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Stars as Laboratories for Fundamental Physics - MPP Theory Group

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546 Chapter 15<br />

vacuum expectation value of a physical field w<strong>as</strong> more plausibly subject<br />

to variations than dimensionless constants such <strong>as</strong> gauge and Yukawa<br />

couplings.<br />

Type Ia supernovae are thought to represent the nuclear deflagration<br />

of a white dwarf pushed beyond its Chandr<strong>as</strong>ekhar limit by accretion<br />

(e.g. Woosley and Weaver 1986b). There<strong>for</strong>e, their light curves are<br />

very reproducible and indeed serve <strong>as</strong> standard candles in an attempt<br />

to improve me<strong>as</strong>urements of the cosmic expansion rate. The shape of<br />

the lightcurve is determined by radioactive heating of the SN remnant<br />

by the decay of 56 Co; its lifetime is proportional to G −2<br />

F . A change of<br />

order 10% in the slope of type Ia SN lightcurves in neighboring galaxies<br />

(Leibundgut et al. 1991) would be readily observable so that G F must<br />

be constant within at le<strong>as</strong>t 5% over 30 Mpc distances.<br />

In addition, Scherrer and Spergel showed that the agreement between<br />

the observed primordial light element abundances and big-bang<br />

nucleosynthesis calculations imply that G F lay within −1% and +9%<br />

of its standard value at this early epoch.<br />

A stringent constraint on the local 93 time variation of G F obtains<br />

from the analysis of ores from the Oklo uranium mine where a natural<br />

fission reactor is thought to have operated about 2 Gyr ago (e.g.<br />

Maurette 1976). A shift of the ground state difference between 150 Sm<br />

and 149 Sm by more than 0.02 eV is inconsistent with the isotope ratios<br />

at Oklo (Shlyakhter 1976, 1983). According to this author the<br />

contribution of the weak interaction to the nuclear binding energy is<br />

about 200 eV, excluding a change of G F by more than 0.1% over the<br />

p<strong>as</strong>t 2 Gyr.<br />

15.2 Constancy of Newton’s Constant<br />

15.2.1 Present-Day Constraints from Celestial Mechanics<br />

Another “constant of nature” that might vary in time is Newton’s constant<br />

G N . Indeed, there exist self-consistent alternative theories to<br />

general relativity which actually predict a temporal variation of G N on<br />

cosmological time scales—see Will (1993) <strong>for</strong> a summary of such theories<br />

and detailed references. A typical scale <strong>for</strong> the rate of change<br />

is the cosmic expansion parameter H so that it is natural to write<br />

Ġ N /G N = σH with σ a dimensionless model-dependent number. Some<br />

93 The Earth moves with the galaxy and the local group relative to the cosmic<br />

microwave background (CMB). Taking 600 km s −1 <strong>for</strong> this peculiar velocity the<br />

Earth moves by about 1.2 Mpc in 2 Gyr relative to a frame defined by the CMB.

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