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The BSM-2023 Conference is organized by the Journal of “Letters in High Energy Physics” UK, like BSM-2021, and aims at discussing the latest developments in physics beyond the standard models of particle physics, cosmology, and gravitation. We hope that the conference will help to strengthen international collaborations among high-energy physicists and allow for fruitful discussions on the most recent theoretical, experimental and observational developments.
The program consists of plenary presentations by invited speakers and contributed talks selected from submitted abstracts. Contributions will be refereed by the Conveners, and accepted ones will be recommended for publication in Letters in High Energy Physics (LHEP) journal.
Deadline for Registration: September 15, 2023
Deadline for Fee Payment: October 1, 2023
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General review of various modified gravity is done. special attention is paid to F(R) and F(G) modified gravity. The realistic exponential model which unifies inflation with dark energy is discussed and compared with LCDM theory. It is shown how modified Gauss-Bonnet gravity may give realistic inflation while it is still compatible with recent GW event data. Stellar astrophysics in the presence of the extended gravity is briefly discussed. It is also demonstrated how F(R) gravity or any other theory maybe reconstructed from slow-roll inflationary indices.
We discuss a model of the universe where dark energy is replaced by
electrically-charged extremely-massive dark matter. The cosmological
constant has a value of the same order as the mean matter density,
consistent with observations, and is obtained classically without fine-tuning.
Wormholes have never been observed but proven to be valid solution to
field equations of general relativity. Patton and Wheeler postulated that
the vacuum state of the gravitational field features a Planch-scale state
virtual geometries known as quantum foam. In early universe, some of
these geometries include submicroscopic wormholes, and their existence
is governed by the uncertainty principle. It has been conjectured that
quantum fluctuations may allow wormholes to grow from submicroscopic
to microscopic scale. It is conceivable that Planck-scale wormholes may
become enlarged to macroscopic size during the inflationary phase of the
early universe, potentially creating a cosmic network. Theoritically, a
wormhole will collapse immediately to a singularity. However, it has
been postulated by Kip Thorn et al. that traversability of a wormhole
requires exotic matter to hold it open against gravitational collapse.
Matter is considered exotic with respect to the null energy condition if its
stress energy is negative. Quantum field theory permits negative energy
and fluxes, subject to certain restrictions imposed by the uncertainty
principle. In this paper, we discuss the various models proposed to
maintain the stability of the wormhole and examine how they align with
the broader framework of quantum gravity theory in the early universe.
Additionally, we will explore the effect of antimatter and the implications
of charge-parity-time reversal (CPT) violation in both flat and curved
spacetime on wormhole physics. We will consider the potential
repercussion of this verdict on the traversability of primordial wormholes.
Finally, traversable wormholes in Einstein-Dirac-Maxwell theory are
reviewed and discussed.