activity
20182026
most citedA deep search for decaying dark matter with XMM-Newton blank-sky observations

123 citations · 691 across the 20 of their papers we have counts for

collaborators

22 papers

hep-ph2026

Re-examining the sensitivity of JWST to decaying axion dark matter

Caleb Gemmell, Christopher Dessert, Andrea Caputo +1

An eV-scale QCD axion comprising the observed dark matter (DM) abundance is expected to generate a photon line at infrared energies that would be observable or near-observable in d…

hep-ph2025

Freezing-in the Axiverse

Christopher Dessert, Soubhik Kumar, Joshua T. Ruderman

The presence of multiple light axions in the infrared is a generic feature of many ultraviolet (UV) scenarios. In many cases the number of axions is o…

hep-ph2025

Search for Axions in Magnetic White Dwarf Polarization at Lick and Keck Observatories

Joshua N. Benabou, Christopher Dessert, Kishore C. Patra +4

We present the most sensitive search to date for light axion-like particles with masses below a micro-eV, using spectropolarimetric data collected from the Lick and Keck Observator…

astro-ph.HE2024

Search for Axions from Magnetic White Dwarfs with Chandra

Orion Ning, Christopher Dessert, Vi Hong +1

Low mass axion-like particles could be produced in abundance within the cores of hot, compact magnetic white dwarf (MWD) stars from electron bremsstrahlung and converted to detecta…

hep-ph2023★ 2 cited

Sensitivity of JWST to eV-Scale Decaying Axion Dark Matter

Sandip Roy, Carlos Blanco, Christopher Dessert +2

The recently-launched James Webb Space Telescope (JWST) can resolve eV-scale emission lines arising from dark matter (DM) decay. We forecast the end-of-mission sensitivity to the d…

astro-ph.CO2023★ 2 cited

Was There a 3.5 keV Line?

Christopher Dessert, Joshua W. Foster, Yujin Park +1

The 3.5 keV line is a purported emission line observed in galaxies, galaxy clusters, and the Milky Way whose origin is inconsistent with known atomic transitions and has previously…

astro-ph.CO2023★ 1 cited

Limits from the grave: resurrecting Hitomi for decaying dark matter and forecasting leading sensitivity for XRISM

Christopher Dessert, Orion Ning, Nicholas L. Rodd +1

The Hitomi X-ray satellite mission carried unique high-resolution spectrometers that were set to revolutionize the search for sterile neutrino dark matter (DM) by looking for narro…

hep-ph2022★ 2 cited

Snowmass Theory Frontier: Astrophysics and Cosmology

Daniel Green, Joshua T. Ruderman, Benjamin R. Safdi +84

We summarize progress made in theoretical astrophysics and cosmology over the past decade and areas of interest for the coming decade. This Report is prepared as the TF09 "Astrophy…

hep-ph2022★ 19 cited

Higgsino Dark Matter Confronts 14 years of Fermi Gamma Ray Data

Christopher Dessert, Joshua W. Foster, Yujin Park +2

Thermal higgsino dark matter (DM), with mass around 1 TeV, is a well-motivated, minimal DM scenario that arises in supersymmetric extensions of the Standard Model. Higgsinos may na…

hep-ph2022★ 2 cited

Upper limit on the axion-photon coupling from magnetic white dwarf polarization

Christopher Dessert, David Dunsky, Benjamin R. Safdi

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…

hep-ph2021★ 7 cited

Red-Giant Branch Stellar Cores as Macroscopic Dark Matter Detectors

Christopher Dessert, Zachary Johnson

We show that macroscopic dark matter (DM) impacts on the degenerate helium cores of red-giant branch (RGB) stars can ignite helium fusion via DM-baryon elastic scattering. The onse…

hep-ph2021★ 118 cited

Upper Limit on the QCD Axion Mass from Isolated Neutron Star Cooling

Malte Buschmann, Christopher Dessert, Joshua W. Foster +2

The quantum chromodynamics (QCD) axion may modify the cooling rates of neutron stars (NSs). The axions are produced within the NS cores from nucleon bremsstrahlung and, when the nu…

hep-ph2021★ 56 cited

No evidence for axions from Chandra observation of magnetic white dwarf

Christopher Dessert, Andrew J. Long, Benjamin R. Safdi

Ultralight axions with axion-photon couplings GeV may resolve a number of astrophysical anomalies, such as unexpected ~TeV transpare…

astro-ph.CO2021★ 123 cited

A deep search for decaying dark matter with XMM-Newton blank-sky observations

Joshua W. Foster, Marius Kongsore, Christopher Dessert +4

Sterile neutrinos with masses in the keV range are well-motivated extensions to the Standard Model that could explain the observed neutrino masses while also making up the dark mat…

hep-ph2020★ 94 cited

X-ray Searches for Axions from Super Star Clusters

Christopher Dessert, Joshua W. Foster, Benjamin R. Safdi

Axions may be produced in abundance inside stellar cores and then convert into observable X-rays in the Galactic magnetic fields. We focus on the Quintuplet and Westerlund 1 super…

hep-ph2020

Systematics in the XENON1T data: the 15-keV anti-axion

Christopher Dessert, Joshua W. Foster, Yonatan Kahn +1

The XENON1T collaboration has found an excess of electron recoil events in their Science Run 1 data below ~7 keV with a spectral shape consistent with that expected from a solar-ax…

astro-ph.CO2020

Technical comment on the paper of Dessert et al. "The dark matter interpretation of the 3.5 keV line is inconsistent with blank-sky observations"

Alexey Boyarsky, Denys Malyshev, Oleg Ruchayskiy +1

An unidentified line at energy around 3.5 keV was detected in the spectra of dark matter-dominated objects. Recent work of Dessert et al. [1812.06976] used 30 Msec of XMM-Newton bl…

hep-ph2019★ 67 cited

Axion Emission Can Explain a New Hard -ray Excess from Nearby Isolated Neutron Stars

Malte Buschmann, Raymond T. Co, Christopher Dessert +1

Axions may be produced thermally inside the cores of neutron stars (NSs), escape the stars due to their feeble interactions with matter, and subsequently convert into X-rays in the…

astro-ph.HE2019★ 28 cited

Hard X-ray Excess from the Magnificent Seven Neutron Stars

Christopher Dessert, Joshua W. Foster, Benjamin R. Safdi

We report significant hard X-ray excesses in the energy range 2-8 keV for two nearby isolated neutron stars RX J1856.6-3754 and RX J0420.0-5022. These neutron stars have previously…

hep-ph2019★ 56 cited

X-ray Signatures of Axion Conversion in Magnetic White Dwarf Stars

Christopher Dessert, Andrew J. Long, Benjamin R. Safdi

White dwarf (WD) stars may radiate keV-energy axions produced in their stellar cores. This has been extensively studied as an extra channel by which WDs may cool, with some analyse…

astro-ph.CO2018★ 94 cited

The dark matter interpretation of the 3.5-keV line is inconsistent with blank-sky observations

Christopher Dessert, Nicholas L. Rodd, Benjamin R. Safdi

Observations of nearby galaxies and galaxy clusters have reported an unexpected X-ray emission line around 3.5 kilo-electron volts (keV). Proposals to explain this line include dec…

hep-ph2018★ 20 cited

Addressing Astrophysical and Cosmological Problems With Secretly Asymmetric Dark Matter

Christopher Dessert, Can Kilic, Cynthia Trendafilova +1

We present a simple model of dark matter that can address astrophysical and cosmological puzzles across a wide range of scales. The model is an application of the Secretly Asymmetr…