ZZ-branes from a spacetime perspective

Michele Cirafici

doi:10.1002/prop.200510280

ZZ-branes from a spacetime perspective

Michele Cirafici

Research output: Contribution to journal › Article › peer-review

Abstract

We review the analysis of the tachyon and RR scalar spacetime field configurations sourced by the (m, n) ZZ D-branes in type 0 theories. We focus on three approaches: the mini-superspace approximation, a motivated ansatz to go beyond the semi-classical approximation and finally by using the FZZT branes as probes. In all the three methods we find that the tension of the (m, n) ZZ brane is m n times the tension of the (1,1) ZZ brane. The RR charge of these branes is non-zero only for the case of both m and n odd, in which case it is identical to the charge of the (1,1) brane. © 2006 WILEY-VCH Verlag GmbH & Co. KGaA.

Original language	English
Pages (from-to)	343-350
Number of pages	8
Journal	Fortschritte der Physik
Volume	54
Issue number	5-6
DOIs	https://doi.org/10.1002/prop.200510280
Publication status	Published - May 2006

Keywords

D-branes
Non-critical strings

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10.1002/prop.200510280

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title = "ZZ-branes from a spacetime perspective",

abstract = "We review the analysis of the tachyon and RR scalar spacetime field configurations sourced by the (m, n) ZZ D-branes in type 0 theories. We focus on three approaches: the mini-superspace approximation, a motivated ansatz to go beyond the semi-classical approximation and finally by using the FZZT branes as probes. In all the three methods we find that the tension of the (m, n) ZZ brane is m n times the tension of the (1,1) ZZ brane. The RR charge of these branes is non-zero only for the case of both m and n odd, in which case it is identical to the charge of the (1,1) brane. {\textcopyright} 2006 WILEY-VCH Verlag GmbH \& Co. KGaA.",

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AU - Cirafici, Michele

PY - 2006/5

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N2 - We review the analysis of the tachyon and RR scalar spacetime field configurations sourced by the (m, n) ZZ D-branes in type 0 theories. We focus on three approaches: the mini-superspace approximation, a motivated ansatz to go beyond the semi-classical approximation and finally by using the FZZT branes as probes. In all the three methods we find that the tension of the (m, n) ZZ brane is m n times the tension of the (1,1) ZZ brane. The RR charge of these branes is non-zero only for the case of both m and n odd, in which case it is identical to the charge of the (1,1) brane. © 2006 WILEY-VCH Verlag GmbH & Co. KGaA.

AB - We review the analysis of the tachyon and RR scalar spacetime field configurations sourced by the (m, n) ZZ D-branes in type 0 theories. We focus on three approaches: the mini-superspace approximation, a motivated ansatz to go beyond the semi-classical approximation and finally by using the FZZT branes as probes. In all the three methods we find that the tension of the (m, n) ZZ brane is m n times the tension of the (1,1) ZZ brane. The RR charge of these branes is non-zero only for the case of both m and n odd, in which case it is identical to the charge of the (1,1) brane. © 2006 WILEY-VCH Verlag GmbH & Co. KGaA.

KW - D-branes

KW - Non-critical strings

UR - https://www.scopus.com/pages/publications/33646715554

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DO - 10.1002/prop.200510280

M3 - Article

SN - 0015-8208

VL - 54

SP - 343

EP - 350

JO - Fortschritte der Physik

JF - Fortschritte der Physik

IS - 5-6

ER -

ZZ-branes from a spacetime perspective

Abstract

Keywords

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