The spectral dimension in 2D CDT gravity coupled to scalar fields

نویسندگان

  • J. Ambjørn
  • A. Görlich
  • J. Jurkiewicz
چکیده

Causal Dynamical Triangulations (CDT) provide a non-perturbative formulation of Quantum Gravity assuming the existence of a global time foliation. In our earlier study we analyzed the effect of including d copies of a massless scalar field in the two-dimensional CDT model with imaginary time. For d > 1 we observed the formation of a “blob”, somewhat similar to that observed in four-dimensional CDT without matter. In the two-dimensional case the “blob” has a Hausdorff dimension DH = 3. In this paper we study the spectral dimension DS of the two-dimensional CDT-universe, both for d = 0 (pure gravity) and d = 4. We show that in both cases the spectral dimension is consistent with DS = 2. 1 ar X iv :1 41 2. 34 34 v1 [ gr -q c] 1 0 D ec 2 01 4

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

The Spectral Dimension of 2D Quantum Gravity

We show that the spectral dimension ds of two-dimensional quantum gravity coupled to Gaussian fields is two for all values of the central charge c ≤ 1. The same arguments provide a simple proof of the known result ds = 4/3 for branched polymers. email [email protected] email [email protected] email [email protected] email [email protected] email [email protected] 1

متن کامل

The microscopic structure of 2D CDT coupled to matter

Article history: Received 29 March 2015 Received in revised form 12 May 2015 Accepted 12 May 2015 Available online 15 May 2015 Editor: J. Hisano We show that for 1 + 1 dimensional Causal Dynamical Triangulations (CDT) coupled to 4 massive scalar fields one can construct an effective transfer matrix if the masses squared are larger than or equal to 0.05. The properties of this transfer matrix ca...

متن کامل

beta functions of a scalar theory coupled to gravity.

We study a scalar field theory coupled to gravity on a flat background, below Planck’s energy. Einstein’s theory is treated as an effective field theory. Within the context of Wilson’s renormalization group, we compute gravitational corrections to the beta functions and the anomalous dimension of the scalar field, taking into account threshold effects.

متن کامل

Extended Slow-Roll Conditions and Primordial Fluctuations: Multiple Scalar Fields and Generalized Gravity

As an extension of our previous study, we derive slow-roll conditions for multiple scalar fields which are non-minimally coupled with gravity and for generalized gravity theories of the form f(φ,R). We provide simple formulae of the spectral indices of scalar/tensor perturbations in terms of the slow-roll parameters. Extended Slow-Roll Conditions and Primordial Fluctuations: Multiple Scalar Fie...

متن کامل

Generalized 2d dilaton gravity with matter fields

We extend the classical integrability of the CGHS model of 2d gravity [1] to a larger class of models, allowing the gravitational part of the action to depend more generally on the dilaton field and, simultaneously, adding fermion– and U(1)–gauge–fields to the scalar matter. On the other hand we provide the complete solution of the most general dilaton–dependent 2d gravity action coupled to chi...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2017