Tanmay Kumar Poddar

ORCID: 0000-0002-9078-6224
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About
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Research Areas
  • Cosmology and Gravitation Theories
  • Dark Matter and Cosmic Phenomena
  • Pulsars and Gravitational Waves Research
  • Gamma-ray bursts and supernovae
  • Particle physics theoretical and experimental studies
  • Astrophysics and Cosmic Phenomena
  • Atomic and Subatomic Physics Research
  • Geophysics and Gravity Measurements
  • Neutrino Physics Research
  • Quantum Mechanics and Applications
  • Relativity and Gravitational Theory
  • Scientific Research and Discoveries
  • Radio Astronomy Observations and Technology
  • Solar and Space Plasma Dynamics
  • Black Holes and Theoretical Physics
  • Superconducting Materials and Applications
  • Astro and Planetary Science
  • Algebraic and Geometric Analysis
  • Quantum Electrodynamics and Casimir Effect
  • Computational Physics and Python Applications
  • Noncommutative and Quantum Gravity Theories
  • Radioactive Decay and Measurement Techniques
  • Advanced Frequency and Time Standards
  • Astronomy and Astrophysical Research

University of Salerno
2021-2025

Istituto Nazionale di Fisica Nucleare, Gruppo Collegato di Salerno
2024-2025

Istituto Nazionale di Fisica Nucleare
2021-2024

Tata Institute of Fundamental Research
2023-2024

Physical Research Laboratory
2019-2023

Indian Institute of Technology Gandhinagar
2020-2023

Federico Santa María Technical University
2021

Abstract The interaction of neutrinos with ultralight scalar and vector dark matter backgrounds induce a modification the neutrino dispersion relation. effects this are reviewed in framework asymmetric emission from supernova core, and, turn, pulsar kicks. We consider oscillations, focusing particular to active-sterile conversion. induced relation contains term form δ Ω · p̂ , where is related field unit along direction momentum. relative orientation p respect affects mechanism for...

10.1088/1475-7516/2024/01/069 article EN Journal of Cosmology and Astroparticle Physics 2024-01-01

Ultralight particles (${m}_{a}\ensuremath{\sim}{10}^{\ensuremath{-}21}--{10}^{\ensuremath{-}22}\text{ }\text{ }\mathrm{eV}$) with axionlike couplings to other can be candidates for fuzzy dark matter (FDM) if the axion decay constant ${f}_{a}\ensuremath{\sim}{10}^{17}\text{ }\mathrm{GeV}$. If a compact star is immersed in such low-mass axionic potential, it develops long-range field outside star. This radiated away when binary orbit. The orbital period of decays mainly due gravitational wave...

10.1103/physrevd.101.083007 article EN cc-by Physical review. D/Physical review. D. 2020-04-07

The orbital period of a compact binary system decays mainly due to quadrupole gravitational radiation, which agrees with the observation within 1%. Other types radiation such as ultralight scalar or pseudoscalar and massive vector boson also contribute decay long mass emitted particle is less than frequency system. We obtain an expression energy loss field from neutron star--neutron star star--white dwarf binaries. Because large chemical potential degenerate electrons, stars (NSs) have muon...

10.1103/physrevd.100.123023 article EN cc-by Physical review. D/Physical review. D. 2019-12-30

Abstract The standard model leptons can be gauged in an anomaly free way by three possible gauge symmetries namely $${L_e-L_\mu }$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:msub> <mml:mi>L</mml:mi> <mml:mi>e</mml:mi> </mml:msub> <mml:mo>-</mml:mo> <mml:mi>μ</mml:mi> </mml:mrow> </mml:math> , $${L_e-L_\tau <mml:mi>τ</mml:mi> and $${L_\mu -L_\tau . Of these, forces mediate between the Sun planets change perihelion precession of planetary orbits. It is well...

10.1140/epjc/s10052-021-09078-9 article EN cc-by The European Physical Journal C 2021-04-01

If an ultralight scalar interacts with the electromagnetic fields of a compact rotating star, then long-range field is developed outside star. The Coulomb-like profile equivalent to effective charge on In binary star system, scalar-induced would result in force between stars, acting as mediator. scalar-photon interactions modify Maxwell's equations for vacuum, resulting modified dispersion relation. This could be observed apparent redshift photons emitted by such sources. also induce...

