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. Updates on the ZAIGA project

    Dongfeng Gao

    ZAIGA (the Zhaoshan long-baseline Atom Interferometer Gravitation Antenna) is a proposed underground long-baseline atom interferometer (AI) facility, aiming for experimental research on gravitation and related problems. It includes gravitational wave detection

    GW3报告Sala 9

  2. Useful Predictions from the 5D Vacuum Equation

    Detlef Hoyer

    Abstract. Since the work of Kaluza it has been known that Maxwell’s equations are mathematically a subset of the Ricci curvature tensor in five dimensions. In the present paper a complete set of equations for the 5D Ricci curvature tensor is described that rep

    TF1报告Sala 7

  3. Using mHz gravitational waves to catch galactic center mergers of supermassive dark matter cores

    Carlos Raúl Argüelles · Jorge Armando Rueda Hernandez · Jose Fernando Rodriguez Ruiz · Remo Ruffini

    There is an open debate about whether some galactic centers (including Sgr A*) could actually be supermassive dark matter cores made of fermions with masses in the range of 60-350 keV. We discuss the possibility of pinpointing mergers of such cores using mHz g

    GW4报告ICRANet Seminar Room

  4. Vacuum Energy from Qubit Entropy

    Gonçalo Quinta · PRIYANKA SAHA · Dipanjan Dey

    We develop a non-conventional description of the vacuum energy in quantum field theory in terms of quantum entropy. Precisely, we show that the vacuum energy of any non-interacting quantum field at zero temperature is proportional to the quantum entropy of the

    QG5报告Sala 4

  5. Vacuum dynamics in the Universe: implications on the cosmological tensions

    Joan Solà Peracaula · Joan Solà Peracaula · Cristian Moreno Pulido

    The possibility that the vacuum energy density (VED) could be time dependent in the expanding Universe is intuitively more reasonable than just a rigid cosmological constant for the entire cosmic history. The framework of the running vacuum model (RVM) is a re

    CM2报告Sala 6

  6. Vacuum instability and Black Hole Evaporation

    Michael Florian Wondrak · Heino Falcke · Walter D. van Suijlekom

    This talk presents a new avenue to black hole evaporation using a heat-kernel approach in the context of effective field theory analogous to deriving the Schwinger effect. Applying this method to an uncharged massless scalar field in a Schwarzschild spacetime,

    QG5报告Sala 4

  7. Vacuum selection in qft

    Daniele Colosi

    In this talk we show that the relevant physical information in the construction of a vacuum state is encoded in the selection of a Lagrangian subspace of the space of complexified solutions. In particular we show the existence of a one-to-one correspondence be

    QG5报告Sala 4

  8. Viability of loop quantum cosmology at the level of bispectrum

    Roshna K · V Sreenath

    Observations by Planck indicate that CMB anisotropies are consistent with predictions of nearly Gaussian primordial perturbations as the one generated in slow roll inflation. On the other hand, loop quantum cosmology (LQC) generates a non-Gaussian bispectrum.

    QG1报告Sala 8

  9. Vibrating ring around black hole

    Martin Kološ

    A thin circular structure vibrating in the central plane of a black hole will be investigated. This circular ring (string loop) can be considered a simplified model for thin magnetic flux tubes (in plasma physics), and connections to accreting fluid structures

    AC1报告Sala 2

  10. What is the true nature of PSR J0901-4046?

    Banibrata Mukhopadhyay · Nirupam Roy · A R Rao

    The radio pulsar PSR J0901-4046 exhibits very slow rotation with a spin period 76 s, which is unusually low for a neutron star. Typically the spin period of radio pulsars ranges 1.4 ms to 23.5 s, when they are divided into various sub-classes, e.g. transient,

    CO5报告Sala 4

  11. Why CGW is yet to be detected from isolated magnetized rotating neutron stars?

    Banibrata Mukhopadhyay · Mayusree Das

    There are evidences for neutron stars (NSs) with the rotational frequency of several 100th of Hz and moderate magnetic fields, though magnetars are slowly spinning. Hence, if their magnetic and rotating axes are misaligned (nonzero obliquity angle), hence they

    GW1报告Sala 7

  12. Wormhole restrictions from quantum energy inequalities

    Eleni-Alexandra Kontou

    It is known that all wormholes violate classical energy conditions, non-negativity constraints on contractions of the stress-energy tensor. Since these conditions are violated by quantum fields, it was believed that wormholes can be constructed in the context

    AT1报告Sala 8

  13. Wormholes geometries in f(R,T^2) gravity satisfying the energy conditions

    Nailya Ganiyeva · Francisco Lobo · João Luís Rosa

    In this work we analyze traversable wormhole spacetimes in the framework of a covariant generalization of Einstein’s General Relativity known as energy-momentum squared gravity. Here, we show that a wide variety of wormhole solutions for which the matter field

    AT1报告Sala 8

  14. X-ray approach to the magnetar-FRB connections using NICER

    Teruaki Enoto

    The NICER (Neutron star Interior Composition ExploreR) X-ray telescope on the International Space Station can provide a powerful approach to the magnetar and FRB connections using its large effective area and prompt follow-up observation of transients. Our NIC

    CO1报告ICRANet Seminar Room

  15. X-ray echoes and the structure of molecular clouds in the Galactic Center

    Giovanni Stel · Francesco Haardt · Gabriele Ponti · Mattia Sormani

    Molecular clouds in the Galactic Center reprocess radiation from past outbursts, generating a strong Fe Kα fluorescent line (6.4 keV). Reflecting the radiation that reaches them as mirrors, these clouds retain the historical activity of their illuminating sour

    HP2报告Sala 5

  16. X-ray polarimetry of GRB 221009A

    Alberto Manfreda

    We present the Imaging X-ray Polarimetry Explorer (IXPE) observation of the gamma-ray burst (GRB) 221009A, which reached Earth on October 9, 2022. Although IXPE was not originally designed for this purpose, the exceptional brightness of GRB 221009A allowed it

    XP1报告Sala 2

  17. X-ray polarization from magnetar sources

    Roberto Taverna

    The launch of the IXPE telescope in late 2021 finally made polarization measurements in the 2-8 keV band a reality, more than 40 years after the pioneering observations of the OSO-8 satellite. In the first two years of operations, IXPE targeted more than 60 so

    CO1报告Sala 9

  18. qUFOs as the key observational feature of SMRIs

    Petra Suková · Francesco Tombesi · Vladimír Karas · Dheeraj Pasham · Michal Zajaček

    Recently, a previously quiescent nearby galactic nucleus, ASASSN-20qc, went to an outburst during which it has shown quasioperiodic ultra-fast outflows (qUFOs) with changing column density every cca 8 days. Different physical mechanisms have been proposed to e

    MA3报告Sala 3

  19. quantum mechanics relativity and gravity

    Giovanni Amelino-Camelia

    I observe that some of the key challenges faced by quantum-gravity research, and particularly by quantum-gravity phenomenology, can be traced back to grey area of our understanding of the interface between quantum mechanics and special relativity

    QG4报告ICRANet Seminar Room