Volume 106, Issue 10

15 November 2022

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HIGHLIGHTED ARTICLES

FEATURED IN PHYSICS

EDITORS' SUGGESTION

Structure of axion miniclusters

David Ellis, David J. E. Marsh, Benedikt Eggemeier, Jens Niemeyer, Javier Redondo, and Klaus Dolag

Phys. Rev. D 106, 103514 (2022) - Published 15 November, 2022

Asteroid-sized clumps of a dark matter candidate known as an axion could be detectable in a gravitational-microlensing survey.

FEATURED IN PHYSICS

Polarized image of equatorial emission in horizonless spacetimes: Traversable wormholes

Valentin Deliyski, Galin Gyulchev, Petya Nedkova, and Stoytcho Yazadjiev

Phys. Rev. D 106, 104024 (2022) - Published 10 November, 2022

Predictions indicate that wormholes and black holes may have nearly identical polarized light spectra, making these astrophysical objects difficult to distinguish.

EDITORS' SUGGESTION

Fast flavor instability in hypermassive neutron star disk outflows

Rodrigo Fernández, Sherwood Richers, Nicole Mulyk, and Steven Fahlman

Phys. Rev. D 106, 103003 (2022) - Published 3 November, 2022

Neutron star mergers are of tremendous astrophysical interest for a variety of reasons that include their role in initiating r-process nucleosynthesis in their ejecta. In this article, the authors tackle the complex influence of extremely rapid neutrino flavor conversion (fast flavor instability - FFI) on ejecta from accretion disks around hypermassive neutron stars (HMNSs) formed in mergers. By studying a wide variety of scenarios, the authors detail the influence of FFI and show that it depends strongly on the lifetime of the HMNS.

EDITORS' SUGGESTION

Bubble dynamics in fluids with $N$ -body simulations

Marek Lewicki, Ville Vaskonen, and Hardi Veermäe

Phys. Rev. D 106, 103501 (2022) - Published 3 November, 2022

The authors set up a new method (proof of concept) for studying bubble wall dynamics in first-order cosmological phase transitions based on N-body simulations. The technique goes beyond commonly used perfect fluid descriptions and equilibrium assumptions. This allows e.g. the computation of the terminal bubble wall velocity, a key ingredient for determining the gravitational wave signal created in the cosmological phase transition, based on particle physics properties rather than on phenomenological fluid parameters.

EDITORS' SUGGESTION

Effective-action model for dynamical scalarization beyond the adiabatic approximation

Mohammed Khalil, Raissa F. P. Mendes, Néstor Ortiz, and Jan Steinhoff

Phys. Rev. D 106, 104016 (2022) - Published 9 November, 2022

The authors provide a model for dynamical scalarization, beyond the adiabatic approximation, using effective field theory techniques, demonstrating that the inclusion of post-adiabatic corrections is crucial. The model is agnostic, i.e., independent of a specific theory of gravity and can therefore be used even for alternative gravity theories.

EDITORS' SUGGESTION

Surrogate model for gravitational wave signals from nonspinning, comparable-to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity

Tousif Islam, Scott E. Field, Scott A. Hughes, Gaurav Khanna, Vijay Varma, Matthew Giesler, Mark A. Scheel, Lawrence E. Kidder, and Harald P. Pfeiffer

Phys. Rev. D 106, 104025 (2022) - Published 14 November, 2022

Gravitational waveforms obtained using numerical relativity (NR) are computationally expensive and slow. Surrogate models provide an alternative to full NR by extrapolating from the point-particle regime of high-mass ratio binary waveforms calibrated to NR to much smaller mass ratios. The authors show that their methods work over a remarkable range of mass ratios of 2.5 to 10000 showing good agreement with NR simulations.

EDITORS' SUGGESTION

Critical phenomena in a gravitational collapse with a competing scalar field and gravitational waves in $4 + 1$ dimensions

Bernardo Porto Veronese and Carsten Gundlach

Phys. Rev. D 106, 104044 (2022) - Published 22 November, 2022

The authors numerically study the interactions between scalar fields and gravitational waves in the context of gravitational collapse at the threshold of black hole formation in $4 + 1$ dimensions. They find evidence for the existence of a co-dimension two attractor in the dynamical systems picture.