10.48550/arxiv.2501.02286 preprint EN arXiv (Cornell University) 2025-01-04

We study the effect of Spontaneous Lorentz Symmetry Breaking (SLSB) on Primordial Gravitational Waves (PGWs) generated during inflation. The SLSB is induced by a time-like Bumblebee vector field which non-minimally coupled to Ricci tensor in Friedmann-Lema\^itre-Robertson-Walker (FLRW) background. power spectrum and GW amplitude are computed investigate how violation leaves observable imprints. Our analysis contrasts Lorentz-violating cosmology with standard context primordial generation....

10.48550/arxiv.2501.14395 preprint EN arXiv (Cornell University) 2025-01-24

We obtain novel constraints on new scalar fields interacting with Standard Model fermions through Lorentz-violating couplings, bridging searches for particles and Lorentz-symmetry tests. These arise from torsion-balance experiments, magnetometer searches, an excessive energy loss in Red Giant stars. Torsion-balance experiments impose stringent constraints, benefitting large macroscopic sources such as the Earth, Moon, Sun. Magnetometer-based which detect pseudo-magnetic spin precession,...

10.48550/arxiv.2502.05263 preprint EN arXiv (Cornell University) 2025-02-07

Abstract Dark matter (DM) within the solar system induces deviations in geodetic drift of a gyroscope spin due to its gravitational interaction. Considering constant DM density as minimal scenario, we constrain overdensity Gravity Probe B (GP-B) orbit around Earth and for Earth's Neptune's orbits Sun. The presence electrons gravitating sources test objects introduces an electrophilic scalar-mediated Yukawa potential, which can be probed from measurement well using terrestrial space-based...

10.1088/1475-7516/2025/03/049 article EN cc-by Journal of Cosmology and Astroparticle Physics 2025-03-01

Abstract Theories with massive gravitons have peculiarity called the van Dam-Veltman-Zakharov discontinuity in that theory propagator does not go to massless graviton zero mass limit. This results large deviation Newtons law for theories even when vanishes. We test vDVZ single vertex process namely gravitational radiation from a classical source. calculate compact binaries using perturbative Feynman diagram method. perform this calculation Einstein's gravity and verify reproduces quadrupole...

10.1088/1475-7516/2022/03/019 article EN Journal of Cosmology and Astroparticle Physics 2022-03-01

Rotating neutron star or pulsar can be a possible source of pseudo Nambu Goldstone bosons axions which mediate long range axionic hair outside the pulsar. When electromagnetic radiation is emitted from and passes through axion hair, rotates polarization produces birefringence. We obtain angle birefringence due to this as $0.42^\circ$. This result independent rotational frequency, radius pulsar, mass axion, photon coupling constant. value within accuracy measuring linear light $\leq...

10.1103/physrevd.102.083029 article EN cc-by Physical review. D/Physical review. D. 2020-10-27

Ultralight axion like particles (ALPs) of mass $m_a\in (10^{-21}\rm{eV}-10^{-22}\rm{eV})$ with decay constant $f_a\sim 10^{17}\rm{GeV}$ can be candidates for fuzzy dark matter (FDM). If celestial bodies Earth and Sun are immersed in a low axionic FDM potential if the ALPs have coupling nucleons then coherent oscillation field results long range hair outside bodies. The mediated Yukawa type fifth force is determined by distance between which fixes upper bound as $m_a\lesssim10^{-18}\rm{eV}$....

10.1088/1475-7516/2021/09/041 article EN Journal of Cosmology and Astroparticle Physics 2021-09-01

The geodetic and frame-dragging effects are the direct consequences of spacetime curvature near Earth which can be probed from Gravity probe B (GP-B) satellite. satellite result matches quite well with Einstein's general relativistic result. gyroscope measures contains lots electrons nucleons. Ultralight axions, vector gauge bosons, unparticles interact these nucleons through different spin-dependent spin-independent operators change drift rate gyroscope. Some ultralight particles either...

10.1140/epjc/s10052-022-10956-z article EN cc-by The European Physical Journal C 2022-11-01

We consider a general, anomaly free U(1)′ extension of the Standard Model (SM) where neutrino mass is generated at tree level via inverse seesaw mechanism. The model contains three right handed neutrinos, additional singlet fermions, one extra complex scalar and neutral gauge boson (Z′). Instead resorting to specific U(1) extension, we class models by taking charges scalars be parameters. Here, assign pair pseudo-Dirac degenerate sterile neutrinos as Dark Matter (DM) candidates which are...

