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SUMMARY:Black Hole Singularity with Quantum Geometric Approach
DTSTART;VALUE=DATE-TIME:20241023T140000Z
DTEND;VALUE=DATE-TIME:20241023T141500Z
DTSTAMP;VALUE=DATE-TIME:20260307T203739Z
UID:indico-contribution-4086@cern.ch
DESCRIPTION:Speakers: Abdel Nasser Tawfik (Future Univrsity of Egypt)\nThe
  emergence of relativistic quantum gravitational effects is well anticipat
 ed when the Planck density ($m_p/\\ell_p^3$\, where $m_p$ is the Planck ma
 ss and $\\ell_p$ is the Planck length)\, regardless of whether the predict
 ion of an infinite-density singularity is viewed as a flaw in general rela
 tivity. Over the past century\, the orthogonality between quantum mechanic
 s and general relativity has been a persistent issue\, prompting the dedic
 ated efforts of brilliant scholars. Our focus is on a quantum geometric ap
 proach that expands the four-dimensional Riemann geometry (spacetime) to i
 ncorporate quantum-mechanical principles. This approach enables a comprehe
 nsive exploration of the fundamental nature of the Universe\, offering a m
 ore profound understanding of the underlying relativity and quantum princi
 ples governing its structure and evolution. The quantum geometric approach
  facilitates the derivation of the fundamental tensor\, upon which quantum
 -mechanically induced revisions are imposed. This\, in turn\, allows for t
 he construction of the general theory of relativity and the verification o
 f various black hole metrics\, while also enabling the examination of init
 ial and space singularities through timelike geodesic congruence.\n\nhttps
 ://indico.particle.mephi.ru/event/436/contributions/4086/
LOCATION: Moskvorechye 1
URL:https://indico.particle.mephi.ru/event/436/contributions/4086/
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