Ramond-Ramond field radiation from rotating ellipsoidal membranes

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Ramond-Ramond field radiation from rotating ellipsoidal membranes. / Harmark, Troels; Savvidy, Konstantin G.

In: Nuclear Physics B, Vol. 585, No. 3, 09.10.2000, p. 567-588.

Research output: Contribution to journal › Journal article › Research › peer-review

Harvard

Harmark, T & Savvidy, KG 2000, 'Ramond-Ramond field radiation from rotating ellipsoidal membranes', Nuclear Physics B, vol. 585, no. 3, pp. 567-588. https://doi.org/10.1016/S0550-3213(00)00333-3

APA

Harmark, T., & Savvidy, K. G. (2000). Ramond-Ramond field radiation from rotating ellipsoidal membranes. Nuclear Physics B, 585(3), 567-588. https://doi.org/10.1016/S0550-3213(00)00333-3

Vancouver

Harmark T, Savvidy KG. Ramond-Ramond field radiation from rotating ellipsoidal membranes. Nuclear Physics B. 2000 Oct 9;585(3):567-588. https://doi.org/10.1016/S0550-3213(00)00333-3

Author

Harmark, Troels ; Savvidy, Konstantin G. / Ramond-Ramond field radiation from rotating ellipsoidal membranes. In: Nuclear Physics B. 2000 ; Vol. 585, No. 3. pp. 567-588.

Bibtex

@article{8ca6ae71aba74ba99d6dcc712065a7ac,
title = "Ramond-Ramond field radiation from rotating ellipsoidal membranes",
abstract = "We find a new stable rotator solution in D0-brane matrix mechanics. The solution is interpreted as a D2/D0 brane bound state, constructed as a transversely rotating ellipsoidal membrane with N D0-branes pinned over it. From the membrane point of view the attractive force of tension is exactly cancelled by the repulsive centrifugal force. Dynamical properties of the system are investigated, in particular the emission of spherical waves in the different massless sectors of supergravity. We compute the RR 1-form quadrupole, the RR 3-form dipole and the gravitational quadrupole radiation. Also, we show that our non-singular classical solution is stable against small perturbations in the initial conditions. Furthermore, we comment on a possible fundamental particle interpretation of our system.",
author = "Troels Harmark and Savvidy, {Konstantin G.}",
year = "2000",
month = oct,
day = "9",
doi = "10.1016/S0550-3213(00)00333-3",
language = "English",
volume = "585",
pages = "567--588",
journal = "Nuclear Physics, Section B",
issn = "0550-3213",
publisher = "Elsevier BV * North-Holland",
number = "3",

}

RIS

TY - JOUR

T1 - Ramond-Ramond field radiation from rotating ellipsoidal membranes

AU - Harmark, Troels

AU - Savvidy, Konstantin G.

PY - 2000/10/9

Y1 - 2000/10/9

N2 - We find a new stable rotator solution in D0-brane matrix mechanics. The solution is interpreted as a D2/D0 brane bound state, constructed as a transversely rotating ellipsoidal membrane with N D0-branes pinned over it. From the membrane point of view the attractive force of tension is exactly cancelled by the repulsive centrifugal force. Dynamical properties of the system are investigated, in particular the emission of spherical waves in the different massless sectors of supergravity. We compute the RR 1-form quadrupole, the RR 3-form dipole and the gravitational quadrupole radiation. Also, we show that our non-singular classical solution is stable against small perturbations in the initial conditions. Furthermore, we comment on a possible fundamental particle interpretation of our system.

AB - We find a new stable rotator solution in D0-brane matrix mechanics. The solution is interpreted as a D2/D0 brane bound state, constructed as a transversely rotating ellipsoidal membrane with N D0-branes pinned over it. From the membrane point of view the attractive force of tension is exactly cancelled by the repulsive centrifugal force. Dynamical properties of the system are investigated, in particular the emission of spherical waves in the different massless sectors of supergravity. We compute the RR 1-form quadrupole, the RR 3-form dipole and the gravitational quadrupole radiation. Also, we show that our non-singular classical solution is stable against small perturbations in the initial conditions. Furthermore, we comment on a possible fundamental particle interpretation of our system.

U2 - 10.1016/S0550-3213(00)00333-3

DO - 10.1016/S0550-3213(00)00333-3

M3 - Journal article

AN - SCOPUS:0001010180

VL - 585

SP - 567

EP - 588

JO - Nuclear Physics, Section B

JF - Nuclear Physics, Section B

SN - 0550-3213

IS - 3

ER -

ID: 226069663