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20162026
most citedDark Matter Axion Clump Resonance of Photons

105 citations · 581 across the 24 of their papers we have counts for

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18 papers · 1 filter

hep-ph2026

A Unified Numerical Study of Axion Stars: From the Nonrelativistic Regime to General Relativity

Parisa Arabameri, Paola Arias, Francisco Colipí-Marchant +1

Axion-star mass-radius relations are commonly computed using different orders of relativistic approximation, making it important to determine where these descriptions remain reliab…

hep-ph2026

Multi-messenger signal from QCD-Axion Ultracompact Minihalos

Dorian W. P. Amaral, Enrico D. Schiappacasse, Karla Tapia-Rebolledo

We explore the multimessenger signatures from ultracompact minihalos (UCMHs) seeded by stellar-mass primordial black holes (PBHs) and composed of QCD-axion dark matter. Using the s…

hep-ph2026

Dipole Radiation and Kinetic Mixing from Dark Photon Solitons

Enrico D. Schiappacasse, Moira Venegas

Wave-like dark matter composed of spin-1 particles, known as dark photons, is theorized to form clumps called "vector solitons". These solitons are compact astrophysical objects th…

hep-ph2025

Constraining Dark Photon Dark Matter with Radio Silence from Soliton Mergers around Supermassive Black Holes

Dorian W. P. Amaral, Enrico D. Schiappacasse, Hong-Yi Zhang

We place the first constraints on the dark matter fraction contained within dark photon solitons using the absence of their predicted radio-frequency signatures, or radio silence,…

hep-ph2025★ 3 cited

Dark photon dark matter from flattened axion potentials

Hong-Yi Zhang, Paola Arias, Andrew Cheek +3

Dark photons can be resonantly produced in the early universe via their coupling to an oscillating axion field. However, this mechanism typically requires large axion--dark photon…

hep-ph2025★ 6 cited

Dark Spin-2 Field Solitons as a Source of Electromagnetic Radiation

Enrico D. Schiappacasse

Spin- light dark boson particles can exhibit wave-like behavior, capable of forming long-lived, coherent, spatially localized structures known as solitons. This work considers t…

hep-ph2024

Resonant conversion of axion dark radiation into terahertz electromagnetic radiation in a neutron star magnetosphere

Andrew J. Long, Enrico D. Schiappacasse

In the strong magnetic field of a neutron star's magnetosphere, axions coupled to electromagnetism develop a nonzero probability to convert into photons. Past studies have revealed…

hep-ph2023★ 7 cited

Rescuing The Primordial Black Holes all-Dark Matter Hypothesis from The Fast Radio Bursts Tension

Dorian W. P. Amaral, Enrico D. Schiappacasse

Primordial black holes (PBHs) as an all-dark matter (DM) hypothesis has recently been demotivated by the prediction that these objects would source an excessive rate of fast radio…

hep-ph2023★ 21 cited

Photons from dark photon solitons via parametric resonance

Mustafa A. Amin, Andrew J. Long, Enrico D. Schiappacasse

Wave-like dark matter made of spin-1 particles (dark photons) is expected to form ground state clumps called "vector solitons", which can have different polarizations. In this work…

hep-ph2022★ 14 cited

PBH assisted search for QCD axion dark matter

Gongjun Choi, Enrico D. Schiappacasse

The entropy production prior to BBN era is one of ways to prevent QCD axion with the decay constant from overclosing the universe when…

hep-ph2021★ 4 cited

Can QCD Axion Stars explain Subaru HSC microlensing?

Enrico D. Schiappacasse, Tsutomu T. Yanagida

A non-negligible fraction of the QCD axion dark matter may form gravitationally bound Bose Einstein condensates, which are commonly known as axion stars or axion clumps. Such astro…

hep-ph2021★ 25 cited

Microlensing constraints on axion stars including finite lens and source size effects

Kohei Fujikura, Mark P. Hertzberg, Enrico D. Schiappacasse +1

A fraction of light scalar dark matter, especially axions, may organize into Bose-Einstein condensates, gravitationally bound clumps, "boson stars", and be present in large number…

hep-ph2021★ 30 cited

Radio signatures from encounters between Neutron Stars and QCD-Axion Minihalos around Primordial Black Holes

Sami Nurmi, Enrico D. Schiappacasse, Tsutomu T. Yanagida

Probing the QCD axion dark matter (DM) hypothesis is extremely challenging as the axion interacts very weakly with Standard Model particles. We propose a new avenue to test the QCD…

hep-ph2020★ 22 cited

Shining Primordial Black Holes

Mark P. Hertzberg, Sami Nurmi, Enrico D. Schiappacasse +1

We study the well-motivated mixed dark matter (DM) scenario composed of a dominant thermal WIMP, highlighting the case of triplet fermion "winos", with a small fraction o…

hep-ph2020★ 53 cited

Merger of Dark Matter Axion Clumps and Resonant Photon Emission

Mark P. Hertzberg, Yao Li, Enrico D. Schiappacasse

A portion of light scalar dark matter, especially axions, may organize into gravitationally bound clumps (stars) and be present in large number in the galaxy today. It is therefore…

hep-ph2018★ 105 cited

Dark Matter Axion Clump Resonance of Photons

Mark P. Hertzberg, Enrico D. Schiappacasse

Recently there has been interest in the physical properties of dark matter axion condensates. Due to gravitational attraction and self-interactions, they can organize into spatial…

hep-ph2018★ 38 cited

Scalar Dark Matter Clumps with Angular Momentum

Mark P. Hertzberg, Enrico D. Schiappacasse

The behavior of light scalar dark matter has been a subject of much interest recently as it can lead to interesting small scale behavior. In particular, this can lead to the format…

hep-ph2017★ 101 cited

Analysis of Dark Matter Axion Clumps with Spherical Symmetry

Enrico D. Schiappacasse, Mark P. Hertzberg

Recently there has been much interest in the spatial distribution of light scalar dark matter, especially axions, throughout the universe. When the local gravitational interactions…