学术报告

本次会议共收录 601 篇报告,分布于 60 个分会。可按标题、作者或正文关键词检索。

共 601 条结果

  1. Asymptotically Schwarzschild solutions in f(R) extension of General Relativity

    Federico Scali · Oliver Fabio Piattella

    section Milan We consider the gravitational field outside a static, spherically symmetric source in the context of a general f(R) extension of General Relativity. We study the modified Einstein equations (EE), which involve the two free potentials of the metri

    AT2报告ICRANet Seminar Room

  2. Auto-stabilized Electron

    Munawar Karim

    We propose a theory to explain the mechanism that stabilizes an electron. We show that the intrinsic divergences that occur in quantum electrodynamics can be removed by casting it within general relativity. The infinities are compensated by the curvature creat

    TF1报告Sala 7

  3. Avoiding Singularities with Propagating Torsion

    Luca Fabbri · Swati Gavas · Jasjeet Bagla · Nishikanta Khandai

    We consider the torsional completion of the theory of gravity in which torsion is a propagating axialvector field: we show how this changes the energy conditions leading to the singularity formation being avoided. We discuss how the same construction possesses

    AT1报告Sala 7

  4. BIack Holes and Massive Galaxies in the Early Universe

    Felix Mirabel

    Recent observations with the JWST and ALMA have identified at z > 10 massive star forming galaxies of up to 1011 solar masses that are already quench at z > 3. The very early formation and rapid evolution of massive galaxies produced great surprise, because it

    PLENARY全体报告Sala Auditorium (Plenary)

  5. Bayesian analysis for rotational curves with l-boson stars as a dark matter component

    Argelia Bernal Bautista · Atalia Navarro-Boullosa · J. Alberto Vázquez

    Using Low Brightness Surface Galaxies (LBSG) rotational curves we inferred the free parameters of l-boson stars as a dark matter component. The l-boson stars are numerical solutions to the nonrelativistic limit of the Einstein-Klein-Gordon system, the Schrödin

    DM3报告Sala 9

  6. Bayesian parameter estimation of continuous gravitational waves from known pulsars

    Anjana Ashok · Maria Alessandra Papa · Pep Covas Vidal · Reinhard Prix

    Continuous gravitational wave (CW) searches targeted at known pulsars utilize electromagnetic observations of the sources to infer the phase-evolution parameters of the gravitational wave signal. We present a new method to perform Bayesian estimation of the am

    MA1报告Sala 9

  7. Bethe-Heitler constraints on proton synchrotron models for GRBs.

    Damien Begue

    GRB spectra seem to be well fitted by models based on marginally fast-cooled synchrotron radiation. This observation challenges the synchrotron process as a viable mechanism as it leads to (too) large emission radii and (too) large bulk Lorentz factors. To ove

    GB2报告Sala 3

  8. Beyond ANTARES: the future of neutrino telescopes, a short review

    Vincent Cecchini

    The observation of neutrinos of cosmic origin opens a whole new field for neutrino astrophysics. This quest has been paved by pioneering experiments in the second half of the 20th century and is now at the dawn of a new era thanks to numerous new proposals. In

    NU1报告ICRANet Seminar Room

  9. Beyond Early Dark Energy: an EFT-based approach to cosmological tensions

    Giampaolo Benevento

    The Transitional Planck Mass (TPM) model is a useful application of the Effective Field Theory of Dark Energy and Modified Gravity, characterized by a step-like transition in the Planck Mass at cosmological scales. This transition, occurring during the radiati

    CM2报告Sala 7

  10. Bi-twistors: an extension of twistor theory for general space-times

    Sandro MereghettiNone

    Twistor theory was initially developed to describe the geometry of Minkowski space-time in terms of its null geodesics. The natural generalization to curved space-times requires the ubiquitous existence of α-surfaces, this requiring the Weyl curvature to be an

    PLENARY全体报告Sala Auditorium (Plenary)

  11. Big Bang Nucleosynthesis constraints on f(T, T ) gravity

    SAI SWAGAT MISHRA · Ameya Kolhatkar · Pradyumn Kumar Sahoo

    Big Bang Nucleosynthesis provides us with an observational insight into the very early Universe. Since this mechanism of light element synthesis comes out of the standard model of particle cosmology which follows directly from General Relativity, it is expecte

    EU1报告Sala 5

  12. Black hole explosions in loop quantum gravity

    Francesco Fazzini

    Effective models of gravitational collapse in loop quantum gravity for the Lemaître-Tolman-Bondi spacetime predict that collapsing matter reaches a maximum finite density, bounces, and then expands outwards. I explain how in the marginally bound case, shell-cr

    QG1报告Sala 7

  13. Black hole thermodynamics and boundary terms

    Marek Liška · David Kubiznak · Robie A. Hennigar

    I discuss sensitivity of black hole thermodynamics to certain boundary terms in the action. While boundary terms cannot affect the classical gravitational dynamics, they apparently influence both the black hole entropy and temperature. Remarkably, this behavio

    BH2报告Sala 2

  14. Black holes in a modified gravity: Hawking radiation and cosmological implications

    Banibrata Mukhopadhyay · Panchajanya Dey

    There are observations supporting the plausible modification to Einstein gravity, while the exact theory of gravity in the strong field regime is indeed under debate. We obtain a new black hole solution in an f(R)-gravity-based modified gravity. Such a black h

    BH2报告Sala 2

  15. Black holes in alternative gravity theories

    Jutta Kunz-Drolshagen

    In our quest towards a theory of gravity beyond General Relativity black holes with their strong gravitational fields represent an important testing ground. Among the numerous alternative theories of gravity much work in recent years has focused on a set of sc

    PLENARY全体报告Sala Auditorium (Plenary)

  16. Blandford-Znajek power as a strong-gravity signature

    Filippo Camilloni

    The Blandford-Znajek (BZ) mechanism is an electromagnetic manifestation of the Penrose process that currently constitutes the best theoretical candidate to explain the launching of relativistic jets by black holes. In this talk we offer a modern review about t

    AC1报告Sala 2

  17. Boson stars and their relatives in semiclassical gravity

    Alberto Diez-Tejedor · Argelia Bernal · Darío Núñez · Juan Barranco · Juan Carlos Degollado · Miguel

    We construct boson star configurations in quantum field theory using the semiclassical gravity approximation. Restricting our attention to the static case, we show that the semiclassical Einstein- Klein- Gordon system for a single real quantum scalar field who

    QG5报告Sala 4

  18. Bubble universe from flat spaces

    Eduardo Guendelman

    We show by matching two flat spaces one in Minkowski coordinates ( empty space) and the other in Minkowski coordinates after a special conformal transformation (also empty space) through a bubble with positive and constant surface tension, that the motion of t

    EU1报告Sala 6