A roadmap review of thermally conductive polymer composites: critical factors, progress, and prospects

Z Wang, Z Wu, L Weng, S Ge, D Jiang… - Advanced functional …, 2023‏ - Wiley Online Library
Recently, the need for miniaturization and high integration have steered a strong technical
wave in develo** (micro‐) electronic devices. However, excessive amounts of heat may …

Hubble tension: The evidence of new physics

JP Hu, FY Wang - Universe, 2023‏ - mdpi.com
The Λ CDM model provides a good fit to most astronomical observations but harbors large
areas of phenomenology and ignorance. With the improvements in the precision and …

[HTML][HTML] Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

S Vagnozzi - Universe, 2023‏ - mdpi.com
The Hubble tension has now grown to a level of significance which can no longer be
ignored and calls for a solution which, despite a huge number of attempts, has so far eluded …

Challenges for ΛCDM: An update

L Perivolaropoulos, F Skara - New Astronomy Reviews, 2022‏ - Elsevier
A number of challenges to the standard Λ CDM model have been emerging during the past
few years as the accuracy of cosmological observations improves. In this review we discuss …

The H0 Olympics: A fair ranking of proposed models

N Schöneberg, GF Abellán, AP Sánchez, SJ Witte… - Physics Reports, 2022‏ - Elsevier
Despite the remarkable success of the Λ Cold Dark Matter (Λ CDM) cosmological model, a
growing discrepancy has emerged (currently measured at the level of∼ 4− 6 σ) between the …

In the realm of the Hubble tension—a review of solutions

E Di Valentino, O Mena, S Pan, L Visinelli… - … and Quantum Gravity, 2021‏ - iopscience.iop.org
The simplest ΛCDM model provides a good fit to a large span of cosmological data but
harbors large areas of phenomenology and ignorance. With the improvement of the number …

Nonminimal dark sector physics and cosmological tensions

E Di Valentino, A Melchiorri, O Mena, S Vagnozzi - Physical Review D, 2020‏ - APS
We explore whether nonstandard dark sector physics might be required to solve the existing
cosmological tensions. The properties we consider in combination are (a) an interaction …

[HTML][HTML] Sterile neutrinos

B Dasgupta, J Kopp - Physics Reports, 2021‏ - Elsevier
Neutrinos, being the only fermions in the Standard Model of Particle Physics that do not
possess electromagnetic or color charges, have the unique opportunity to communicate with …

Neutrino self-interactions: A white paper

JM Berryman, N Blinov, V Brdar, T Brinckmann… - Physics of the Dark …, 2023‏ - Elsevier
Abstract Neutrinos are the Standard Model (SM) particles which we understand the least,
often due to how weakly they interact with the other SM particles. Beyond this, very little is …

tension, phantom dark energy, and cosmological parameter degeneracies

G Alestas, L Kazantzidis, L Perivolaropoulos - Physical Review D, 2020‏ - APS
Phantom dark energy (w<-1) can produce amplified cosmic acceleration at late times, thus
increasing the value of H 0 favored by CMB data and releasing the tension with local …