<p>We consider general <i>k</i> = −1 FLRW covariant quantum spacetimes <InlineEquation ID="IEq1"> <EquationSource Format="MATHML"><math display="inline"> <msup> <mi mathvariant="script">M</mi> <mrow> <mn>3</mn> <mo>,</mo> <mn>1</mn> </mrow> </msup> <mo>×</mo> <mi mathvariant="script">K</mi> </math></EquationSource> <EquationSource Format="TEX">\( {\mathcal{M}}^{3,1}\times \mathcal{K} \)</EquationSource> </InlineEquation> with fuzzy extra dimensions <InlineEquation ID="IEq2"> <EquationSource Format="MATHML"><math display="inline"> <mi mathvariant="script">K</mi> </math></EquationSource> <EquationSource Format="TEX">\( \mathcal{K} \)</EquationSource> </InlineEquation> as classical solutions of the IKKT matrix model. The coupled equations of motion are recast in terms of conservation laws, which allow to determine the evolution of spacetime in a transparent way. We show that <InlineEquation ID="IEq3"> <EquationSource Format="MATHML"><math display="inline"> <mi mathvariant="script">K</mi> </math></EquationSource> <EquationSource Format="TEX">\( \mathcal{K} \)</EquationSource> </InlineEquation> is stabilized as a classical solution in the presence of a large <i>R</i> charge, corresponding to internal angular momentum. This provides a mechanism to maintain a large hierarchy between UV and IR scales. We also argue that the evolution of spacetime is determined by a balance between classical and quantum effects, leading to a cosmic scale factor <i>a</i>(<i>t</i>) ~ <i>t</i> and constant dilaton at late times. On such a background, the undeformed IKKT model leads to a higher-spin gauge theory including gravity.</p>

错误:搜索内容不能为空,请输入英文关键词
错误:关键词超出字数限制,请精简
高级检索

Dynamical covariant quantum spacetime with fuzzy extra dimensions in the IKKT model

  • Alessandro Manta,
  • Harold C. Steinacker

摘要

We consider general k = −1 FLRW covariant quantum spacetimes M 3 , 1 × K \( {\mathcal{M}}^{3,1}\times \mathcal{K} \) with fuzzy extra dimensions K \( \mathcal{K} \) as classical solutions of the IKKT matrix model. The coupled equations of motion are recast in terms of conservation laws, which allow to determine the evolution of spacetime in a transparent way. We show that K \( \mathcal{K} \) is stabilized as a classical solution in the presence of a large R charge, corresponding to internal angular momentum. This provides a mechanism to maintain a large hierarchy between UV and IR scales. We also argue that the evolution of spacetime is determined by a balance between classical and quantum effects, leading to a cosmic scale factor a(t) ~ t and constant dilaton at late times. On such a background, the undeformed IKKT model leads to a higher-spin gauge theory including gravity.