activity
20122026
most citedIn the Realm of the Hubble tension a Review of Solutions

2k citations · 7.8k across the 94 of their papers we have counts for

collaborators

94 papers

astro-ph.CO2026

Do DESI-DR2 BAO data imply a coupling of dark matter and dark energy?

Weiqiang Yang, Sibo Zhang, Dinorah Barbosa +3

We revisit an interacting dark matter (DM) -- dark energy (DE) model characterized by the interaction function , where is a constant coupling parameter and is t…

astro-ph.CO2026

Late-Time Emergence of Dark Energy and Its Interaction with Dark Matter

Sibo Zhang, Weiqiang Yang, Supriya Pan +3

We present an interacting scenario between dark energy (DE) and dark matter (DM), where DE has an emergent nature, that means, DE was absent in the early universe but it becomes ef…

astro-ph.CO2026

Beyond dynamical dark energy: the role of dark sector interactions after DESI DR2

Weiqiang Yang, Sibo Zhang, Supriya Pan +2

Recent DESI DR2 observations have renewed interest in extensions of the CDM cosmological model, particularly through indications of a time-varying dark energy equation of state.…

astro-ph.CO2026

When One-Parameter Dark Energy Makes Neutrinos Physical Again

Weiqiang Yang, Eleonora Di Valentino, Eric V. Linder +2

A puzzling implication of current data interpreted in the -Cold Dark Matter cosmology is the preference for a negative sum of neutrino masses. Moving to CDM brings an ap…

gr-qc2026

Plasma impact on black hole shadow and gravitational weak lensing for Schwarzschild-like black hole

Weiqiang Yang, Mirzabek Alloqulov, Ahmadjon Abdujabbarov +3

This article delves into the observational properties of a Schwarzschild-like black hole (BH). Initially, the research provides a succinct examination of the spacetime geometry and…

astro-ph.CO2026

When Dark Energy Turns On: Constraints on a Critical Emergence Model

Mahdi Najafi, Mahdi Habibollahi, Masoume Reyhani +4

We investigate a specific emergent dark energy scenario, known as critically emergent dark energy (CEDE), in which dark energy is effectively absent in the early Universe and becom…

astro-ph.CO2026

Cosmological analysis of a viable gravity model

Siqi He, Weiqiang Yang, Hangyi Jin

Since viable gravity models must reconcile early-universe inflation with late-time acceleration, we specifically study the dynamical behavior of such a theory during the mat…

astro-ph.CO2026★ 6 cited

Joint Constraints on Neutrinos and Dynamical Dark Energy in Minimally Modified Gravity

Artur Ladeira, Rafael C. Nunes, Supriya Pan +1

The \(w_{\dagger}\)VCDM framework provides a theoretically well-controlled extension of \(Λ\)CDM within the class of minimally modified gravity theories, allowing for flexible cosm…

astro-ph.CO2025★ 3 cited

Is Dark Energy Changing? Probing the Universe's Expansion with present and future astronomical probes

Mehdi Rezaei, Supriya Pan, Weiqiang Yang +1

This study explores the possibility of a time-varying dark energy (DE) equation of state (EoS) deviating from -1. We employ a comprehensive dataset of usual astronomical probes (Ty…

astro-ph.CO2025

Dark Energy Is Not That Into You: Variable Couplings after DESI DR2 BAO

Weiqiang Yang, Sibo Zhang, Olga Mena +2

In interacting dark energy (DE) and dark matter (DM) scenarios, the interaction function typically includes a coupling parameter that quantifies the strength of energy exchange…

gr-qc2025★ 2 cited

Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints

Wenzhong Liu, Yabo Wu, Supriya Pan +1

Astronomical observations suggest that the current standard -Cold Dark Matter model in modern cosmology has some discrepancies when fitting the data during the whole expansion h…

astro-ph.CO2025★ 13 cited

Shape of Dark Energy: Constraining Its Evolution with a General Parametrization

Dong Ha Lee, Weiqiang Yang, Eleonora Di Valentino +2

We consider a general dark energy (DE) model parametrized by its equation-of-state (EoS), featuring three free parameters: (the present-day value of the DE EoS), (quant…

