Author

Harsh Mehta

Institution: Tata Institute of Fundamental Research

Observed institution: Tata Institute of Fundamental Research

ORCID: 0009-0007-4664-4820

Observed ORCID: 0009-0007-4664-4820

OpenAlex ID: A5033333841

A power spectrum approach to the search for axion-like particles from resolved galaxy clusters using CMB as a backlight

2024 · Harsh Mehta, Suvodip Mukherjee · Journal of Cosmology and Astroparticle Physics · 9

A diffused background from axion-like particles in the microwave sky

2024 · Harsh Mehta, Suvodip Mukherjee · Journal of Cosmology and Astroparticle Physics · 8

SpectrAx: spectral search of axion-like particles using multi-band observations of galaxy clusters from SKA, SO, CMB-S4 and eROSITA

2025 · Harsh Mehta, Suvodip Mukherjee · Journal of Cosmology and Astroparticle Physics · 5

Turbulence induced non-Gaussian spectral distortion in the microwave sky from photon-axion conversion in galaxy clusters

2025 · Harsh Mehta, Suvodip Mukherjee · Journal of Cosmology and Astroparticle Physics · 3

Modified Cosmology or Modified Galaxy Astrophysics is Driving the z > 6 JWST Results? Cosmic Microwave Background Experiments Can Discover the Origin in the Near Future

2026 · Harsh Mehta, Suvodip Mukherjee · The Astrophysical Journal · 1

The prospect from the upcoming CMB experiment LiteBIRD to discover axion-like particles using Milky Way

2025 · Harsh Mehta, Suvodip Mukherjee · Journal of Cosmology and Astroparticle Physics · 1

Detecting axion-like particles using cosmic variance cancellation with CMB and radio surveys

2026 · Harsh Mehta, Anaya Dixit, et al. · Journal of Cosmology and Astroparticle Physics

Works count: 7

Citation count: 27

H-index: 3

I10-index: