Cosmology of rolling tachyon

نویسنده

  • HANG BAE KIM
چکیده

Recent analysis of string theory 1,2,3 suggests that classical dynamics of tachyon on an unstable D-brane is described by a scalar Born-Infeld type action with a runaway potential 4. Characteristic of such tachyon effective theory is absence of perturbative tachyonic modes around the potential minimum and existence of spatially homogeneous rolling tachyon configuration 5. In the background of the rolling tachyon, Abelian gauge field on the D-brane cannot support perturbative spectrum at late-time 6,7,9. In this review, we summarize firstly bosonic effective action both in the bulk and on the D-brane, together with shapes of the tachyon potential. In section 3, we introduce Carrolian limit, and then discuss nonexistence of perturbative spectra of the tachyon and the Abelian gauge field in the potential minimum, of which dynamics are governed by nonlocal D-brane action. For the tachyon, there exists the classical rolling tachyon solution connecting smoothly unstable maximum

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

More on Tachyon Cosmology in De Sitter Gravity

We aim to study rolling tachyon cosmological solutions in de Sitter gravity. The solutions are taken to be flat FRW type and these are not time-reversal symmetric. We find that cosmological constant of our universe has to be fine-tuned at the level of the action itself, as in KKLT string compactification. The rolling tachyon can give rise to required inflation with suitable choice of the initia...

متن کامل

ar X iv : h ep - t h / 02 05 00 3 v 5 2 7 Ju n 20 02 UPR - 992 - T Cosmological Constraints on Tachyon Matter

We examine whether tachyon matter is a viable candidate for the cosmological dark matter. First, we demonstrate that in order for the density of tachyon matter to have an acceptable value today, the magnitude of the tachyon potential energy at the onset of rolling must be finely tuned. For a tachyon potential V (T ) ∼ M4 P l exp(−T/τ), the tachyon must start rolling at T ≃ 60τ in order for the ...

متن کامل

Cosmological Constraints on Tachyon Matter

We examine whether tachyon matter is a viable candidate for the cosmological dark matter. First, we demonstrate that in order for the density of tachyon matter to have an acceptable value today, the magnitude of the tachyon potential energy at the onset of rolling must be finely tuned. For a tachyon potential V (T ) ∼ M4 P l exp(−T/τ), the tachyon must start rolling at T ≃ 60τ in order for the ...

متن کامل

Rolling Closed String Tachyons and the Big Crunch

We study the low-energy effective field equations that couple gravity, the dilaton, and the bulk closed string tachyon of bosonic closed string theory. We establish that whenever the tachyon induces the rolling process, the string metric remains fixed while the dilaton rolls to strong coupling. For negative definite potentials we show that this results in an Einstein metric that crunches the un...

متن کامل

Quantum Cosmology and Tachyons

We discuss the relevance of the classical and quantum rolling tachyons inflation in the frame of the standard, p-adic and adelic minisuperspace quantum cosmology. The field theory of tachyon matter proposed by Sen in a zero-dimensional version suggested by Kar leads to a model of a particle moving in a constant external field with quadratic damping. We calculate the exact quantum propagator of ...

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 2008