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Gravity and Strings

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19.3 The masses <strong>and</strong> charges of the p-brane solutions 549<br />

5. In d dimensions, the mass M of any static, asymptotically flat metric describing<br />

a point-like object can be found from its asymptotic behavior at spatial infinity<br />

[706, 877]. In the string-theory context, the mass ME associated with the “Einstein<br />

metric” (i.e. with the “wrong” normalization factor g2 (16πG (d)<br />

N )−1 in the action) can<br />

be implicitly defined by<br />

gE tt ∼ 1 − 16πG(d) N ME<br />

g2 1<br />

(d − 2)ω(d−2) |xd−1| d−3 , xd−1 = (x 1 ,...,x d−1 ), (19.92)<br />

The mass M associated with the modified Einstein metric (i.e. with the “right” normalization<br />

factor (16πG (d)<br />

N )−1 )isdefined analogously by,<br />

˜gE tt ∼ 1 − 16πG(d)<br />

N M<br />

(d − 2)ω(d−2)<br />

1<br />

. (19.93)<br />

|xd−1|<br />

d−3<br />

If both the string metric <strong>and</strong> the “modified string metric” are asymptotically flat (as<br />

we have assumed) then the Einstein metric is not, <strong>and</strong> it is necessary to rescale the<br />

coordinates with factors of g 1 4 in order to be able to use Eq. (19.92). Taking this into<br />

account, we find that the relation (in any dimension) between ME <strong>and</strong> M is given by<br />

ME = g 1 4 M. (19.94)<br />

6. Under IIB S duality, it is the (unmodified) Einstein-frame metric that is invariant.<br />

Then ME is S-duality-invariant, which implies the following S-duality transformation<br />

rule for M, which was already given in Eq. (19.3):<br />

M ′ E = ME, ⇒ M ′ = g ′− 1 4<br />

B g 1 4<br />

B M = g 1 2<br />

B M. (19.95)<br />

We can apply these formulae to find the masses of any of the solutions we have studied.<br />

They should coincide with the masses of the corresponding states in string/M theory.<br />

Let us take, for example, the F1 solution given in Eq. (19.56), assuming that the string is<br />

compactified on a circle <strong>and</strong> y is a compact dimension so we can dimensionally reduce the<br />

above solution, <strong>and</strong> calculate the modified Einstein mass of the resulting point-like object<br />

that lives in d = 9byusing Eq. (19.93).<br />

First, we need the nine-dimensional dilaton (see Eq. (15.16)),<br />

e −2(φ−φ0)<br />

<br />

−2( ˆφ− ˆφ0)<br />

= e<br />

|ˆgyy|=H 1 2<br />

F1<br />

so, in this case, the relation between the nine-dimensional metrics is<br />

˜gEµν = H 1 7<br />

F1 gµν, ⇒˜gE tt = H − 6 7<br />

F1<br />

which, compared with Eq. (19.93), gives the right value,<br />

MF1w = 6hF1ω(7)<br />

16πG (9) =<br />

N<br />

12π R9hF1ω(7)<br />

on account of Eqs. (19.87), (19.26), <strong>and</strong> (19.57).<br />

16πG (10)<br />

N<br />

, (19.96)<br />

6hF1<br />

∼ 1 − , (19.97)<br />

7ρ6 = R9<br />

ℓ9 , (19.98)<br />

s

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