TY - GEN
T1 - How changing physical constants and violation of local position invariance may occur?
AU - Flambaum, V. V.
AU - Shuryak, E. V.
PY - 2008
Y1 - 2008
N2 - Light scalar fields very naturally appear in modern cosmological models, affecting such parameters of Standard Model as electromagnetic fine structure constant α, dimensionless ratios of electron or quark mass to the QCD scale, me,q/ΛQCD. Cosmological variations of these scalar fields should occur because of drastic changes of matter composition in Universe: the latest such event is rather recent (redshift z∼0.5), from matter to dark energy domination. In a two-brane model (we use as a pedagogical example) these modifications are due to changing distance to "the second brane", a massive companion of "our brane". Back from extra dimensions, massive bodies (stars or galaxies) can also affect physical constants. They have large scalar charge Qd proportional to number of particles which produces a Coulomb-like scalar field =Qd/r. This leads to a variation of the fundamental constants proportional to the gravitational potential, e.g. δα/α=kαδ (GM/rc2). We compare different manifestations of this effect, which is usually called violation of local position invariance. The strongest limits kα+0.17ke=(-3.5±6)*10-7 are obtained from the measurements of dependence of atomic frequencies on the distance from Sun (the distance varies due to the ellipticity of the Earth's orbit).
AB - Light scalar fields very naturally appear in modern cosmological models, affecting such parameters of Standard Model as electromagnetic fine structure constant α, dimensionless ratios of electron or quark mass to the QCD scale, me,q/ΛQCD. Cosmological variations of these scalar fields should occur because of drastic changes of matter composition in Universe: the latest such event is rather recent (redshift z∼0.5), from matter to dark energy domination. In a two-brane model (we use as a pedagogical example) these modifications are due to changing distance to "the second brane", a massive companion of "our brane". Back from extra dimensions, massive bodies (stars or galaxies) can also affect physical constants. They have large scalar charge Qd proportional to number of particles which produces a Coulomb-like scalar field =Qd/r. This leads to a variation of the fundamental constants proportional to the gravitational potential, e.g. δα/α=kαδ (GM/rc2). We compare different manifestations of this effect, which is usually called violation of local position invariance. The strongest limits kα+0.17ke=(-3.5±6)*10-7 are obtained from the measurements of dependence of atomic frequencies on the distance from Sun (the distance varies due to the ellipticity of the Earth's orbit).
KW - Variation fundamental constants
UR - https://www.scopus.com/pages/publications/42549105477
U2 - 10.1063/1.2915601
DO - 10.1063/1.2915601
M3 - Conference contribution
AN - SCOPUS:42549105477
SN - 9780735405141
T3 - AIP Conference Proceedings
SP - 1
EP - 11
BT - Nuclei and Mesoscopic Physics - Workshop on Nuclei and Mesoscopic Physics, WNMP 2007
T2 - 2nd Workshop on Nuclei and Mesoscopic Physics, WNMP 2007
Y2 - 20 October 2007 through 22 October 2007
ER -