EDITORS' SUGGESTION

Rethinking mirror symmetry as a local duality on fields

Chiung Hwang, Sara Pasquetti, and Matteo Sacchi

Phys. Rev. D 106, 105014 (2022) - Published 17 November, 2022

The authors develop an algorithm for a field theoretical implementation of mirror symmetry. This is based on the so-called quiver representation of certain $N = 1$ supersymmetric theories and is a non-abelian generalization of the piecewise dualization of three-dimensional abelian theories. Extensions of this local field-theoretic operations to non-supersymmetric theories are expected.

EDITORS' SUGGESTION

Augmenting the residue theorem with boundary terms in finite-density calculations

Tyler Gorda, Juuso Österman, and Saga Säppi

Phys. Rev. D 106, 105026 (2022) - Published 29 November, 2022

Within the framework of the imaginary time formalism applied to systems at zero temperature but finite density, the authors investigate whether the order of integration, namely the spatial momentum integration is performed before that of the temporal momentum or vice versa, matters. They show that the former yields results consistent with those for nonzero but very low values of the temperature whilst the latter does not. They attribute this to the way the limit of the Fermi-Dirac distribution is taken as the temperature goes to zero.

LETTERS

LETTER

Measurement of stray electric fields in a capacitive inertial sensor using contactless test-mass charge modulation

S. M. Apple, S. Parry Kenyon, S. Barke, M. R. Clark, A. Y. Davila, B. C. Letson, G. Mueller, T. J. Olatunde, J. Sanjuan, O. E. Sauter, J. Siu, T. J. Sumner, P. J. Wass, and J. W. Conklin

Phys. Rev. D 106, L101101 (2022) - Published 28 November, 2022

LETTER

Searching for cosmic string induced stochastic gravitational wave background with the Parkes Pulsar Timing Array

Ligong Bian, Jing Shu, Bo Wang, Qiang Yuan, and Junchao Zong

Phys. Rev. D 106, L101301 (2022) - Published 14 November, 2022

LETTER

Gravitational radiation from inspiralling compact objects: Spin effects to the fourth post-Newtonian order

Gihyuk Cho, Rafael A. Porto, and Zixin Yang

Phys. Rev. D 106, L101501 (2022) - Published 3 November, 2022

LETTER

Quantum-mechanical mechanism for reducing the cosmological constant

Nemanja Kaloper and Alexander Westphal

Phys. Rev. D 106, L101701 (2022) - Published 28 November, 2022

ARTICLES

Evaluation of the potential of a gamma-ray observatory to detect astrophysical neutrinos through inclined showers

Jaime Alvarez-Muñiz, Ruben Conceição, Pedro J. Costa, Mário Pimenta, and Bernardo Tomé

Phys. Rev. D 106, 102001 (2022) - Published 3 November, 2022

ADMX-Orpheus first search for $70 μ eV$ dark photon dark matter: Detailed design, operations, and analysis

R. Cervantes, G. Carosi, S. Kimes, C. Hanretty, B. H. LaRoque, G. Leum, P. Mohapatra, N. S. Oblath, R. Ottens, Y. Park, G. Rybka, J. Sinnis, and J. Yang

Phys. Rev. D 106, 102002 (2022) - Published 9 November, 2022

Demonstration of length control for a filter cavity with coherent control sidebands

Naoki Aritomi, Yuhang Zhao, Eleonora Capocasa, Matteo Leonardi, Marc Eisenmann, Michael Page, Yuefan Guo, Eleonora Polini, Akihiro Tomura, Koji Arai, Yoichi Aso, Martin van Beuzekom, Yao-Chin Huang, Ray-Kuang Lee, Harald Lück, Osamu Miyakawa, Pierre Prat, Ayaka Shoda, Matteo Tacca, Ryutaro Takahashi, Henning Vahlbruch, Marco Vardaro, Chien-Ming Wu, Matteo Barsuglia, and Raffaele Flaminio

Phys. Rev. D 106, 102003 (2022) - Published 10 November, 2022

Resolving Galactic binaries using a network of space-borne gravitational wave detectors

Xue-Hao Zhang, Shao-Dong Zhao, Soumya D. Mohanty, and Yu-Xiao Liu

Phys. Rev. D 106, 102004 (2022) - Published 16 November, 2022

Effect of celestial body gravity on Taiji mission range and range acceleration noise