astro-ph.CO2025★ 4 cited

When Dark Matter Heats Up: A Model-Independent Search for Non-Cold Behavior

Mazaharul Abedin, Luis A. Escamilla, Supriya Pan +2

This article questions the common assumption of cold dark matter (DM) by exploring the possibility of a non-zero equation of state (EoS) without relying on any parametric approach.…

astro-ph.CO2025

Probing the cold nature of dark matter

Weiqiang Yang, Supriya Pan, Eleonora Di Valentino +3

A pressureless dark matter component fits well with several cosmological observations. However, there are indications that cold dark matter may encounter challenges in explaining o…

astro-ph.CO2025★ 6 cited

A New Window on Dynamical Dark Energy: Combining DESI-DR2 BAO with future Gravitational Wave Observations

Felipe Bruno Medeiros dos Santos, Jonathan Morais, Supriya Pan +2

Baryon acoustic oscillation (BAO) data from the Dark Energy Spectroscopic Instrument (DESI) appear to indicate the first evidence for dynamical dark energy (DDE), with a present-da…

astro-ph.CO2025★ 299 cited

The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics

Eleonora Di Valentino, Jackson Levi Said, Adam Riess +533

The standard model of cosmology has provided a good phenomenological description of a wide range of observations both at astrophysical and cosmological scales for several decades.…

astro-ph.CO2025★ 17 cited

Interacting dark energy after DESI DR2: a challenge for CDM paradigm?

Supriya Pan, Sivasish Paul, Emmanuel N. Saridakis +1

We investigate the scenario of interacting dark energy through a detailed confrontation with various observational datasets. We quantify the interaction in a general way, through t…

astro-ph.CO2024★ 25 cited

Testing an oscillatory behavior of dark energy

Luis A. Escamilla, Supriya Pan, Eleonora Di Valentino +3

The main aim of this work is to use a model-independent approach, along with late-time observational probes, to reconstruct the dark energy (DE) equation of state .…

astro-ph.CO2023★ 15 cited

On the interacting dark energy scenarios the case for Hubble constant tension

Supriya Pan, Weiqiang Yang

The Hubble constant is one of the important cosmological parameters measuring the expansion rate of our universe at present moment. Over the last couple of years, has c…

astro-ph.CO2023

Evidence of dynamical dark energy in a non-flat universe: current and future observations

Mehdi Rezaei, Supriya Pan, Weiqiang Yang +1

We investigate the dark energy phenomenology in an extended parameter space where we allow the curvature density of our universe as a free-to-vary parameter. The inclusion of the c…

astro-ph.CO2023★ 12 cited

Exploring bulk viscous unified scenarios with Gravitational Waves Standard Sirens

Weiqiang Yang, Supriya Pan, Eleonora Di Valentino +2

We consider the unified bulk viscous scenarios and constrain them using the Cosmic Microwave Background observations from Planck 2018 and the Pantheon sample from Type Ia Supernova…

astro-ph.CO2022★ 27 cited

IWDM: The fate of an interacting non-cold dark matter vacuum scenario

Supriya Pan, Weiqiang Yang, Eleonora Di Valentino +2

In most cosmological models, the equation of state of the dark matter is assumed to be zero, which means that the dark matter is pressure-less or cold. While this hypothesis is bas…

astro-ph.CO2022★ 67 cited

Revealing the effects of curvature on the cosmological models

Weiqiang Yang, William Giarè, Supriya Pan +3

In this paper we consider the effects of adding curvature in extended cosmologies involving a free-to-vary neutrino sector and different parametrizations of Dark Energy (DE). We ma…

hep-ph2022★ 10 cited

Report of the Topical Group on Cosmic Probes of Fundamental Physics for for Snowmass 2021

Rana X. Adhikari, Luis A. Anchordoqui, Ke Fang +118

Cosmic Probes of Fundamental Physics take two primary forms: Very high energy particles (cosmic rays, neutrinos, and gamma rays) and gravitational waves. Already today, these probe…