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Fig. 2 above shows that the constraints provided by gravity are surprisingly weak, leaving a wide open window for new interactions at large scales. This observation, made already in [47], not only triggered new interest in experimental tests of Newton’s law on small scales, as pointed out already, but also in phenomenological analyses of possible bounds on the string scale from collider processes [64, 66]. In the context of phenomenological models a wider range of possible interaction strengths is of interest than indicated in Fig. 2. Data constraining new interactions on shorter distance scales are shown in Fig. 3 [3], which is adapted from [55]. interactions on shorter distance scales are shown in Fig. 3 [3], which is adapted from [55]. Figure 3: Constraints on ISL-violating interactions, summarized from data in with Inm < A < lym.

Figure 2 above shows that the constraints provided by gravity are surprisingly weak, leaving a wide open window for new interactions at large scales. This observation, made already in [47], not only triggered new interest in experimental tests of Newton’s law on small scales, as pointed out already, but also in phenomenological analyses of possible bounds on the string scale from collider processes [64, 66]. In the context of phenomenological models a wider range of possible interaction strengths is of interest than indicated in Fig. 2. Data constraining new interactions on shorter distance scales are shown in Fig. 3 [3], which is adapted from [55]. interactions on shorter distance scales are shown in Fig. 3 [3], which is adapted from [55]. Figure 3: Constraints on ISL-violating interactions, summarized from data in with Inm < A < lym.

Related Figures (3)

Figure 1: An illustration of the universal moduli space that is expected to link all known string theories. as limits of a fundamental one is illustrated in Fig. 1 [95].
Figure 1: An illustration of the universal moduli space that is expected to link all known string theories. as limits of a fundamental one is illustrated in Fig. 1 [95].
for extra dimensions is given in Fig. 2 [80]. Figure 2: Constraints on ISL-violating Yukawa interactions with lum < A < lcm. E6ot- wash 2004 refers to the results in [72], E6t-wash2006 summarizes work done in [80], while the Stanford, Colorado and Irvine results are from [33, 87, 70, 108].
for extra dimensions is given in Fig. 2 [80]. Figure 2: Constraints on ISL-violating Yukawa interactions with lum < A < lcm. E6ot- wash 2004 refers to the results in [72], E6t-wash2006 summarizes work done in [80], while the Stanford, Colorado and Irvine results are from [33, 87, 70, 108].
Figure 4: Constraints on ISL-violating interactions, summarized from data in with Imm < \ < 10!°m.
Figure 4: Constraints on ISL-violating interactions, summarized from data in with Imm < \ < 10!°m.
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PhysicsTheoretical PhysicsString TheoryHigh Energy PhysicsString theory (Physics)String PhenomenologyCalabi-Yau
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