Xiaoqing Han, Xiaodong Peng, Wenlin Tang, Zhen Yang, Xiaoshan Ma, Chen Gao, Li-e Qiang, Yuzhu Zhang, Mengyuan Zhao, Jiafeng Zhang, and Binbin Liu

Phys. Rev. D 106, 102005 (2022) - Published 18 November, 2022

Incorporating information from LIGO data quality streams into the PyCBC search for gravitational waves

Derek Davis, Max Trevor, Simone Mozzon, and Laura K. Nuttall

Phys. Rev. D 106, 102006 (2022) - Published 22 November, 2022

Confirmation of stimulated Hawking radiation, but not of black hole lasing

Jeff Steinhauer

Phys. Rev. D 106, 102007 (2022) - Published 29 November, 2022

All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO and Advanced Virgo O3 data

R. Abbott et al. (LIGO Scientific Collaboration, Virgo Collaboration, and KAGRA Collaboration)

Phys. Rev. D 106, 102008 (2022) - Published 28 November, 2022

Assessing the data-analysis impact of LISA orbit approximations using a GPU-accelerated response model

Michael L. Katz, Jean-Baptiste Bayle, Alvin J. K. Chua, and Michele Vallisneri

Phys. Rev. D 106, 103001 (2022) - Published 1 November, 2022

When quantum corrections alter the predictions of classical field theory for scalar field dark matter

Andrew Eberhardt, Michael Kopp, and Tom Abel

Phys. Rev. D 106, 103002 (2022) - Published 3 November, 2022

EDITORS' SUGGESTION

Fast flavor instability in hypermassive neutron star disk outflows

Rodrigo Fernández, Sherwood Richers, Nicole Mulyk, and Steven Fahlman

Phys. Rev. D 106, 103003 (2022) - Published 3 November, 2022

Local thermodynamical equilibrium and relativistic dissipation

J. Félix Salazar and Thomas Zannias

Phys. Rev. D 106, 103004 (2022) - Published 3 November, 2022

Neutron star mass formula with nuclear saturation parameters for asymmetric nuclear matter

Hajime Sotani and Shinsuke Ota

Phys. Rev. D 106, 103005 (2022) - Published 4 November, 2022

Follow-up analyses of the binary-neutron-star signals GW170817 and GW190425 by using post-Newtonian waveform models

Tatsuya Narikawa and Nami Uchikata

Phys. Rev. D 106, 103006 (2022) - Published 4 November, 2022

Exploiting stellar explosion induced by the QCD phase transition in large-scale neutrino detectors

Tetyana Pitik, Daniel J. Heimsoth, Anna M. Suliga, and A. Baha Balantekin

Phys. Rev. D 106, 103007 (2022) - Published 4 November, 2022

Projected sensitivity of ${DMRadio-m}^{3}$ : A search for the QCD axion below $1 μ eV$

L. Brouwer et al. (DMRadio Collaboration)

Phys. Rev. D 106, 103008 (2022) - Published 8 November, 2022

Nonanalytic behavior of the relativistic $r$ -modes in slowly rotating neutron stars

K. Y. Kraav, M. E. Gusakov, and E. M. Kantor

Phys. Rev. D 106, 103009 (2022) - Published 7 November, 2022

Multiband light curves from eccentric accreting supermassive black hole binaries

John Ryan Westernacher-Schneider, Jonathan Zrake, Andrew MacFadyen, and Zoltán Haiman

Phys. Rev. D 106, 103010 (2022) - Published 8 November, 2022

Interpretation of the light curve of gamma-ray emission from the 2021 outburst of the recurrent nova RS Ophiuchi

Jian-He Zheng, Yi-Yun Huang, Ze-Lin Zhang, Hai-Ming Zhang, Ruo-Yu Liu, and Xiang-Yu Wang

Phys. Rev. D 106, 103011 (2022) - Published 9 November, 2022

Redshift effects in particle production from Kerr primordial black holes

Andrew Cheek, Lucien Heurtier, Yuber F. Perez-Gonzalez, and Jessica Turner

Phys. Rev. D 106, 103012 (2022) - Published 10 November, 2022

Deep learning and Bayesian inference of gravitational-wave populations: Hierarchical black-hole mergers

Matthew Mould, Davide Gerosa, and Stephen R. Taylor

Phys. Rev. D 106, 103013 (2022) - Published 10 November, 2022

Constraining the primordial curvature perturbation using dark matter substructure

