Oem Trivedi
Current Organizations / Institutes
The organizations/institutes from the scholar's latest article
Research Subjects
Oem Trivedi has a total of 45 co-authors. Here are the top co-authors by number of shared publications:
- Maxim Yu. Khlopov
Institute of Physics, Southern Federal University, 194 Stachki, Rostov-on-Donu, Russia
14 shared publications - Abraham Loeb
Harvard University
9 shared publications - Alexander V. Timoshkin
Institute of Scientific Research and Development, Tomsk State Pedagogical University (TSPU), Tomsk, Russia
5 shared publications - Paulo Vargas Moniz
Universidade da Beira Interior
5 shared publications - Robert J. Scherrer
Vanderbilt University
5 shared publications - Ayush Bidlan
Department of Physics Sardar Vallabhbhai National Institute of Technology 395007 Surat Gujarat India
3 shared publications
Latest Publications
- Open Access
- 25 August 2026
- Published by Elsevier in Nuclear Physics B
- Vol. 1031
Nonlinear dynamical regimes of cosmological frequency combs
- 25 August 2026
- Published by Elsevier in Nuclear Physics B
- Vol. 1031
Open AccessNonlinear dynamical regimes of cosmological frequency combs
- Open Access
- 19 August 2026
- Published by Elsevier in Physics of the Dark Universe
- Vol. 53
Dark matter deficient galaxies as probes of dark matter
- 19 August 2026
- Published by Elsevier in Physics of the Dark Universe
- Vol. 53
Open AccessDark matter deficient galaxies as probes of dark matter
- 6 August 2026
- Published by American Physical Society (APS) in Physical Review D
- Vol. 114 (4)
Non-Hermitian quantum mechanics with applications to gravity
- 6 August 2026
- Published by American Physical Society (APS) in Physical Review D
- Vol. 114 (4)
Non-Hermitian quantum mechanics with applications to gravity
- Open Access
- 30 July 2026
- Published by Springer Nature in The European Physical Journal C
- Vol. 86 (7) , 900
Atomic clock constraints on locally coupled scalar dark energy
We show that atomic clock measurements constrain the locally accessible scalar clock combination $$\Delta k_\textrm{eff}\sqrt{1+w_0}$$ for scalar dark energy models coupled to Standard Model sectors. Under the benchmark assumption of weak environmental suppression and an effective scalar clock sensitivity $$\Delta k_\textrm{eff}\sim 10^{-5}$$ , the inferred constraint corresponds to $$1+w_0\sim 10^{-4}-10^{-5}$$ with a Monte Carlo median $$1+w_0\simeq 9.4\times 10^{-5}$$ . More conservatively, the result should be interpreted as an exclusion surface in the joint parameter space of scalar coupling, environmental matching, and dark energy dynamics. In this form, atomic clocks and Solar System tests provide a powerful local consistency test for scalar-tensor dark energy, forcing near $$\Lambda $$ behavior whenever the same scalar remains locally active and appreciably coupled.- 30 July 2026
- Published by Springer Nature in The European Physical Journal C
- Vol. 86 (7) , 900
Open AccessAtomic clock constraints on locally coupled scalar dark energy
We show that atomic clock measurements constrain the locally accessible scalar clock combination $$\Delta k_\textrm{eff}\sqrt{1+w_0}$$ for scalar dark energy models coupled to Standard Model sectors. Under the benchmark assumption of weak environmental suppression and an effective scalar clock sensitivity $$\Delta k_\textrm{eff}\sim 10^{-5}$$ , the inferred constraint corresponds to $$1+w_0\sim 10^{-4}-10^{-5}$$ with a Monte Carlo median $$1+w_0\simeq 9.4\times 10^{-5}$$ . More conservatively, the result should be interpreted as an exclusion surface in the joint parameter space of scalar coupling, environmental matching, and dark energy dynamics. In this form, atomic clocks and Solar System tests provide a powerful local consistency test for scalar-tensor dark energy, forcing near $$\Lambda $$ behavior whenever the same scalar remains locally active and appreciably coupled. - Open Access
- 21 July 2026
- Published by Elsevier in Physics of the Dark Universe
- Vol. 53
Unique gravitational-wave signals from negative mass binaries
- 21 July 2026
- Published by Elsevier in Physics of the Dark Universe
- Vol. 53
Open AccessUnique gravitational-wave signals from negative mass binaries
- Open Access
Accelerated Expansion of the Universe as a Quantum Gravity Phenomenon
It has been known for about hundred years that the universe is expanding, but an impressive discovery came at the end of 20th century, when it was found that the universe is expanding with acceleration. Since then, many models have been developed in cosmology to explain this phenomenon. One of the possible elucidations is that the theory of gravity must be modified at the classical level. However, many such models have already been excluded by gravitational wave experiments. Therefore, one must put a more critical question: could accelerated expansion of the universe be a phenomenon of quantum gravity? Here, we review the basic models of how one explains the origin of dark energy or the cosmological constant in metastring theory, discrete approaches to quantum gravity, group field theory, non-commutative geometry, causal dynamical triangulation, asymptotic safety, and models based on holography and entropic gravity. At the end of a newly formed approach to the quantization of gravity, we mention the ring paradigm, which may, after application to cosmology, naturally model the late-time accelerated expansion epoch in the universe. What is most remarkable, though, is that the final formulation of this theory may ultimately solve the old problem of the cosmological constant.
