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101
Phenomenology of MaVaN’s Models in Reactor Neutrino Data
Published 2013-01-01“…In some scenarios, this mass can present a dependence on the baryonic density felt by neutrinos, creating an effective neutrino mass that depends both on the neutrino and baryonic densities. …”
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102
Dynamics of Mixed Dark Energy Domination in Teleparallel Gravity and Phase-Space Analysis
Published 2015-01-01“…Here we propose a mixed dark energy domination which is constituted by tachyon, quintessence, and phantom scalar fields nonminimally coupled to gravity, in the absence of background dark matter and baryonic matter, in the framework of teleparallel gravity. …”
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103
Measurement of p−𝚵− (p - 𝚵+) Correlation Function in Isobar and Au+Au Collisions at √sNN = 200 GeV with the STAR Detector
Published 2025-01-01“…Understanding the strong interactions between baryons, especially hyperon-nucleon (Y-N) interactions, is crucial for comprehending the equation-of-state (EoS) of the nuclear matter and inner structure of neutron star. …”
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104
Bayesian location of the QCD critical point: A holographic perspective
Published 2025-01-01“…We employ two different parametrizations of the functions that characterize the breaking of conformal invariance and the baryonic charge in the Einstein-Maxwell-dilaton holographic model. …”
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105
The Master Space of Supersymmetric Gauge Theories
Published 2010-01-01“…We demonstrate that most of the information on the moduli space and spectrum of the quiver gauge theories is encoded in the concept of the “Master Space”, which is roughly the full moduli space for one brane, consisting of mesonic and baryonic degrees of freedom. We summarize the relevant information in generating functions for chiral operators, which can be computed using plethystics techniques and the language of complex geometry.…”
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106
Modified Newtonian Dynamics: A Falsification of Cold Dark Matter
Published 2009-01-01“…MOND may be viewed as an algorithm for calculating the distribution of force in an astronomical object from the observed distribution of baryonic matter. The fact that it works very well on the scale of galaxies is problematic for cold dark matter (CDM). …”
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107
Rapidity dependence of antideuteron coalescence in pp collisions at s=13 TeV with ALICE
Published 2025-01-01“…The pT and rapidity dependence of the obtained B2 is extrapolated for pT>1.7 GeV/c and |y|>0.7 using the phenomenological antideuteron production model implemented in Pythia 8.3 as well as a baryon coalescence afterburner model based on EPOS 3. …”
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108
Testing the lepton content of the proton at HERA and EIC
Published 2025-01-01“…Abstract Although protons are baryons with an overall vanishing lepton number, they possess a non-trivial leptonic content arising from quantum fluctuations which can be described by lepton parton distribution functions (PDFs) of the proton. …”
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109
Charm fragmentation fractions and $$\mathbf {c\overline{c}}$$ c c ¯ cross section in p–Pb collisions at $$\mathbf {\sqrt{s _{NN}}=5.02 TeV}$$ s NN = 5.02 TeV
Published 2024-12-01“…The measured fragmentation fractions are compatible with those measured in pp collisions at $$\sqrt{s} = 5.02$$ s = 5.02 and 13 TeV, showing an increase in the relative production rates of charm baryons with respect to charm mesons in pp and p–Pb collisions compared with $$\mathrm {e^{+}e^{-}}$$ e + e - and $$\mathrm {e^{-}p}$$ e - p collisions. …”
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110
Measurements of global and local spin polarization of Λ and Λ in Au+Au collisions from the RHIC Beam Energy Scan
Published 2025-01-01“…The net local polarization observable, Λ and Λ¯ and 〈P2,ynet> = 〈P2,y(Λ)〉 - 〈P2,y(Λ¯)〉 and 〈P2,znet〉 = 〈P2,z(Λ)〉 - 〈P2,z(Λ¯)〉 designed to probe baryonic spin Hall effect, is consistent with zero with large uncertainty.…”
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111
Stability of a Noncanonical Scalar Field Model during Cosmological Date
Published 2016-01-01“…In different epochs in the evolution of the Universe for different values of q and n, the potentials as a function of scalar field are attained. The behavior of baryonic perturbations in linear perturbation scenario as a considerable amount of energy density of scalar field at low redshifts prevents the growth of perturbations in the ordinary matter fluid. …”
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112
Heavy Scalar, Vector, and Axial-Vector Mesons in Hot and Dense Nuclear Medium
Published 2014-01-01“…The results of present investigations of medium modifications of scalar, vector, and axial-vector mesons at finite density and temperature can be verified in the compressed baryonic matter (CBM) experiment of FAIR facility at GSI, Germany.…”
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113
Dynamical systems of modified Gauss–Bonnet gravity: cosmological implications
Published 2025-01-01“…We utilize the dynamical system approach to study the cosmic dynamics of two different class of f(R, G) models composed of radiation and matter (cold dark matter and baryonic matter). The linear perturbations around the fixed points are studied to explore the corresponding stability of points. …”
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114
Detection of a New GeV Source in the Outer Region of the Coma Cluster: A Signature of External Accretion Shock?
Published 2025-01-01“…The supersonic flow motions associated with infall of baryonic gas toward sheets and filaments, as well as cluster mergers, produces large-scale shock waves. …”
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115
Simulating High-redshift Galaxies: Enhancing UV Luminosity with Star Formation Efficiency and a Top-heavy IMF
Published 2025-01-01“…To achieve this, we conduct cosmological hydrodynamic zoom-in simulations, modifying baryonic subgrid physics, and post-process our simulation results to confirm the observability of our simulated galaxies. …”
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