{"title":"Inequivalence between the Euclidean and Lorentzian Versions of the Type IIB Matrix Model from Lefschetz Thimble Calculations","authors":"Chien-Yu Chou, Jun Nishimura, Ashutosh Tripathi","doi":"10.1103/physrevlett.134.211601","DOIUrl":null,"url":null,"abstract":"The type IIB matrix model is conjectured to describe superstring theory nonperturbatively in terms of ten N</a:mi>×</a:mo>N</a:mi></a:math> bosonic traceless Hermitian matrices <c:math xmlns:c=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><c:msub><c:mi>A</c:mi><c:mi>μ</c:mi></c:msub></c:math> (<e:math xmlns:e=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><e:mi>μ</e:mi><e:mo>=</e:mo><e:mn>0</e:mn><e:mo>,</e:mo><e:mo>…</e:mo><e:mo>,</e:mo><e:mn>9</e:mn></e:math>), whose eigenvalues correspond to (<g:math xmlns:g=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><g:mrow><g:mn>9</g:mn><g:mo>+</g:mo><g:mn>1</g:mn></g:mrow></g:math>)-dimensional space-time. Quite often, this model has been investigated in its Euclidean version, which is well defined although the <i:math xmlns:i=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><i:mrow><i:mi>SO</i:mi></i:mrow><i:mo stretchy=\"false\">(</i:mo><i:mn>9</i:mn><i:mo>,</i:mo><i:mn>1</i:mn><i:mo stretchy=\"false\">)</i:mo></i:math> Lorentz symmetry of the original model is replaced by the <m:math xmlns:m=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><m:mrow><m:mrow><m:mi>SO</m:mi></m:mrow><m:mo stretchy=\"false\">(</m:mo><m:mn>10</m:mn><m:mo stretchy=\"false\">)</m:mo></m:mrow></m:math> rotational symmetry. Recently, a well-defined model respecting the Lorentz symmetry has been proposed by “gauge-fixing” the Lorentz symmetry nonperturbatively using the Faddeev-Popov procedure. Here we investigate the two models by Monte Carlo simulations overcoming the severe sign problem by the Lefschetz thimble method, in the case of matrix size <q:math xmlns:q=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><q:mi>N</q:mi><q:mo>=</q:mo><q:mn>2</q:mn></q:math> omitting fermionic contributions. We add a quadratic term <s:math xmlns:s=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><s:mrow><s:mi>γ</s:mi><s:mi>tr</s:mi><s:mo stretchy=\"false\">(</s:mo><s:msub><s:mrow><s:mi>A</s:mi></s:mrow><s:mrow><s:mi>μ</s:mi></s:mrow></s:msub><s:msup><s:mrow><s:mi>A</s:mi></s:mrow><s:mrow><s:mi>μ</s:mi></s:mrow></s:msup><s:mo stretchy=\"false\">)</s:mo></s:mrow></s:math> in the action and calculate the expectation values of rotationally symmetric (or Lorentz symmetric) observables as a function of the coefficient <w:math xmlns:w=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><w:mi>γ</w:mi></w:math>. Our results exhibit striking differences between the two models around <y:math xmlns:y=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><y:mi>γ</y:mi><y:mo>=</y:mo><y:mn>0</y:mn></y:math> and in the γ</ab:mi>></ab:mo>0</ab:mn></ab:math> region associated with the appearance of different saddle points, clearly demonstrating their inequivalence against naive expectations from quantum field theory. <jats:supplementary-material> <jats:copyright-statement>Published by the American Physical Society</jats:copyright-statement> <jats:copyright-year>2025</jats:copyright-year> </jats:permissions> </jats:supplementary-material>","PeriodicalId":20069,"journal":{"name":"Physical review letters","volume":"25 1","pages":""},"PeriodicalIF":8.1000,"publicationDate":"2025-05-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physical review letters","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1103/physrevlett.134.211601","RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"PHYSICS, MULTIDISCIPLINARY","Score":null,"Total":0}
引用次数: 0
Abstract
The type IIB matrix model is conjectured to describe superstring theory nonperturbatively in terms of ten N×N bosonic traceless Hermitian matrices Aμ (μ=0,…,9), whose eigenvalues correspond to (9+1)-dimensional space-time. Quite often, this model has been investigated in its Euclidean version, which is well defined although the SO(9,1) Lorentz symmetry of the original model is replaced by the SO(10) rotational symmetry. Recently, a well-defined model respecting the Lorentz symmetry has been proposed by “gauge-fixing” the Lorentz symmetry nonperturbatively using the Faddeev-Popov procedure. Here we investigate the two models by Monte Carlo simulations overcoming the severe sign problem by the Lefschetz thimble method, in the case of matrix size N=2 omitting fermionic contributions. We add a quadratic term γtr(AμAμ) in the action and calculate the expectation values of rotationally symmetric (or Lorentz symmetric) observables as a function of the coefficient γ. Our results exhibit striking differences between the two models around γ=0 and in the γ>0 region associated with the appearance of different saddle points, clearly demonstrating their inequivalence against naive expectations from quantum field theory. Published by the American Physical Society2025
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