25 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR3 papers
- Indian Institute of AstrophysicsIN3 papers
- Raman Research InstituteIN3 papers
- Commonwealth Scientific and Industrial Research OrganisationAU2 papers
- Indian Institute of Science BangaloreIN2 papers
- Institut de PhysiqueFR2 papers
- Institut de Physique des 2 Infinis de LyonFR2 papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR2 papers
- International Centre for Theoretical SciencesIN2 papers
- Lyon 1 UniversitéFR2 papers
- National Radio Astronomy ObservatoryUS2 papers
- Ravenshaw UniversityIN2 papers
5 papers · 1 filter
Invariants in Polarimetric Interferometry: a non-Abelian Gauge Theory
Joseph Samuel, Rajaram Nityananda, Nithyanandan Thyagarajan
The discovery of magnetic fields close to the M87 black hole using Very Long Baseline Interferometry (VLBI) by the Event Horizon Telescope collaboration utilized the novel concept…
Invariants in Co-polar Interferometry: an Abelian Gauge Theory
Nithyanandan Thyagarajan, Rajaram Nityananda, Joseph Samuel
An -element interferometer measures correlations among pairs of array elements. Closure invariants associated with closed loops among array elements are immune to multiplicative…
Testing charge-radius coupling of the composite Higgs boson at hadron colliders
G. Cacciapaglia, S. Gascon-Shotkin, A. Lesauvage +2
We explore the collider relevance of a charge-radius coupling among light mesons in composite Higgs models. In particular, we focus of a coupling of the photon to the composite Hig…
Tera-Zooming in on light (composite) axion-like particles
G. Cacciapaglia, A. Deandrea, A. M. Iyer +1
The Tera-Z phase of future colliders, FCC-ee and CepC, is a goldmine for exploring portal physics. We focus on axion-like particles (ALPs) that can be produced via $Z…
A geometric method to locate Neptune
Siddharth Bhatnagar, Jayanth P. Vyasanakere, Jayant Murthy
We develop a direct geometric method to determine the orbital parameters and mass of a planet, and we then apply the method to Neptune using high-precision data for the other plane…