activity
20172023
most citedChallenges in Inflationary Magnetogenesis: Constraints from Strong Coupling, Backreaction and the Schwinger Effect

78 citations · 333 across the 15 of their papers we have counts for

collaborators

15 papers

gr-qc2023★ 26 cited

Shallow relic gravitational wave spectrum with acoustic peak

Ramkishor Sharma, Jani Dahl, Axel Brandenburg +1

We study the gravitational wave (GW) spectrum produced by acoustic waves in the early universe, such as would be produced by a first order phase transition, focusing on the low-fre…

physics.plasm-ph2023★ 8 cited

Inverse cascading for initial MHD turbulence spectra between Saffman and Batchelor

Axel Brandenburg, Ramkishor Sharma, Tanmay Vachaspati

In decaying magnetohydrodynamic (MHD) turbulence with a strong magnetic field, the spectral magnetic energy density is known to increase with time at small wavenumbers , provide…

hep-ph2022★ 7 cited

Magnetohydrodynamics predicts heavy-tailed distributions of axion-photon conversion

Pierluca Carenza, Ramkishor Sharma, M. C. David Marsh +2

The interconversion of axionlike particles (ALPs) and photons in magnetised astrophysical environments provides a promising route to search for ALPs. The strongest limits to date o…

astro-ph.GA2022★ 11 cited

Batchelor, Saffman, and Kazantsev spectra in galactic small-scale dynamos

Axel Brandenburg, Hongzhe Zhou, Ramkishor Sharma

The magnetic fields in galaxy clusters and probably also in the interstellar medium are believed to be generated by a small-scale dynamo. Theoretically, during its kinematic stage,…

physics.plasm-ph2022★ 28 cited

Scaling of the Hosking integral in decaying magnetically-dominated turbulence

Hongzhe Zhou, Ramkishor Sharma, Axel Brandenburg

The Saffman helicity invariant of Hosking and Schekochihin (2021, PRX 11, 041005), which we here call the Hosking integral, has emerged as an important quantity that may govern the…

astro-ph.CO2022★ 10 cited

Low frequency tail of gravitational wave spectra from hydromagnetic turbulence

Ramkishor Sharma, Axel Brandenburg

Hydrodynamic and magnetohydrodynamic turbulence in the early Universe can drive gravitational waves (GWs) and imprint their spectrum onto that of GWs, which might still be observab…

astro-ph.CO2021★ 2 cited

Simulations of helical inflationary magnetogenesis and gravitational waves

Axel Brandenburg, Yutong He, Ramkishor Sharma

Using numerical simulations of helical inflationary magnetogenesis in a low reheating temperature scenario, we show that the magnetic energy spectrum is strongly peaked at a partic…

astro-ph.CO2021★ 15 cited

Simulating relic gravitational waves from inflationary magnetogenesis

Axel Brandenburg, Ramkishor Sharma

We present three-dimensional direct numerical simulations of the production of magnetic fields and gravitational waves (GWs) in the early Universe during a low energy scale matter-…

astro-ph.CO2021★ 11 cited

Constraining models of Inflationary Magnetogenesis with NANOGrav

Ramkishor Sharma

Generation of magnetic field during inflation can explain its presence over a wide range of scales in the Universe. In Ref.\cite{sharma2017}, we proposed a model to generate these…

astro-ph.CO2020★ 3 cited

Imprints of the post recombination dissipation of helical magnetic field on the Cosmic Microwave Background Radiation

Sandhya Jagannathan, Ramkishor Sharma, T. R. Seshadri

Astrophysical magnetic fields decay primarily via two processes namely, ambipolar diffusion and turbulence. Constraints on the strength and the spectral index of non-helical magnet…

astro-ph.CO2019★ 22 cited

Gravitational wave generation in a viable scenario of inflationary magnetogenesis

Ramkishor Sharma, Kandaswamy Subramanian, T. R. Seshadri

Generation of magnetic fields during inflation is a promising mechanism for the origin of the observed large scale magnetic fields in the universe. Among several attempts, a popula…

astro-ph.CO2018★ 3 cited

Scalar spectral index in the presence of Primordial Black Holes

Gaveshna Gupta, Ramkishor Sharma, T. R. Seshadri

We study the possibility of reheating the universe in its early stages through the evaporation of Primordial Black Holes (PBHs) that are formed due to the collapse of the inhomogen…

astro-ph.CO2018★ 69 cited

The generation of helical magnetic field in a viable scenario of Inflationary Magnetogenesis

Ramkishor Sharma, Kandaswamy Subramanian, T. R. Seshadri

We study the generation of helical magnetic fields in a model of inflationary magnetogenesis which is free from the strong coupling and back-reaction problems. To generate helical…

astro-ph.CO2017★ 78 cited

Challenges in Inflationary Magnetogenesis: Constraints from Strong Coupling, Backreaction and the Schwinger Effect

Ramkishor Sharma, Sandhya Jagannathan, T. R. Seshadri +1

Models of inflationary magnetogenesis with a coupling to the electromagnetic action of the form , are known to suffer from several problems. These include the str…

gr-qc2017★ 40 cited

Multifaceted Schwinger effect in de Sitter space

Ramkishor Sharma, Suprit Singh

We investigate particle production à la Schwinger mechanism in an expanding, flat de Sitter patch as is relevant for the inflationary epoch of our universe. Defining states and par…