Open AccessAccelerated Expansion of the Universe as a Quantum Gravity Phenomenon
It has been known for about hundred years that the universe is expanding, but an impressive discovery came at the end of 20th century, when it was found that the universe is expanding with acceleration. Since then, many models have been developed in cosmology to explain this phenomenon. One of the possible elucidations is that the theory of gravity must be modified at the classical level. However, many such models have already been excluded by gravitational wave experiments. Therefore, one must put a more critical question: could accelerated expansion of the universe be a phenomenon of quantum gravity? Here, we review the basic models of how one explains the origin of dark energy or the cosmological constant in metastring theory, discrete approaches to quantum gravity, group field theory, non-commutative geometry, causal dynamical triangulation, asymptotic safety, and models based on holography and entropic gravity. At the end of a newly formed approach to the quantization of gravity, we mention the ring paradigm, which may, after application to cosmology, naturally model the late-time accelerated expansion epoch in the universe. What is most remarkable, though, is that the final formulation of this theory may ultimately solve the old problem of the cosmological constant.
- Open Access
Machine Learning for Multi-Messenger Probes of New Physics and Cosmology: Review and Perspective
The multi-messenger exploration of dark matter and physics beyond the Standard Model has emerged as a central direction in modern astro-particle physics, particularly following the discovery of gravitational waves. In this work, we present a comprehensive review and forward-looking perspective on machine-learning-enhanced multi-messenger approaches, combining information from gravitational waves, cosmic rays, gamma rays, neutrinos, and collider experiments. We summarize the current state of the field, discuss recent methodological developments, and outline a coherent research program aimed at integrating heterogeneous datasets within a unified inference framework. We collaboratively propose a plan for forthcoming analyses aiming at extracting information on the properties and interactions of dark matter, and finally on its genesis, combining multi-messenger astronomy techniques and inputs from laboratory physics. The main objectives planned in this line of research comprise: (i) the multi-messenger analysis of new physics in cosmology, including mainly, but not only, several different models of dark matter; (ii) the phenomenology of new physics signatures in ground-based cosmic rays experiments, with cross-correlation to the corresponding physical, astrophysical and cosmological observations; (iii) the development of machine learning methods for data analysis in ground-based cosmic rays experiments, in light of the new physics signatures. We note that several groups have explored the use of multi-messenger observations, including gravitational waves, to probe alternative dark matter candidates. The present work builds on these developments by focusing on the role of machine learning in integrating heterogeneous datasets. We foresee that a cross-fertilizing approach combining the information that arises from very different experimental methodologies will represent the right and successful path to extract information about the very elusive dark matter particles and provide answers to the main questions that are left in fundamental physics.
