A toy model of quantum gravity with a quantized cosmological constant∗

نویسنده

  • Kazuo Fujikawa
چکیده

The path integral for the hydrogen atom, for example, is formulated as a onedimensional quantum gravity coupled to matter fields representing the electron coordinates. The (renormalized) cosmological constant, which corresponds to the energy eigenvalue, is thus quantized in this model. Possible implications of the quantized cosmological constant are briefly discussed. The problem of the cosmological constant in quantum gravity has a long history. For a review of this subject, see ref.[1] and papers cited therein. Recently, we pointed out that the path integral of the hydrogen atom, for example, in non-relativistic quantum mechanics is formulated as a one-dimensional quantum gravity coupled to matter fields representing the electron coordinates. The basic idea of this formulation is to use the Jacobi’s principle of least action for the evaluation of the Green’s function with a given energy[2]. In this formulation, the (renormalized) cosmological constant corresponds to the energy eigenvalue of the Schroedinger equation, and thus the cosmological constant is quantized. Since the notion of a quantized cosmological constant appears to be something novel, at least to my knowledge, we would like to present a brief description of the model. The ∗To be published in Progress of Theoretical Physics(Kyoto)

برای دانلود رایگان 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

Fat Euclidean Gravity with Small Cosmological Constant

The cosmological constant problem is usually considered an inevitable feature of any effective theory capturing well-tested gravitational and matter physics, without regard to the details of short-distance gravitational couplings. In this paper, a subtle effective description avoiding the problem is presented in a first quantized language, consistent with experiments and the Equivalence Princip...

متن کامل

The Classical Limit of Quantum Gravity Isn ’ t *

Two-dimensional quantum gravity coupled to conformally invariant matter with central charge c > 25 has been proposed as a toy model for quantum gravity in higher dimensions. The associated Wheeler-Dewitt equation is non-linear and unstable to forming a condensate of baby universes. This will occur even in the classical c + 00 limit, and as a result, large scale cosmological solutions with a con...

متن کامل

The Cosmological Constant of One-Dimensional Matter Coupled Quantum Gravity is Quantized

Coupling any interacting quantum mechanical system to gravity in one dimension requires the cosmological constant to belong to the matter energy spectrum and thus to be quantized, even though the gravity sector is free of any quantum dynamics, while physical states are also confined to the subspace of matter quantum states whose energy coincides with the cosmological constant value. These gener...

متن کامل

The cosmological constant: a lesson from Bose–Einstein condensates

The cosmological constant is one of the most pressing problems in modern physics. In this Letter, we address the issue of its nature and computation using an analogue gravity standpoint as a toy model for an emergent gravity scenario. Even if it is well known that phonons in some condense matter systems propagate like a quantum field on a curved spacetime, only recently it has been shown that t...

متن کامل

Infrared Divergences in dS/CFT

dS/CFT gives a perturbatively gauge invariant definition of particle masses in de Sitter (dS) space. We show, in a toy model in which the graviton is replaced with a minimally coupled massless scalar field, that loop corrections to these masses are infrared (IR) divergent. We argue that this implies anomalous dependence of masses on the cosmological constant, in a true theory of quantum gravity...

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

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 1996