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  1. 301

    Bianchi Type-V Bulk Viscous Cosmic String in f(R,T) Gravity with Time Varying Deceleration Parameter by Bïnaya K. Bishi, K. L. Mahanta

    Published 2015-01-01
    “…We study the Bianchi type-V string cosmological model with bulk viscosity in f(R,T) theory of gravity by considering a special form and linearly varying deceleration parameter. …”
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    Article
  2. 302

    Warm Inflation with Nonminimal Derivative Coupling by Kourosh Nozari, M. Shoukrani, N. Rashidi

    Published 2014-01-01
    “…We present a detailed calculation of the cosmological perturbations in this setup. We use the recent observational data from the joint data set of WMAP9 + BAO + H0 and also the Planck satellite data to constrain our model parameters for natural and chaotic inflation potentials. …”
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  3. 303

    Localization of Energy-Momentum for a Black Hole Spacetime Geometry with Constant Topological Euler Density by Irina Radinschi, Theophanes Grammenos, Farook Rahaman, Andromahi Spanou, Marius Mihai Cazacu, Surajit Chattopadhyay, Antonio Pasqua

    Published 2018-01-01
    “…The energy is found to depend on the mass M and the charge q of the black hole, the cosmological constant Λ, and the radial coordinate r, while in both prescriptions all the momenta vanish. …”
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  4. 304

    Early matter domination at colliders: Long live the glueball! by Fady Bishara, Filippo Sala, Kai Schmidt-Hoberg

    Published 2025-02-01
    “…In this letter we concentrate on the specific example of glueballs from a GeV-scale confining dark sector and compute the dilution of cosmological relics induced by their decay. We then show that searches for long-lived glueballs from Higgs decays test increasing values of dilution at ATLAS and CMS, CODEX-b, ANUBIS and MATHUSLA. …”
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  5. 305

    Construct α′ corrected or loop corrected solutions without curvature singularities by Peng Wang, Houwen Wu, Haitang Yang, Shuxuan Ying

    Published 2020-01-01
    “…Abstract For the bosonic gravi-dilaton system, we provide systematical approaches to construct non-perturbative string cosmological solutions without curvature singularities, which can match the perturbative solution to any order in α′ expansion. …”
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    Article
  6. 306

    Wigner function method for the Gibbons–Hawking and the Unruh effect by Landau, Ziv, Leonhardt, Ulf

    Published 2024-11-01
    “…We found excellent Planck spectra for a class of realistic cosmological models, but also strongly non–Planckian, negative Wigner functions for a standard scenario testable with laboratory analogues.…”
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  7. 307

    More on the Non-Gaussianity of Perturbations in a Nonminimal Inflationary Model by R. Shojaee, K. Nozari, F. Darabi

    Published 2018-01-01
    “…We study nonlinear cosmological perturbations and their possible non-Gaussian character in an extended nonminimal inflation where gravity is coupled nonminimally to both the scalar field and its derivatives. …”
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    Article
  8. 308

    Thermodynamics of the substantial universe by V. Yu. Stetsenko

    Published 2024-06-01
    “…Based on thermodynamic calculations of the substantial Universe, it is shown that the cosmological theory of the Big Bang is erroneous. The thermodynamic ban on this theory makes the hypothesis of dark energy expanding the substantial Universe also erroneous. …”
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    Article
  9. 309

    Sangue de Lua: reflexôes sobre espíritos e eclipses by Carlos Fausto

    Published 2012-07-01
    “…Taking this ethnographic and cinematographic experience as his starting point, the author reflects on the meaning of the eclipse for the Kuikuro, focusing on the explicit cosmological knowledge conveyed by them, on the nature of their adherence to a belief system, and on some mytho-ritual themes that, lacking a native exegesis, can only be understood through a comparative perspective.…”
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  10. 310

    The Relation between the Quasi-Localized Energy-Momentum Complexes and the Thermodynamic Potential for the Schwarzschild-de Sitter Black Hole by I-Ching Yang

