DOES ENTROPIC GRAVITY BOUND THE MASSES OF THE PHOTON AND GRAVITON?

被引:22
作者
Mureika, J. R. [1 ]
Mann, R. B. [2 ,3 ]
机构
[1] Loyola Marymount Univ, Dept Phys, Los Angeles, CA 90045 USA
[2] Univ Waterloo, Perimeter Inst Theoret Phys, Waterloo, ON N2L 3G1, Canada
[3] Univ Waterloo, Dept Phys & Astron, Waterloo, ON N2L 3G1, Canada
基金
加拿大自然科学与工程研究理事会;
关键词
Emergent gravity; holographic principle; massive photon/graviton; BLACK-HOLES; ENERGY;
D O I
10.1142/S0217732311034840
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
If the information transfer between test particle and holographic screen in entropic gravity respects both the uncertainty principle and causality, a lower limit on the numb er of bits in the universe relative to its mass may be derived. Furthermore, these limits indicate particles that putatively travel at the speed of light - the photon and/or graviton-have a nonzero mass m >= 10(-68) kg. This result is found to be in excellent agreement with current experimental mass bounds on the graviton and photon, suggesting that entropic gravity may be the result of a (recent) softly-broken local symmetry. Stronger bounds emerge from consideration of ultra dense matter such as neutron stars, yielding limits of m >= 10(-48)-10(-50) kg, barely within the experimental photon range and outside that of the graviton. We find that for black holes these criteria cannot be satisfied, and suggest some possible implications of this result.
引用
收藏
页码:171 / 181
页数:11
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