Area of research
Nuclear and High Energy Physics · Astronomy and Astrophysics
Research interest
Research interests include Physics, Dark matter, Annihilation, Astrophysics, Cosmic microwave background, and Particle physics.
Inhomogeneous energy injection in the 21-cm power spectrum: Sensitivity to dark matter decay
Birth of the first stars amidst decaying and annihilating dark matter
Exotic energy injection in the early Universe. II. CMB spectral distortions and constraints on light dark matter
Endothermic self-interacting dark matter in Milky Way-like dark matter haloes
Exotic energy injection in the early Universe. I. A novel treatment for low-energy electrons and photons
New pathways to the relic abundance of vector-portal dark matter
Glueballs in a thermal squeezeout model
Prospects for detecting heavy WIMP dark matter with the Cherenkov Telescope Array: The Wino and Higgsino
Lyman-<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>α</mml:mi></mml:math> constraints on cosmic heating from dark matter annihilation and decay
Thermal squeezeout of dark matter
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Code package for calculating modified cosmic ionization and thermal histories with dark matter and other exotic energy injections
Spurious Point Source Signals in the Galactic Center Excess
The enigmatic Galactic Center excess: Spurious point sources and signal mismodeling
Revival of the Dark Matter Hypothesis for the Galactic Center Gamma-Ray Excess
Evaporating the Milky Way halo and its satellites with inelastic self-interacting dark matter
Early-Universe constraints on dark matter-baryon scattering and their implications for a global 21 cm signal
GeV-scale thermal WIMPs: Not even slightly ruled out
Implications of a 21-cm signal for dark matter annihilation and decay
Indirect Detection of Dark Matter
Comment on “Characterizing the population of pulsars in the Galactic bulge with the Fermi large area telescope” [arXiv:1705.00009v1]
General constraints on dark matter decay from the cosmic microwave background
Enabling forbidden dark matter
Indirect dark matter signatures in the cosmic dark ages. I. Generalizing the bound on<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>s</mml:mi></mml:math>-wave dark matter annihilation from Planck results
Evidence for Unresolved<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>γ</mml:mi></mml:math>-Ray Point Sources in the Inner Galaxy
Indirect dark matter signatures in the cosmic dark ages. II. Ionization, heating, and photon production from arbitrary energy injections
Contributions to cosmic reionization from dark matter annihilation and decay
Model-independent indirect detection constraints on hidden sector dark matter
Self-consistent calculation of the Sommerfeld enhancement
High-energy tail of the Galactic Center gamma-ray excess