10.1016/j.nuclphysb.2024.116568 article EN cc-by Nuclear Physics B 2024-05-22

The pair annihilation of neutrinos $(\nu\overline{\nu}\rightarrow e^+e^-)$ can energize violent stellar explosions such as gamma ray bursts (GRBs). energy in this neutrino heating mechanism be further enhanced by modifying the background spacetime over that Newtonian spacetime. However, one cannot attain maximum GRB $(\sim 10^{52}~\rm{erg})$ either or Schwarzschild and Hartle-Thorne background. On other hand, using modified gravity theories Quintessence field geometries, reached. In paper,...

10.1140/epjc/s10052-023-11367-4 article EN cc-by The European Physical Journal C 2023-03-17

We analyze the effect of dark large mixing angle (DLMA) solution on effective Majorana mass (${m}_{\ensuremath{\beta}\ensuremath{\beta}}$) governing neutrinoless double beta decay ($0\ensuremath{\nu}\ensuremath{\beta}\ensuremath{\beta}$) in presence a sterile neutrino. consider $3+1$ picture, comprised one additional check that Mikheyev-Smirnov-Wolfenstein resonance Sun can take place DLMA parameter space this scenario. Next, we investigate how values solar ${\ensuremath{\theta}}_{12}$...

10.1103/physrevd.102.015020 article EN cc-by Physical review. D/Physical review. D. 2020-07-21

An ultralight axion like particle (ALP) can mediate a macroscopic force with long-range monopole-dipole interactions between the Earth and Sun, if is treated as polarized source. Because of geomagnetic field, there exists an estimated ${10}^{42}$ electrons within Earth. These electrons, in state, interact unpolarized nucleons giving rise to potential Sun-Earth system. This phenomenon ultimately influences trajectories light celestial bodies, resulting observable effects such gravitational...

10.1103/physrevd.108.103024 article EN cc-by Physical review. D/Physical review. D. 2023-11-14

We consider a general, anomaly free U$(1)^\prime$ extension of the Standard Model (SM) where neutrino mass is generated at tree level via inverse seesaw mechanism. The model contains three right handed neutrinos, additional singlet fermions, one extra complex scalar and neutral gauge boson $(Z^\prime)$. Instead resorting to specific $U(1)$ extension, we class models by taking $U(1)^\prime$ charges scalars be parameters. Here, assign pair pseudo-Dirac degenerate sterile neutrinos as Dark...

10.48550/arxiv.2104.13986 preprint EN other-oa arXiv (Cornell University) 2021-01-01

Ultralight electrophilic scalar field can mediate a long-range force or radiate from pulsar magnetar if the has coupling with Goldreich-Julian charge density net electron of star. The interaction profile results in spatial variation mass. A induced magnetic is created due to such interaction. mass cases constrained by radius also binary system an isolated star less than orbital frequency and spin respectively. radiation contribute period loss systems spin-down. Comparing existing projected...

10.48550/arxiv.2404.18309 preprint EN arXiv (Cornell University) 2024-04-28

The high speeds seen in rapidly rotating pulsars after supernova explosions present a longstanding puzzle astrophysics. Numerous theories have been suggested over the years to explain this sudden &amp;quot;kick&amp;quot; imparted neutron star, yet each comes with its own set of challenges and limitations. Key explanations for pulsar kicks include hydrodynamic instabilities supernovae, anisotropic neutrino emission, asymmetries magnetic field, binary system disruption, physics beyond Standard...

10.20944/preprints202411.1370.v1 preprint EN 2024-11-19

The high speeds seen in rapidly rotating pulsars after supernova explosions present a longstanding puzzle astrophysics. Numerous theories have been suggested over the years to explain this sudden "kick" imparted neutron star, yet each comes with its own set of challenges and limitations. Key explanations for pulsar kicks include hydrodynamic instabilities supernovae, anisotropic neutrino emission, asymmetries magnetic field, binary system disruption, physics beyond Standard Model. Unraveling...

10.48550/arxiv.2412.08446 preprint EN arXiv (Cornell University) 2024-12-11

Dark matter (DM) within the solar system induces deviations in geodetic drift of gyroscope spin due to its gravitational interaction. Assuming a constant DM density as minimal scenario, we constrain overdensity Gravity Probe B (GP-B) orbit and project limits for Earth's Neptune's orbits around Sun. The presence electrons gravitating sources test objects introduces scalar-mediated Yukawa potential, which can be probed using terrestrial space--based precision clocks. We derive projected...

10.48550/arxiv.2412.09575 preprint EN arXiv (Cornell University) 2024-12-12
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