Gravity Induced Anomalies Smearing in Standard Model so that Protons May Never Decay, Except in Black Holes

viXra Pub Date : 2020-06-01 DOI:10.31219/osf.io/w4pfm
Stephane H Maes
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引用次数: 29

Abstract

Gravity is not modeled in the Standard Model. The Proton decay, predicted by many GUTs, TOEs, supersymmetry, supergravity theories and superstrings, is forbidden in the Standard Model because the proton is the lightest baryon and the conservation of the lepton and baryon numbers would be violated. In New Physics beyond the Standard Model, such violations could be tolerated because the baryon and lepton number symmetries have chirality anomalies. We discuss that in a multi-fold universe, where gravity emerges from entanglement effects, or in a universe where gravity is strong enough to cause chirality flips of fermions, these anomalies are smeared so that the baryon and lepton symmetries could be no more anomalous, and conservation of the baryon and lepton numbers could be seen as stricter. As a result, proton decay could remain forbidden, except when gravity is extreme. It has significant consequences for theories predicting proton decay but matches the total lack of any proton decay observation so far.
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引力引起的标准模型中的异常涂抹使得质子可能永远不会衰变,除非在黑洞中
标准模型中没有描述重力。许多大统一理论、超对称理论、超引力理论和超弦理论都预言了质子衰变,但在标准模型中是被禁止的,因为质子是最轻的重子,轻子和重子数量的守恒将被打破。在超越标准模型的新物理学中,这种违反是可以容忍的,因为重子和轻子数对称性具有手性异常。我们讨论了在多重宇宙中,引力从纠缠效应中产生,或者在引力强到足以引起费米子手性翻转的宇宙中,这些异常被抹去,以便重子和轻子对称性不再异常,重子和轻子数量的守恒可以被视为更严格。因此,质子衰变可能一直被禁止,除非重力非常大。它对预测质子衰变的理论有着重要的影响,但与迄今为止任何质子衰变观测的完全缺乏相匹配。
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