نتایج جستجو برای: central square hole

تعداد نتایج: 650702  

2008
Jiliang Jing

With Carlip’s boundary conditions, a standard Virasoro subalgebra with corresponding central charge for stationary dilaton black hole obtained in the low-energy effective field theory describing string is constructed at a Killing horizon. The statistical entropy of stationary dilaton black hole yielded by standard Cardy formula agree with its Bekenstein-Hawking entropy only if we take period T ...

پایان نامه :دانشگاه آزاد اسلامی - دانشگاه آزاد اسلامی واحد شاهرود - دانشکده مهندسی شیمی 1389

on this project we try to calculated power of hydrogen on dycarbonil compound in different ways ; the first way is shoster way , for sain power of hydrogen notice the different power between central conforms on it and main conform that’s didn’t have hydrogen joint . or in other way different of energy between open and close form. second way, is average way? this is for way that studied conf...

Journal: :Physical review letters 2012
N A Sinitsyn Yan Li S A Crooker A Saxena D L Smith

Strain-induced gradients of local electric fields in semiconductor quantum dots can couple to the quadrupole moments of nuclear spins. We develop a theory describing the influence of this quadrupolar coupling on the spin correlators of electron and hole "central" spins localized in such dots. We show that when the quadrupolar coupling strength is comparable to or larger than the hyperfine coupl...

2008
Paolo Aniello

We introduce the notion of square integrable group representation modulo a relatively central subgroup and, establishing a link with square integrable projective representations, we prove a generalization of a classical theorem of Duflo and Moore. As an example, we apply the results obtained to the Weyl-Heisenberg group.

2003
Eliot Quataert

Winds from massive stars supply ≈ 10 −3 M ⊙ yr −1 of gas to the central parsec of the Galactic Center. Spherically symmetric hydrodynamic calculations show that ≈ 1% of this gas, or ≈ 10 −5 M ⊙ yr −1 , flows in towards the central massive black hole Sgr A*; the remaining gas, ≈ 10 −3 M ⊙ yr −1 , is thermally driven out of the central star cluster in a wind. This dynamical model accounts for the...

2000
Andreas Burkert

The observed relation between central black hole mass and spheroid velocity dispersion is interpreted in terms of a self-regulation model that incorporates a viscous Keplerian accretion disk to feed the black hole, embedded in a massive, self-gravitating star forming disk that eventually populates the spheroid. The model leads to a constant ratio between black hole mass and spheroid mass which ...

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