    Published 2017-01-01
    “…Here M is the patch between cosmological event horizon and black hole event horizon of the SdS black hole solution. …”
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  11. 311

    La part manquante du paysage by Valentine Losseau

    Published 2010-07-01
    “…In turn, the Lacandon Mayas who live in the forest transform their territory in a reflexive relationship...two cosmological, aestethical, cultural prisms are crossing the forest and redesigning its landscapes. …”
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    Article
  12. 312

    Energy Conditions in a Generalized Second-Order Scalar-Tensor Gravity by M. Sharif, Saira Waheed

    Published 2013-01-01
    “…The study of energy conditions has many significant applications in general relativistic and cosmological contexts. This paper explores the energy conditions in the framework of the most general scalar-tensor theory with field equations involving second-order derivatives. …”
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  13. 313

    La organización social de los mazahuas del Estado de México

    Published 2001-01-01
    “…This group posits their cosmological bases on a cultural matrix dating back to pre columbian and colonial times. …”
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    Article
  14. 314

    Black string solutions in Lifshitz spacetime by L. A. Lessa, J. E. G. Silva, J. Furtado

    Published 2025-01-01
    “…We have shown that a new class of asymptotically Lifshitz solutions can be generated by an Einstein–Maxwell-Dilaton theory with a cosmological constant. In the limit where we recover conformal scale invariance, we retrieve the usual black string solution. …”
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  15. 315

    Neutrinoless Double Beta Decay: 2015 Review by Stefano Dell’Oro, Simone Marcocci, Matteo Viel, Francesco Vissani

    Published 2016-01-01
    “…Also, experimental data coming from cosmological surveys are considered and their impact on 0νββ expectations is examined.…”
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  16. 316

    Modified Newtonian Dynamics: A Falsification of Cold Dark Matter by R. H. Sanders

    Published 2009-01-01
    “…This hypothesis, suggested by Milgrom, has been successful in explaining systematic properties of spiral and elliptical galaxies and predicting in detail the observed rotation curves of spiral galaxies with only one additional parameter—a critical acceleration which is on the order of the cosmologically interesting value of 𝑐𝐻𝑜. MOND may be viewed as an algorithm for calculating the distribution of force in an astronomical object from the observed distribution of baryonic matter. …”
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  17. 317

    Perihelion Precession and Deflection of Light in the General Spherically Symmetric Spacetime by Ya-Peng Hu, Hongsheng Zhang, Jun-Peng Hou, Liang-Zun Tang

    Published 2014-01-01
    “…We find that both the electric charge and f(R) gravity can affect the perihelion precession and deflection of light, while the cosmological constant can only effect the perihelion precession. …”
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  18. 318

    Images of person in an Amerindian society. An ethnographic account of Kuna woodcarving by Paolo Fortis

    Published 2012-07-01
    “…Explored through art the theme of alterity, both at the level of the person and the cosmological world, provides a framework to look at ideas of birth and death, and the centrality of kinship in the creation of human bodies.…”
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  19. 319

    Phase Transition of the Higher Dimensional Charged Gauss-Bonnet Black Hole in de Sitter Spacetime by Meng-Sen Ma, Li-Chun Zhang, Hui-Hua Zhao, Ren Zhao

    Published 2015-01-01
    “…For black holes in de Sitter spacetime, there is not only black hole horizon, but also cosmological horizon. The thermodynamic quantities on both horizons satisfy the first law of the black hole thermodynamics, respectively; moreover, there are additional connections between them. …”
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  20. 320

    Conformally Flat Pseudoprojective Symmetric Spacetimes in fR,G Gravity by Uday Chand De, Sameh Shenawy, Abdallah Abdelhameed Syied, Nasser Bin Turki

    Published 2022-01-01
    “…Finally, we investigate conformally flat  PPS4 spacetimes and conformally flat  PPS4 perfect fluids in fR,G theory of gravity, and amongst many results, it is proved that the isotropic pressure and the energy density of conformally flat perfect fluid  PPS4 spacetimes are constants and such perfect fluid behaves like a cosmological constant. Further, in this setting, we consider some energy conditions.…”
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