Shin’ichiro Ando, Nagisa Hiroshima, and Koji Ishiwata

Phys. Rev. D 106, 103014 (2022) - Published 14 November, 2022

MHD decomposition explains diffuse $γ$ -ray emission in Cygnus X

Ottavio Fornieri and Heshou Zhang

Phys. Rev. D 106, 103015 (2022) - Published 15 November, 2022

Indirect detection of low mass dark matter in direct detection experiments with inelastic scattering

Nicole F. Bell, James B. Dent, Bhaskar Dutta, Jason Kumar, and Jayden L. Newstead

Phys. Rev. D 106, 103016 (2022) - Published 15 November, 2022

Massive black hole binaries in LISA: Multimessenger prospects and electromagnetic counterparts

Alberto Mangiagli, Chiara Caprini, Marta Volonteri, Sylvain Marsat, Susanna Vergani, Nicola Tamanini, and Henri Inchauspé

Phys. Rev. D 106, 103017 (2022) - Published 15 November, 2022

Search for continuous gravitational waves from HESS J1427-608 with a hidden Markov model

Deeksha Beniwal, Patrick Clearwater, Liam Dunn, Lucy Strang, Gavin Rowell, Andrew Melatos, and David Ottaway

Phys. Rev. D 106, 103018 (2022) - Published 15 November, 2022

Population properties of spinning black holes using the gravitational-wave transient catalog 3

Hui Tong, Shanika Galaudage, and Eric Thrane

Phys. Rev. D 106, 103019 (2022) - Published 16 November, 2022

Thermal effects on nuclear matter properties

Lucas Tonetto and Omar Benhar

Phys. Rev. D 106, 103020 (2022) - Published 16 November, 2022

Hadronuclear interactions in the jet of low TeV luminosity AGN: Implications for the low-state very-high-energy gamma-ray emission

Rui Xue, Ze-Rui Wang, and Wei-Jian Li

Phys. Rev. D 106, 103021 (2022) - Published 17 November, 2022

Temporal evolution and rigidity dependence of the solar modulation lag of Galactic cosmic rays

Nicola Tomassetti, Bruna Bertucci, and Emanuele Fiandrini

Phys. Rev. D 106, 103022 (2022) - Published 17 November, 2022

Extracting nuclear matter properties from the neutron star matter equation of state using deep neural networks

Márcio Ferreira, Valéria Carvalho, and Constança Providência

Phys. Rev. D 106, 103023 (2022) - Published 17 November, 2022

Constraining ultralight bosonic dark matter with Keck observations of S2’s orbit and kinematics

Guan-Wen Yuan, Zhao-Qiang Shen, Yue-Lin Sming Tsai, Qiang Yuan, and Yi-Zhong Fan

Phys. Rev. D 106, 103024 (2022) - Published 18 November, 2022

Testing modified gravity theories with numerical solutions of the external field effect in rotationally supported galaxies

Kyu-Hyun Chae, Federico Lelli, Harry Desmond, Stacy S. McGaugh, and James M. Schombert

Phys. Rev. D 106, 103025 (2022) - Published 21 November, 2022

Diffuse supernova neutrino background as a probe of late-time neutrino mass generation

André de Gouvêa, Ivan Martinez-Soler, Yuber F. Perez-Gonzalez, and Manibrata Sen

Phys. Rev. D 106, 103026 (2022) - Published 22 November, 2022

Binary neutron star mergers as a probe of quark-hadron crossover equations of state

Atul Kedia, Hee Il Kim, In-Saeng Suh, and Grant J. Mathews

Phys. Rev. D 106, 103027 (2022) - Published 22 November, 2022

Primordial black holes having gravitomagnetic monopole

Chandrachur Chakraborty and Sudip Bhattacharyya

Phys. Rev. D 106, 103028 (2022) - Published 22 November, 2022

Collisional instabilities of neutrinos and their interplay with fast flavor conversion in compact objects

Lucas Johns and Zewei Xiong

Phys. Rev. D 106, 103029 (2022) - Published 23 November, 2022

Evolution of equal mass binary bare quark stars in full general relativity: Could a supramassive merger remnant experience prompt collapse?

