Two observers calculate the trace anomaly

نویسندگان
چکیده

برای دانلود باید عضویت طلایی داشته باشید

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

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Two observers calculate the trace anomaly

We adapt a calculation due to Massacand and Schmid to the coordinate independent definition of time and vacuum given by Capri and Roy in order to compute the trace anomaly for a massless scalar field in a curved spacetime in 1+1 dimensions. The computation which requires only a simple regulator and normal ordering yields the well-known result R 24π in a straightforward manner. 03.70 Typeset usi...

متن کامل

Classical Trace Anomaly

We seek the analogy of the mathematical form of the alternative form of Einstein's field equations for Lovelock's field equations. We find that the price for this analogy is to accept the existence of the trace anomaly of the energy-momentum tensor even in classical treatments.

متن کامل

Higgs decay into two photons , dispersion relations and trace anomaly

We examine the contribution ofW boson loops to the amplitude of the process H −→ γγ within the dispersion relation approach, taking up an issue raised in this context recently. We show that the non-vanishing limit of the relevant formfactor for mW → 0 is due to a finite subtraction induced by the value of the corresponding trace anomaly. The argument can be turned around and one thus arrives at...

متن کامل

Trace Anomaly of Dilaton Coupled Scalars in Two Dimensions

Conformal scalar fields coupled to the dilaton appear naturally in two-dimensional models of black hole evaporation. We show that their trace anomaly is (1/24π)[R− 6(∇φ)2 − 22φ]. It follows that the RST counterterm appears naturally in the one-loop effective action. [email protected] [email protected]

متن کامل

Trace anomaly driven inflation

This paper investigates Starobinsky's model of inflation driven by the trace anomaly of conformally coupled matter fields. This model does not suffer from the problem of contrived initial conditions that occurs in most models of inflation driven by a scalar field. The universe can be nucleated semi-classically by a cosmological instanton that is much larger than the Planck scale provided there ...

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

ژورنال

عنوان ژورنال: Classical and Quantum Gravity

سال: 1996

ISSN: 0264-9381,1361-6382

DOI: 10.1088/0264-9381/13/2/006