Ultraviolet-Complete Local Field Theory of Persistent Symmetry Breaking in 2+1 Dimensions

IF 9 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Physical review letters Pub Date : 2025-01-28 DOI:10.1103/physrevlett.134.041602
Bilal Hawashin, Junchen Rong, Michael M. Scherer
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Abstract

Spontaneous symmetry breaking can persist at all temperatures in certain biconical O(N)×Z2 vector models when the underlying field theories are ultraviolet complete. So far, the existence of such theories has been established in fractional dimensions for local but nonunitary models or in 2+1 dimensions but for nonlocal models. Here, we study local models at zero and finite temperature directly in 2+1 dimensions employing functional methods. At zero temperature, we establish that our approach describes the quantum critical behavior with good accuracy for all N2. We then exhibit the mechanism of discrete symmetry breaking from O(N)×Z2O(N) for increasing temperature near the biconical critical point when N is finite but large. We calculate the corresponding finite-temperature phase diagram and further show that the Hohenberg-Mermin-Wagner theorem is fully respected within this approach, i.e., symmetry breaking only occurs in the Z2 sector. Finally, we determine the critical N above which this phenomenon can be observed to be Nc15. Published by the American Physical Society 2025
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2+1维持续对称破缺的紫外完全局部场论
当基础场论是紫外线完备时,在某些双二次O(N)×Z2矢量模型中,自发对称性破缺可以在所有温度下持续存在。到目前为止,这些理论的存在性已经在分数维局部但非酉模型或2+1维非局部模型中得到了证实。本文采用泛函方法直接在2+1维空间研究了零温度和有限温度下的局部模型。在零温度下,我们建立了我们的方法可以很好地描述所有N≥2的量子临界行为。然后,我们展示了从O(N)×Z2→O(N)的离散对称破缺机制,当N有限但很大时,在双锥临界点附近温度升高。我们计算了相应的有限温度相图,并进一步证明了在这种方法中完全遵守Hohenberg-Mermin-Wagner定理,即对称破缺只发生在Z2扇区。最后,我们确定了该现象的临界N为Nc≈15。2025年由美国物理学会出版
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来源期刊
Physical review letters
Physical review letters 物理-物理:综合
CiteScore
16.50
自引率
7.00%
发文量
2673
审稿时长
2.2 months
期刊介绍: Physical review letters(PRL)covers the full range of applied, fundamental, and interdisciplinary physics research topics: General physics, including statistical and quantum mechanics and quantum information Gravitation, astrophysics, and cosmology Elementary particles and fields Nuclear physics Atomic, molecular, and optical physics Nonlinear dynamics, fluid dynamics, and classical optics Plasma and beam physics Condensed matter and materials physics Polymers, soft matter, biological, climate and interdisciplinary physics, including networks
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