Enping Zhou, Kenta Kiuchi, Masaru Shibata, Antonios Tsokaros, and Kōji Uryū

Phys. Rev. D 106, 103030 (2022) - Published 23 November, 2022

Neutrino fast flavor pendulum. II. Collisional damping

Ian Padilla-Gay, Irene Tamborra, and Georg G. Raffelt

Phys. Rev. D 106, 103031 (2022) - Published 23 November, 2022

Formation and evaporation of strangelets during the merger of two compact stars

Niccoló Bucciantini, Alessandro Drago, Giuseppe Pagliara, Silvia Traversi, and Andreas Bauswein

Phys. Rev. D 106, 103032 (2022) - Published 28 November, 2022

Detecting cosmic strings with lensed fast radio bursts

Huangyu Xiao, Liang Dai, and Matthew McQuinn

Phys. Rev. D 106, 103033 (2022) - Published 28 November, 2022

Red-giant branch stellar cores as macroscopic dark matter detectors

Christopher Dessert and Zachary Johnson

Phys. Rev. D 106, 103034 (2022) - Published 28 November, 2022

Sensitivity of spin-aligned searches for neutron star-black hole systems using future detectors

Rahul Dhurkunde and Alexander H. Nitz

Phys. Rev. D 106, 103035 (2022) - Published 28 November, 2022

Implications for cosmic domain walls from the first three observing runs of LIGO-Virgo

Yang Jiang and Qing-Guo Huang

Phys. Rev. D 106, 103036 (2022) - Published 28 November, 2022

Prospects for detecting and localizing short-duration transient gravitational waves from glitching neutron stars without electromagnetic counterparts

Dixeena Lopez, Shubhanshu Tiwari, Marco Drago, David Keitel, Claudia Lazzaro, and Giovanni Andrea Prodi

Phys. Rev. D 106, 103037 (2022) - Published 28 November, 2022

Periastron precession effect of $f$ -mode dynamical tides on gravitational waves from eccentric double white dwarfs

Shu Yan Lau, Kent Yagi, and Phil Arras

Phys. Rev. D 106, 103038 (2022) - Published 30 November, 2022

Elaborating the ultimate fate of fast collective neutrino flavor oscillations

Soumya Bhattacharyya and Basudeb Dasgupta

Phys. Rev. D 106, 103039 (2022) - Published 30 November, 2022

Binaries wandering around supermassive black holes due to gravitoelectromagnetism

Xian Chen and Zhongfu Zhang

Phys. Rev. D 106, 103040 (2022) - Published 30 November, 2022

EDITORS' SUGGESTION

Bubble dynamics in fluids with $N$ -body simulations

Marek Lewicki, Ville Vaskonen, and Hardi Veermäe

Phys. Rev. D 106, 103501 (2022) - Published 3 November, 2022

Aether-quasi-dilaton massive gravity

Sobhan Kazempour, Amin Rezaei Akbarieh, and Emmanuel N. Saridakis

Phys. Rev. D 106, 103502 (2022) - Published 4 November, 2022

Power-law inflation satisfies Penrose’s Weyl curvature hypothesis

Guido D’Amico and Nemanja Kaloper

Phys. Rev. D 106, 103503 (2022) - Published 7 November, 2022

Dark radiation as a probe for a phase transition in the early Universe

Zihang Wang and Lijing Shao

Phys. Rev. D 106, 103504 (2022) - Published 8 November, 2022

Anisotropic cosmic optical background bound for decaying dark matter in light of the LORRI anomaly

Kazunori Nakayama and Wen Yin

Phys. Rev. D 106, 103505 (2022) - Published 9 November, 2022

Health checkup test of the standard cosmological model in view of recent cosmic microwave background anisotropies experiments

Eleonora Di Valentino, William Giarè, Alessandro Melchiorri, and Joseph Silk

Phys. Rev. D 106, 103506 (2022) - Published 10 November, 2022

Planck integrated Sachs-Wolfe-lensing likelihood and the CMB temperature

Julien Carron, Antony Lewis, and Giulio Fabbian

Phys. Rev. D 106, 103507 (2022) - Published 14 November, 2022

Phantom cosmologies from QCD ghost dark energy

Miguel Cruz, Samuel Lepe, and Germán E. Soto

Phys. Rev. D 106, 103508 (2022) - Published 14 November, 2022

Going beyond the galaxy power spectrum: An analysis of BOSS data with wavelet scattering transforms

