White dwarf star throws light on possible variability of a constant of Nature

Jul 04, 2013
Researchers have studied a distant star where gravity is more than 30,000 times greater than on Earth to test the controversial theory that one of the constants of Nature -- the strength of the electromagnetic force, known as alpha -- is not a constant. Credit: UNSW

An international team led by the University of New South Wales has studied a distant star where gravity is more than 30,000 times greater than on Earth to test its controversial theory that one of the constants of Nature is not a constant.

Answering the ultimate question to Life, Universe and Everything? Not quite, but an international team of scientists have conducted research that opens up new possibilities for exploring what have previously only been theories of physics. Using the Hubble Space Telescope, the astronomers have tested whether the strength of the electromagnetic force is altered in the strong gravitational field of a white dwarf star. Team member Professor Martin Barstow of the University of Leicester will present the new work at the RAS National Astronomy Meeting in St Andrews, Scotland.

In a letter in the journal Physical Review Letters, the team from the University of Leicester, University of Cambridge, University of Arizona and University of New South Wales highlight the potential impact of their research.

"The research opens up new possibilities for searching for exotic "scalar fields", forms of energy that often appear in theories of physics that seek to combine the Standard Model of particle physics with Einstein's general theory of relativity," said Professor Barstow.

The electromagnetic force is one of four fundamental forces that shape the universe. Its strength is given in the Standard Model by a pure number, with no units, known as the "fine-structure constant", denoted by the Greek letter alpha (α). Combining the speed of light, the electric charge of an electron, and Planck's constant, alpha has always been measured on earth to have the same value, approximately 1/137.

A key question is whether alpha changes in different parts of the Universe or in strong gravity fields. Recent observations of light from distant quasars (luminous sources thought to be caused by material heating up as it swirls around a black hole) hint that the fine-structure constant varies over the sky at large distances. But as yet there is no independent check for this result.

Some theories predict that alpha will vary in the presence of exotic scalar fields like those that are invoked to help unite the Standard Model with Einstein's theory of general relativity that describes gravitation.

White dwarf stars, the compact remnants left behind when stars like the Sun reach the end of their lives are an ideal natural laboratory to test this idea. With a lot of matter packed into a sphere about the size of the Earth, they have strong gravitational fields.

By measuring the value of alpha near a white dwarf, and comparing it with its value here and now in the laboratory, astronomers can indirectly probe whether these alpha-changing scalar fields actually exist.

The team measured alpha for the first time the white dwarf star G191-B2B using iron and nickel ions (atoms where electrons are added or removed to give them a net electrical charge) trapped in the atmosphere of the white dwarf. Despite the strong gravitational field of the white dwarf - nearly 100,000 times that on Earth - the ions stay above the surface because they are continually pushed up by the strong radiation from the star.

The ions absorb some of the light from the white dwarf, making an "absorption spectrum" that was observed using the Hubble Space Telescope. That absorption spectrum allows the scientists to probe the value of alpha in the atmosphere of the white dwarf with high accuracy. By comparing the positions of the absorption lines measured by the telescope with the positions measured in the laboratory, they can tell whether alpha is different near the white dwarf.

Professor Barstow adds: "We found that any difference between the value of alpha on Earth and that measured in the strong gravitational field of the white dwarf must be smaller than a part in ten thousand, which means that any scalar fields must only weakly affect the electromagnetic force.

'Unfortunately, our work was limited by the need to use very old laboratory measurements from the 1970s. In the future, with better laboratory data to complement the high-precision astronomical data, we should be able to measure the change in alpha down to one part per million. At that level we would be able to place strong restrictions on whether alpha is a true constant of nature."

Explore further: Researchers demonstrate ultra low-field nuclear magnetic resonance using Earth's magnetic field

More information: Their work appears in "Limits on variations of the fine-structure constant with gravitational potential from white-dwarf spectra", Physical Review Letters, J. C. Berengut, V. V. Flambaum, A. Ong, J. K. Webb, John D. Barrow, M. A. Barstow, S. P. Preval, J. B. Holberg, in press. A preprint of the paper can be seen at arxiv.org/pdf/1305.1337.pdf

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danut_sun
1 / 5 (1) Jul 04, 2013
So, Mr. Rupert Sheldrake is right after all?
SHREEKANT
1 / 5 (8) Jul 04, 2013
"This idea that the laws of physics are different in different places in the cosmos is a huge claim, and needs to be backed up with solid evidence," he says.

I have already written in my blog [swarajgroups.blogspot.in ] under title 'OUT OF BOX THINKING' ,20th,June'13

"Our mathematical approach is good, but it is for 'justifying/proving our assumption & theory' not always for 'explaining theory & assumption'. 
Take an example of gravitational force 'F'=GMm/r², 
                                                                    here the value of F depends on certain factors only, as shown in the formula. It is also true that this is proved many times.
But no one claim that the value of F at particular point is only due to above mentioned factor only. 
Let us take Virial theorem, is the reason of particular value of 'F' is so simple?
At earth it is due to some different set of situation & at Neptune or at the 'planet of other stars'[situated in another galaxy]; it is due to different set of situation."

I WANT TO PROTECT MY DETAILED WORK BEFORE DISCLOSING.
brt
5 / 5 (2) Jul 05, 2013
SHREEKANT,

That's basic physics that scientists and engineers learn in undergraduate programs in college. You don't have to worry about your 'detailed work' because it's about 170 years old.
ValeriaT
1 / 5 (1) Jul 05, 2013
In GUT theory all forces should vanish mutually into supergravity at large energy density. I.e. the ratio of relative strength of electromagnetic force and gravity which is expressed with fine-structure constant should converge to 1.The fine structure constant α = e²/2ε0hc is a running constant, and thus isn't actually constant, see for example the NIST web, where you can read:
"Thus α depends upon the energy at which it is measured, increasing with increasing energy, and is considered an effective or running coupling constant. Indeed, due to e+e- and other vacuum polarization processes, at an energy corresponding to the mass of the W boson (approximately 81 GeV, equivalent to a distance of approximately 2 x 10-18 m), α(mW) is approximately 1/128 compared with its zero-energy value of approximately 1/137. Thus the famous number 1/137 is not unique or especially fundamental"
Note that varying with energy also infers varying with gravitational potential due to the spatial self-energy of a gravitational field. When you spot a variation in fine structure constant out in space, what you're actually seeing is a variation in spatial energy density. This inhomogeneity causes gravity, and of course energy has a mass equivalence. Gravitationally speaking, it acts just like matter.
So that the values of natural constants can change quite easily, for example with passing of matter through dense cloud of (anti)neutrinos, which are difficult to detect and which would increase the mass density of vacuum with compare to mass density of observable matter. As the result, the observable matter would swell in the more dense vacuum and the gravity constants and fine structure constants would decrease. So we can observe the changes in speed of light, gravity constant, mass of kilogram prototype and/or the lenght of meter prototype.