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Dilatonic black holes in higher curvature string gravity. II. Linear stability

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Figure

Figure 2: The graph depicts the coefficients B/A and B/A, for a typicalmember of the family of the black hole solutions of Fig.1 corresponding toφh = −1, rh = 1
Figure 3: This diagram depicts the coefficients E/A and E/A for a typicalmember of the family of the black hole solutions depicted in Fig
Figure 4: The graph depicts rrfor a fixed value ofh versus the ADM Mass 2M of the black hole, φh = −1
Figure 5:The magnification around the critical point, depicted in the abovefigure, shows clearly the abrupt (almost vertical) slope with which this pointis approached

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