Search Publications

Invisible dilaton
DOI: 10.1103/PhysRevD.107.095015 Bibcode: 2023PhRvD.107i5015B

Brax, Philippe; Valageas, Patrick; Burrage, Clare +1 more

We analyze the dynamics of a light scalar field responsible for the µ term of the Higgs potential and coupled to matter via the Higgs-portal mechanism. We find that this dilaton model is stable under radiative corrections induced by the standard model particle masses. When the background value of the scalar field is stabilized at the minimum…

2023 Physical Review D
MICROSCOPE 4
Calibrating the effective magnitudes of type Ia supernovae with a model-independent method
DOI: 10.1103/PhysRevD.108.083024 Bibcode: 2023PhRvD.108h3024H

Li, Zhongmu; Chen, Jing; Hu, Jian +2 more

This research explores the correlation between the absolute magnitude and the redshift of type Ia supernovae (SNe Ia) with a model-independent approach. The Pantheon sample of SNe Ia and strong gravitational lensing systems (SGLS) are used. With the cosmic distance-duality relation (CDDR), the evolution parameter of the magnitude, the light curve …

2023 Physical Review D
eHST 3
Investigating starburst-driven neutrino emission from galaxies in the Great Observatories All-Sky LIRG Survey
DOI: 10.1103/PhysRevD.108.023015 Bibcode: 2023PhRvD.108b3015M

Privon, G. C.; van Eijndhoven, N.; Merckx, Y. +3 more

We present a phenomenological framework for starburst-driven neutrino production via proton-proton collisions and apply it to (ultra)luminous infrared galaxies (U/LIRGs) in the Great Observatories All-Sky LIRG Survey (GOALS). The framework relates the infrared luminosity of a GOALS galaxy, derived from consistently available Herschel Space Observa…

2023 Physical Review D
Herschel 3
Noise effect of test mass surface roughness in spaceborne gravitational wave detectors
DOI: 10.1103/PhysRevD.108.042001 Bibcode: 2023PhRvD.108d2001Y

Wang, Shun; Yan, Hao; Miao, Haixing +2 more

The spaceborne gravitational wave detection mission has a demanding requirement for the precision of displacement sensing, which is conducted by the interaction between the laser field and test mass. However, due to the roughness of the reflecting surface of the test mass, the displacement measurement along the sensitive axis suffers a coupling er…

2023 Physical Review D
LISAPathfinder 0
Primordial black hole production during first-order phase transitions
DOI: 10.1103/PhysRevD.105.L021303 Bibcode: 2022PhRvD.105b1303L

Cai, Rong-Gen; Guo, Zong-Kuan; Liu, Jing +2 more

A novel mechanism for the primordial black hole (PBH) production is proposed as a natural and inevitable consequence of general first-order phase transitions without reference to specific underlying particle physics models. We obtain mutual predictions and constraints between primordial black holes and gravitational waves from phase transitions in…

2022 Physical Review D
INTEGRAL 119
Upper limit on the axion-photon coupling from magnetic white dwarf polarization
DOI: 10.1103/PhysRevD.105.103034 Bibcode: 2022PhRvD.105j3034D

Safdi, Benjamin R.; Dessert, Christopher; Dunsky, David

Polarization measurements of thermal radiation from magnetic white dwarf (MWD) stars have been proposed as a probe of axion-photon mixing. The radiation leaving the surface of the MWD is unpolarized, but if low-mass axions exist then photons polarized parallel to the direction of the MWD's magnetic field may convert into axions, which induces a li…

2022 Physical Review D
Gaia 100
Hunt for light primordial black hole dark matter with ultrahigh-frequency gravitational waves
DOI: 10.1103/PhysRevD.106.103520 Bibcode: 2022PhRvD.106j3520F

Franciolini, Gabriele; Maharana, Anshuman; Muia, Francesco

Light primordial black holes may comprise a dominant fraction of the dark matter in our Universe. This paper critically assesses whether planned and future gravitational wave detectors in the ultrahigh-frequency band could constrain the fraction of dark matter composed of subsolar primordial black holes. Adopting the state-of-the-art description o…

2022 Physical Review D
INTEGRAL 69
Sensitivities on nonspinning and spinning primordial black hole dark matter with global 21-cm troughs
DOI: 10.1103/PhysRevD.105.103026 Bibcode: 2022PhRvD.105j3026S

Laha, Ranjan; Saha, Akash Kumar

Detection of the global 21 cm signal arising from neutral hydrogen can revolutionize our understanding of the standard evolution of the Universe after recombination. In addition, it can also be an excellent probe of dark matter (DM). Among all the DM candidates, primordial black holes (PBHs) are one of the most well motivated. Hawking emission fro…

2022 Physical Review D
INTEGRAL 56
Asteroids for µ Hz gravitational-wave detection
DOI: 10.1103/PhysRevD.105.103018 Bibcode: 2022PhRvD.105j3018F

Rajendran, Surjeet; Graham, Peter W.; Fedderke, Michael A.

A major challenge for gravitational-wave (GW) detection in the µ Hz band is engineering a test mass (TM) with sufficiently low acceleration noise. We propose a GW detection concept using asteroids located in the inner Solar System as TMs. Our main purpose is to evaluate the acceleration noise of asteroids in the µ Hz band. We show that…

2022 Physical Review D
SOHO 47
Dark dimension, the swampland, and the dark matter fraction composed of primordial black holes
DOI: 10.1103/PhysRevD.106.086001 Bibcode: 2022PhRvD.106h6001A

Anchordoqui, Luis A.; Antoniadis, Ignatios; Lüst, Dieter

Very recently, it was suggested that combining the swampland program with the smallness of the dark energy and confronting these ideas to experiment lead to the prediction of the existence of a single extra dimension (dubbed the dark dimension) with characteristic length scale in the micron range. We show that the rate of Hawking radiation slows d…

2022 Physical Review D
INTEGRAL 46