Georgios Valogiannis and Cora Dvorkin

Phys. Rev. D 106, 103509 (2022) - Published 14 November, 2022

Inflating and reheating the Universe with an independent affine connection

Alberto Salvio

Phys. Rev. D 106, 103510 (2022) - Published 14 November, 2022

D-term inflation in braneworld models: Consistency with cosmic-string bounds and early-time Hubble tension resolving models

Chia-Min Lin

Phys. Rev. D 106, 103511 (2022) - Published 14 November, 2022

Dynamical system analysis of Myrzakulov gravity

G. Papagiannopoulos, Spyros Basilakos, and Emmanuel N. Saridakis

Phys. Rev. D 106, 103512 (2022) - Published 15 November, 2022

Revisiting sterile neutrino dark matter in gauged $U (1)_{B - L}$ model

Shintaro Eijima, Osamu Seto, and Takashi Shimomura

Phys. Rev. D 106, 103513 (2022) - Published 15 November, 2022

FEATURED IN PHYSICS

EDITORS' SUGGESTION

Structure of axion miniclusters

David Ellis, David J. E. Marsh, Benedikt Eggemeier, Jens Niemeyer, Javier Redondo, and Klaus Dolag

Phys. Rev. D 106, 103514 (2022) - Published 15 November, 2022

Asteroid-sized clumps of a dark matter candidate known as an axion could be detectable in a gravitational-microlensing survey.

Cannibal dark matter decoupled from the standard model: Cosmological constraints

Avirup Ghosh, Sourav Gope, and Satyanarayan Mukhopadhyay

Phys. Rev. D 106, 103515 (2022) - Published 15 November, 2022

How slowly can the early Universe expand?

Robert J. Scherrer

Phys. Rev. D 106, 103516 (2022) - Published 15 November, 2022

Early or phantom dark energy, self-interacting, extra, or massive neutrinos, primordial magnetic fields, or a curved universe: An exploration of possible solutions to the $H_{0}$ and $σ_{8}$ problems

Helena García Escudero, Jui-Lin Kuo, Ryan E. Keeley, and Kevork N. Abazajian

Phys. Rev. D 106, 103517 (2022) - Published 16 November, 2022

$I - Love - C$ relation for an anisotropic neutron star

H. C. Das

Phys. Rev. D 106, 103518 (2022) - Published 16 November, 2022

Machine learning constraints on deviations from general relativity from the large scale structure of the Universe

George Alestas, Lavrentios Kazantzidis, and Savvas Nesseris

Phys. Rev. D 106, 103519 (2022) - Published 17 November, 2022

Hunt for light primordial black hole dark matter with ultrahigh-frequency gravitational waves

Gabriele Franciolini, Anshuman Maharana, and Francesco Muia

Phys. Rev. D 106, 103520 (2022) - Published 17 November, 2022

Cosmic microwave background spectral distortions from Rayleigh scattering at second order

Atsuhisa Ota

Phys. Rev. D 106, 103521 (2022) - Published 17 November, 2022

Coupled and uncoupled early dark energy, massive neutrinos, and the cosmological tensions

Adrià Gómez-Valent, Ziyang Zheng, Luca Amendola, Christof Wetterich, and Valeria Pettorino

Phys. Rev. D 106, 103522 (2022) - Published 18 November, 2022

Have pulsar timing arrays detected the hot big bang: Gravitational waves from strong first order phase transitions in the early Universe

Katherine Freese and Martin Wolfgang Winkler

Phys. Rev. D 106, 103523 (2022) - Published 18 November, 2022

Droplet collapse during strongly supercooled transitions

Daniel Cutting, Essi Vilhonen, and David J. Weir

Phys. Rev. D 106, 103524 (2022) - Published 23 November, 2022

Structure formation and the global 21-cm signal in the presence of Coulomb-like dark matter-baryon interactions

Trey Driskell, Ethan O. Nadler, Jordan Mirocha, Andrew Benson, Kimberly K. Boddy, Timothy D. Morton, Jack Lashner, Rui An, and Vera Gluscevic

Phys. Rev. D 106, 103525 (2022) - Published 28 November, 2022

Constraints on dark matter annihilation and decay from the large-scale structure of the nearby Universe

D. J. Bartlett, A. Kostić, H. Desmond, J. Jasche, and G. Lavaux

Phys. Rev. D 106, 103526 (2022) - Published 29 November, 2022

Sample variance for supernovae distance measurements and the Hubble tension

Zhongxu Zhai and Will J. Percival

Phys. Rev. D 106, 103527 (2022) - Published 28 November, 2022

Toward inflation with $n_{s} = 1$ in light of the Hubble tension and implications for primordial gravitational waves

Gen Ye, Jun-Qian Jiang, and Yun-Song Piao

Phys. Rev. D 106, 103528 (2022) - Published 29 November, 2022

Can primordial parity violation explain the observed cosmic birefringence?

