Higgs field governs the interior spacetime of black holes

The Higgs field is conventionally treated as a small local perturbation atop a large, constant vacuum value that uniformly permeates the Universe. I propose instead that in regions of extreme gravitational intensity—such as near gravitational singularities—the Higgs field behaves in a profoundly nonperturbative manner. In such environments, spacetime and the Higgs field engage in a dynamic interplay that extends spacetime beyond the singularity, achieving geodesic completeness. The continuation beyond the singularity is dominated by antigravity effects, reshaping the causal structure of spacetime and enabling novel flows of matter and information, including traversal through singularities. In its standard form, the combined framework of the Standard Model (SM) and general relativity (GR), as well as most of its extensions, fails to capture these phenomena due to its geodesic incompleteness. By contrast, a refined, locally conformal-symmetric formulation—denoted i( <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"> <a:mrow> <a:mi>SM</a:mi> <a:mo>+</a:mo> <a:mi>GR</a:mi> </a:mrow> </a:math> )—naturally incorporates these effects. GR is not an optional component of i( <c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"> <c:mrow> <c:mi>SM</c:mi> <c:mo>+</c:mo> <c:mi>GR</c:mi> </c:mrow> </c:math> ) but an essential ingredient. This framework preserves the empirical success of <e:math xmlns:e="http://www.w3.org/1998/Math/MathML" display="inline"> <e:mrow> <e:mi>SM</e:mi> <e:mo>+</e:mo> <e:mi>GR</e:mi> </e:mrow> </e:math> in the low-energy regime while predicting striking new phenomena in extreme gravitational settings, including within black holes (on both sides of the singularity) and in pre–big bang cosmology. At the classical field theory level, i( <g:math xmlns:g="http://www.w3.org/1998/Math/MathML" display="inline"> <g:mrow> <g:mi>SM</g:mi> <g:mo>+</g:mo> <g:mi>GR</g:mi> </g:mrow> </g:math> ) offers fresh perspectives on the black hole information puzzle and provides a platform for locally scale-invariant generalizations, such as geodesically complete quantum field theory, string theory, and unified models of fundamental interactions. This paper presents the detailed derivations and explanations that underlie a condensed letter version recently published in Itzhak Bars, Higgs field as architect of a geodesically complete universe and agent for new physics in interiors of black holes, .

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Journal
Physical review. D/Physical review. D.
Published
2025-09-30
DOI
https://doi.org/10.1103/n3hw-831m
Primary Topic
Black Holes and Theoretical Physics
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article
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article

Higgs field governs the interior spacetime of black holes

Itzhak Bars
Physical review. D/Physical review. D.
Black Holes and Theoretical Physics
article

Higgs field governs the interior spacetime of black holes

Itzhak Bars
article en

Abstract

The Higgs field is conventionally treated as a small local perturbation atop a large, constant vacuum value that uniformly permeates the Universe. I propose instead that in regions of extreme gravitational intensity—such as near gravitational singularities—the Higgs field behaves in a profoundly nonperturbative manner. In such environments, spacetime and the Higgs field engage in a dynamic interplay that extends spacetime beyond the singularity, achieving geodesic completeness. The continuation beyond the singularity is dominated by antigravity effects, reshaping the causal structure of spacetime and enabling novel flows of matter and information, including traversal through singularities. In its standard form, the combined framework of the Standard Model (SM) and general relativity (GR), as well as most of its extensions, fails to capture these phenomena due to its geodesic incompleteness. By contrast, a refined, locally conformal-symmetric formulation—denoted i( <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"> <a:mrow> <a:mi>SM</a:mi> <a:mo>+</a:mo> <a:mi>GR</a:mi> </a:mrow> </a:math> )—naturally incorporates these effects. GR is not an optional component of i( <c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"> <c:mrow> <c:mi>SM</c:mi> <c:mo>+</c:mo> <c:mi>GR</c:mi> </c:mrow> </c:math> ) but an essential ingredient. This framework preserves the empirical success of <e:math xmlns:e="http://www.w3.org/1998/Math/MathML" display="inline"> <e:mrow> <e:mi>SM</e:mi> <e:mo>+</e:mo> <e:mi>GR</e:mi> </e:mrow> </e:math> in the low-energy regime while predicting striking new phenomena in extreme gravitational settings, including within black holes (on both sides of the singularity) and in pre–big bang cosmology. At the classical field theory level, i( <g:math xmlns:g="http://www.w3.org/1998/Math/MathML" display="inline"> <g:mrow> <g:mi>SM</g:mi> <g:mo>+</g:mo> <g:mi>GR</g:mi> </g:mrow> </g:math> ) offers fresh perspectives on the black hole information puzzle and provides a platform for locally scale-invariant generalizations, such as geodesically complete quantum field theory, string theory, and unified models of fundamental interactions. This paper presents the detailed derivations and explanations that underlie a condensed letter version recently published in Itzhak Bars, Higgs field as architect of a geodesically complete universe and agent for new physics in interiors of black holes, .

Physical review. D/Physical review. D.Vol. 112(7)
University of Southern California (US), California Southern University (US)
Openalex Percentile: Top 86%
Black Holes and Theoretical Physics
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