Open AccessMachine Learning for Multi-Messenger Probes of New Physics and Cosmology: Review and Perspective
The multi-messenger exploration of dark matter and physics beyond the Standard Model has emerged as a central direction in modern astro-particle physics, particularly following the discovery of gravitational waves. In this work, we present a comprehensive review and forward-looking perspective on machine-learning-enhanced multi-messenger approaches, combining information from gravitational waves, cosmic rays, gamma rays, neutrinos, and collider experiments. We summarize the current state of the field, discuss recent methodological developments, and outline a coherent research program aimed at integrating heterogeneous datasets within a unified inference framework. We collaboratively propose a plan for forthcoming analyses aiming at extracting information on the properties and interactions of dark matter, and finally on its genesis, combining multi-messenger astronomy techniques and inputs from laboratory physics. The main objectives planned in this line of research comprise: (i) the multi-messenger analysis of new physics in cosmology, including mainly, but not only, several different models of dark matter; (ii) the phenomenology of new physics signatures in ground-based cosmic rays experiments, with cross-correlation to the corresponding physical, astrophysical and cosmological observations; (iii) the development of machine learning methods for data analysis in ground-based cosmic rays experiments, in light of the new physics signatures. We note that several groups have explored the use of multi-messenger observations, including gravitational waves, to probe alternative dark matter candidates. The present work builds on these developments by focusing on the role of machine learning in integrating heterogeneous datasets. We foresee that a cross-fertilizing approach combining the information that arises from very different experimental methodologies will represent the right and successful path to extract information about the very elusive dark matter particles and provide answers to the main questions that are left in fundamental physics.
- Open Access
- 29 June 2026
- Published by Elsevier in Physics Letters B
- Vol. 879
Does cosmology require Hermiticity in quantum mechanics?
- 29 June 2026
- Published by Elsevier in Physics Letters B
- Vol. 879
Open AccessDoes cosmology require Hermiticity in quantum mechanics?
- 19 June 2026
- Published by World Scientific Pub Co Pte Ltd in International Journal of Modern Physics D
Polymer Network Cosmology and the Dark Sector
We develop Polymer Network Cosmic Teleodynamics (PNCT), a covariant effective framework in which the cosmic web is modeled as a percolating, memory-bearing, self-gravitating network whose constitutive response is guided by viscoelastic polymer physics. Affine filament stretching, transverse tidal confinement, and nonlocal strain memory generate, respectively, an effective dark energy-like background component, environment-dependent clustering corrections, and a history-dependent teleodynamic bias functional. The central structural event is a sol-gel-like percolation transition at z * ∼ 1-2, after which a coherent spanning web stores elastic free energy and can drive late-time acceleration. The resulting effective equation of state exhibits a three-stage trajectory, including phantom-like growth near activation, phantom divide crossing as transverse coherence is lost, and relaxation toward w TD → −1 + through gravitational saturation and post-gel strand balance. The framework predicts two testable observables: synchronization between cosmic web percolation and dark sector activation, and environment-dependent growth/lensing residuals in nodes, filaments, walls, and voids. These signatures are testable with DESI, Euclid, Roman, and LSST and would distinguish PNCT from smooth dark energy models and generic scale-dependent modified gravity.
- 19 June 2026
- Published by World Scientific Pub Co Pte Ltd in International Journal of Modern Physics D
Polymer Network Cosmology and the Dark Sector
We develop Polymer Network Cosmic Teleodynamics (PNCT), a covariant effective framework in which the cosmic web is modeled as a percolating, memory-bearing, self-gravitating network whose constitutive response is guided by viscoelastic polymer physics. Affine filament stretching, transverse tidal confinement, and nonlocal strain memory generate, respectively, an effective dark energy-like background component, environment-dependent clustering corrections, and a history-dependent teleodynamic bias functional. The central structural event is a sol-gel-like percolation transition at z * ∼ 1-2, after which a coherent spanning web stores elastic free energy and can drive late-time acceleration. The resulting effective equation of state exhibits a three-stage trajectory, including phantom-like growth near activation, phantom divide crossing as transverse coherence is lost, and relaxation toward w TD → −1 + through gravitational saturation and post-gel strand balance. The framework predicts two testable observables: synchronization between cosmic web percolation and dark sector activation, and environment-dependent growth/lensing residuals in nodes, filaments, walls, and voids. These signatures are testable with DESI, Euclid, Roman, and LSST and would distinguish PNCT from smooth dark energy models and generic scale-dependent modified gravity.