Tomohiro Fujita, Yuto Minami, Maresuke Shiraishi, and Shuichiro Yokoyama

Phys. Rev. D 106, 103529 (2022) - Published 28 November, 2022

Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and galaxy-galaxy lensing using the MagLim lens sample

A. Porredon et al. (DES Collaboration)

Phys. Rev. D 106, 103530 (2022) - Published 28 November, 2022

Cosmological perturbations: Noncold relics without the Boltzmann hierarchy

Lingyuan Ji, Marc Kamionkowski, and José Luis Bernal

Phys. Rev. D 106, 103531 (2022) - Published 29 November, 2022

Analytical approach to the core-halo structure of fuzzy dark matter

Atsushi Taruya and Shohei Saga

Phys. Rev. D 106, 103532 (2022) - Published 28 November, 2022

Comprehensive analysis of the compact phase space for Hu-Sawicki $f (R)$ dark energy models including spatial curvature

Kelly MacDevette, Peter Dunsby, and Saikat Chakraborty

Phys. Rev. D 106, 103533 (2022) - Published 28 November, 2022

Analytical covariance between the voxel intensity distribution and the power spectrum of line-intensity maps

Gabriela Sato-Polito and José Luis Bernal

Phys. Rev. D 106, 103534 (2022) - Published 29 November, 2022

Constraining the Barbero-Immirzi parameter from the duration of inflation in loop quantum cosmology

L. N. Barboza, G. L. L. W. Levy, L. L. Graef, and Rudnei O. Ramos

Phys. Rev. D 106, 103535 (2022) - Published 29 November, 2022

Low frequency tail of gravitational wave spectra from hydromagnetic turbulence

Ramkishor Sharma and Axel Brandenburg

Phys. Rev. D 106, 103536 (2022) - Published 30 November, 2022

Argument for the radiation-dominated behavior of matter fields in the preinflationary era

Taylor M. Ordines and Eric D. Carlson

Phys. Rev. D 106, 103537 (2022) - Published 30 November, 2022

Modeling transient resonances in extreme-mass-ratio inspirals

Priti Gupta, Lorenzo Speri, Beátrice Bonga, Alvin J. K. Chua, and Takahiro Tanaka

Phys. Rev. D 106, 104001 (2022) - Published 2 November, 2022

Where is the ringdown: Reconstructing quasinormal modes from dispersive waves

Josu C. Aurrekoetxea, Pedro G. Ferreira, Katy Clough, Eugene A. Lim, and Oliver J. Tattersall

Phys. Rev. D 106, 104002 (2022) - Published 2 November, 2022

Experimental system to detect the electromagnetic response of high-frequency gravitational waves

H. Zheng and L. F. Wei

Phys. Rev. D 106, 104003 (2022) - Published 3 November, 2022

Beyond Schwarzschild–de Sitter spacetimes: A new exhaustive class of metrics inspired by Buchdahl for pure $R^{2}$ gravity in a compact form

Hoang Ky Nguyen

Phys. Rev. D 106, 104004 (2022) - Published 3 November, 2022

Possible fluid interpretation and tidal force equation on a generic null hypersurface in Einstein-Cartan theory

Sumit Dey and Bibhas Ranjan Majhi

Phys. Rev. D 106, 104005 (2022) - Published 3 November, 2022

Magnetically charged Euler-Heisenberg black holes with scalar hair

Thanasis Karakasis, George Koutsoumbas, Andri Machattou, and Eleftherios Papantonopoulos

Phys. Rev. D 106, 104006 (2022) - Published 3 November, 2022

First post-Minkowskian approach to turbulent gravity

Donato Bini, Stuart Kauffman, Sauro Succi, and Pablo G. Tello

Phys. Rev. D 106, 104007 (2022) - Published 3 November, 2022

Electrically charged spherical matter shells in higher dimensions: Entropy, thermodynamic stability, and the black hole limit

