activity
20162026
most citedDoubly peaked induced stochastic gravitational wave background : Testing baryogenesis from primordial black holes

76 citations · 1.3k across the 130 of their papers we have counts for

collaborators

132 papers

astro-ph.CO2026

Gauge Backreaction in Standard Model Warm Inflation

Rafid H. Dejrah, Anish Ghoshal

Standard-Model warm inflation (SMWI) makes QCD the microscopic origin of inflationary dissipation, so the real-time response of the gauge plasma enters the cosmological prediction.…

astro-ph.CO2026

Statistical Fluctuations as Primordial Correlators in the CMB: Finite Chemical Potential Thermodynamics

Anish Ghoshal, Anupam Mazumdar, Bartłomiej Sikorski

Can primordial cosmological correlations originate from statistical fluctuations of an early-universe thermal system? We connect grand-canonical thermodynamics, stochastic transpor…

hep-ph2026

Primordial Black Hole Assisted Dirac Leptogenesis

Marco Manno, Anish Ghoshal

Dirac leptogenesis offers a qualitatively different route to the baryon asymmetry: total lepton number is conserved, but equal and opposite asymmetries are stored in the Standard M…

astro-ph.CO2026

Impact of Scale-dependent Primordial Non-Gaussianity on Scalar-induced Gravitational Waves

Alisha Marriott-Best, Devanshu Sharma, Anish Ghoshal +1

Scalar-induced gravitational waves (SIGWs) probe primordial curvature perturbations beyond cosmic microwave background scales, while primordial black holes (PBHs) probe the rare ta…

hep-th2026

Exact Lattice Identities and Continuum-Limit Dyson--Schwinger Equations for Yang-Mills Theory

Arpan Chatterjee, Marco Frasca, Anish Ghoshal +1

Starting from SU(N) on the lattice, we give a rigorous derivation of the Dyson--Schwinger equations in the continuum limit. We formulate the Dyson--Schwinger identities for the lat…

astro-ph.CO2026

Magnetically assisted primordial scalar perturbations: Scalar-Induced Gravitational Waves

Arko Bhaumik, Theodoros Papanikolaou, Anish Ghoshal

Primordial magnetic fields (PMFs) provide a well-motivated source of cosmological perturbations through their anisotropic stress and may leave observable imprints in both the scala…