Dr John Hartnett
Physics, Cosmology (Australia)
Biography
John G. Hartnett received both his B.Sc. (hons) and his Ph.D. with distinction from
the Department of Physics at the University of Western Australia (UWA). He works
with the Frequency Standards and Metrology research group, holding the rank of tenured
Research Professor (the equivalent of Reader in the UK, would be Full Professor
in the USA). See John’s university
web page.
John’s research interests include the development of ultra-stable cryogenically
cooled microwave oscillators based on a sapphire crystal, ultra low-noise radar,
tests of fundamental theories of physics such as Special and General Relativity
and measurement of drift in fundamental constants and their cosmological implications.
John has a keen interest in cosmology and how it applies to the creationist world-view.
He is also developing new physics that has established that there is no need to
assume the existence of dark matter in the universe. He has published more than
150 papers in scientific journals and holds 2 patents.
Stop press, 5 March 2010
Dr Hartnett has just been announced as the winner of the 2010 W.G. Cady award by
IEEE Ultrasonics, Ferroelectrics and Frequency Control Society.
The W.G. Cady Award recognizes outstanding contributions in the fields of piezoelectric
or other classical frequency control, selection and measurement and resonant sensor
devices.
The citation reads: “for the construction of ultra-stable cryogenic sapphire
dielectric resonator oscillators and promotion of their applications in the fields
of frequency metrology and radio-astronomy.”
The award will be presented during the 2010 IEEE International Frequency Control Symposium at Newport Beach, California in June.
Last year’s winner was Sir Eric Ash.
Products
Interview
Ground-breaking cosmological papers for secular journals
- Hartnett, J.G.,
The distance modulus determined from Carmeli’s cosmology fits the accelerating
universe data of the high-redshift type Ia supernovae without dark matter, Found.
Phys. 36(6):839–861, June 2006. <arxiv.org/abs/astro-ph/0501526>
- Hartnett, J.G.,
Spiral galaxy rotation curves determined from Carmelian general relativity,
Int. J. Theor. Phys. 45(11):2118–2136, November
2006. <arxiv.org/abs/astro-ph/0511756>
- Hartnett, J.G., Tobar, M.E.,
Properties of gravitational waves in Cosmological general relativity, Int. J.
Theor. Phys. 45(11):2181–2190, November 2006. <arxiv.org/abs/gr-qc/0603067>
- Oliveira, F.J., Hartnett, J.G.,
Carmeli’s cosmology fits data for an accelerating and decelerating universe
without dark matter or dark energy, Found. Phys. Lett. 19(6):519–535,
November 2006. <arxiv.org/abs/astro-ph/0603500>
- Hartnett, J.G., Oliveira,F.J.,
Luminosity distance, angular size and surface brightness in Cosmological General
Relativity, Found. Phys. 37(3):446–454, 2007.
<arxiv.org/abs/astro-ph/0603500>
- Hartnett, J.G.,
Spheroidal and elliptical galaxy radial velocity dispersion determined from Cosmological
General Relativity, Int. J. Theor. Phys. 47(5): 1252–1260,
2008. <arxiv.org/abs/0707.2858>
- Hartnett, J.G.,
Extending the redshift-distance relation in Cosmological General Relativity to higher
redshifts, Found. Phys. 38(3): 201–215, 2008.
<arxiv.org/abs/0705.3097>
- J.G. Hartnett, K. Hirano,
Galaxy redshift abundance periodicity from Fourier analysis of number counts N(z)
using SDSS and 2dF GRS galaxy surveys, Astrophysics and Space Science,
Vol. 318, No. 1 & 2, pp. 13-24, 2008. <arxiv.org/abs/0711.4885>
Articles for CMI
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