Tiago V. Fernandes and José P. S. Lemos

Phys. Rev. D 106, 104008 (2022) - Published 4 November, 2022

Quasinormal modes of rotating black holes in Einstein-dilaton Gauss-Bonnet gravity: The second order in rotation

Lorenzo Pierini and Leonardo Gualtieri

Phys. Rev. D 106, 104009 (2022) - Published 4 November, 2022

Self-gravitating disks around rapidly spinning, tilted black holes: General-relativistic simulations

Antonios Tsokaros, Milton Ruiz, Stuart L. Shapiro, and Vasileios Paschalidis

Phys. Rev. D 106, 104010 (2022) - Published 4 November, 2022

Trouble with geodesics in black-to-white hole bouncing scenarios

Deog Ki Hong, Wei-Chen Lin, and Dong-han Yeom

Phys. Rev. D 106, 104011 (2022) - Published 7 November, 2022

Gravitational waveform model based on photon motion for spinning black holes

Song Li and Wen-Biao Han

Phys. Rev. D 106, 104013 (2022) - Published 9 November, 2022

Observational limits on the rate of radiation-driven binary black hole capture events

Michael Ebersold, Shubhanshu Tiwari, Leigh Smith, Yeong-Bok Bae, Gungwon Kang, Daniel Williams, Achamveedu Gopakumar, Ik Siong Heng, and Maria Haney

Phys. Rev. D 106, 104014 (2022) - Published 9 November, 2022

Premerger localization of intermediate mass binary black holes with LISA and prospects of joint observations with Athena and LSST

Pankaj Saini, Sajad A. Bhat, and K. G. Arun

Phys. Rev. D 106, 104015 (2022) - Published 9 November, 2022

EDITORS' SUGGESTION

Effective-action model for dynamical scalarization beyond the adiabatic approximation

Mohammed Khalil, Raissa F. P. Mendes, Néstor Ortiz, and Jan Steinhoff

Phys. Rev. D 106, 104016 (2022) - Published 9 November, 2022

Curious case of GW200129: Interplay between spin-precession inference and data-quality issues

Ethan Payne, Sophie Hourihane, Jacob Golomb, Rhiannon Udall, Derek Davis, and Katerina Chatziioannou

Phys. Rev. D 106, 104017 (2022) - Published 9 November, 2022

Approach to computing spectral shifts for black holes beyond Kerr

Asad Hussain and Aaron Zimmerman

Phys. Rev. D 106, 104018 (2022) - Published 9 November, 2022

Well-posed formulation of Einstein-Maxwell effective field theory

Iain Davies and Harvey S. Reall

Phys. Rev. D 106, 104019 (2022) - Published 10 November, 2022

Ultracompact object within a nonlocal Tolman VII model

B. N. Jayawiguna, I. Prasetyo, A. Sulaksono, and H. S. Ramadhan

Phys. Rev. D 106, 104020 (2022) - Published 10 November, 2022

Concurrent estimation of noise and compact-binary signal parameters in gravitational-wave data

Cailin Plunkett, Sophie Hourihane, and Katerina Chatziioannou

Phys. Rev. D 106, 104021 (2022) - Published 10 November, 2022

Debye superpotential for charged rings or circular currents around Kerr black holes

David Kofroň and Petr Kotlařík

Phys. Rev. D 106, 104022 (2022) - Published 10 November, 2022

Magnetostatic boson stars

Víctor Jaramillo and Darío Núñez

Phys. Rev. D 106, 104023 (2022) - Published 10 November, 2022

FEATURED IN PHYSICS

Polarized image of equatorial emission in horizonless spacetimes: Traversable wormholes

Valentin Deliyski, Galin Gyulchev, Petya Nedkova, and Stoytcho Yazadjiev

Phys. Rev. D 106, 104024 (2022) - Published 10 November, 2022

Predictions indicate that wormholes and black holes may have nearly identical polarized light spectra, making these astrophysical objects difficult to distinguish.

EDITORS' SUGGESTION

Surrogate model for gravitational wave signals from nonspinning, comparable-to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity

Tousif Islam, Scott E. Field, Scott A. Hughes, Gaurav Khanna, Vijay Varma, Matthew Giesler, Mark A. Scheel, Lawrence E. Kidder, and Harald P. Pfeiffer

Phys. Rev. D 106, 104025 (2022) - Published 14 November, 2022