative to Early Dark Energy for alleviating the $H_0$ tension

Youri Carloni, Orlando Luongo ยท 2026

We propose a cosmological scenario in which, beyond matter and radiation, an additional barotropic fluid with positive equation of state $\omega_s$ contributes to the cosmic energy budget, in contrastโ€ฆ

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Constraining Cosmological and Astrophysical Parameters with the Cosmic Star Formation History

Miguel Moyses, Rafael C. Nunes ยท 2026

Identifying new observational probes to constrain cosmological parameters has become an important goal in modern cosmology. In this work, we explore the potential of the cosmic star formation rate denโ€ฆ

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Physics Preprint PDF DOI

Observational tests of \texorpdfstring{$\Lambda(t)$}{Lambda(t)} cosmology in light of DESI DR2

D. Revanth Kumar, Santosh Kumar Yadav, S. A. Kadam ยท 2026

In this article, we investigate two phenomenological decaying vacuum cosmological models describing the accelerated expansion of the Universe. We constrain the model parameters using a Markov Chain Moโ€ฆ

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Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe?

Ozgur Akarsu, Maria Caruana, Konstantinos F. Dialektopoulos, Luis A. Escamilla, Emre O. Kahya, Jackson Levi Said ยท 2026

We investigate how strongly late-time inferences about DE dynamics depend on the functional prior used to represent the expansion history. Using identical late-time combinations of CC, DESI BAO measurโ€ฆ

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Model-Independent Analysis of Type Ia Supernova Datasets and Implications for Dark Energy

Zhenyuan Wang, Yun Wang ยท 2026

Recent analyses combining DESI DR2 BAO with CMB and SNe Ia data have reported $2.8$--$4.2\sigma$ evidence for dynamical dark energy, but the significance depends strongly on the supernova sample, raisโ€ฆ

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On the origin of the BAOtr-DESI tension

Ioannis Pantos, Leandros Perivolaropoulos ยท 2026

The fiducial-independent angular/transverse BAO dataset, obtained from two-point angular correlation functions in thin redshift shells (hereafter BAOtr), systematically prefers smaller comoving distanโ€ฆ

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Cosmological Parameters in $f(T)$ Gravity: Theoretical and Observational Analysis

Suraj Kumar Behera, S. A. Kadam, Pratik P. Ray, B. Mishra ยท 2026

The $f(T)$ gravity is one of the extensions of teleparallel equivalent of general relativity, in which more general functions of the torsion scalar $T$ can be described. With the proposed functional fโ€ฆ

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Self-similar Dynamics in Percolation and Sandpile

Mingzhong Lu, Ming Li, Youjin Deng ยท 2026

Spatial self-similarity is a hallmark of critical phenomena. We study the dynamic process of percolation, in which bonds are incrementally added to an initially empty lattice until the system becomes โ€ฆ

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