Macronix Research Corporation was established in 1986, to complete and operate Pulsed Power facility of the National Research Council of Canada. In the eighties and nineties, Macronix provided consulting services to the industry and the government in the field of finite-element modeling of electrical and magneto-hydrodynamics devices. Currently our focus is on Process & Product development and Quality Assurance, in large scale industries. Macronix provides consulting services across the globe to our clients in North America, South America, Europe, Middle East, Asia, Africa, and Australia.
About
Macronix was federally incorporated in Canada in 1986 to complete and operate the Pulsed Power (1 MJ, 1 TW) facility of the National Research Council of Canada on Montreal Road, Ottawa, and to provide consultancy to industry and the government. Founding directors included Professor Peter Silvester, Head of the Electrical Engineering Department at McGill University, and Dr. Rajendra Gupta, Senior Research Officer at the National Research Council, who was also a visiting professor at McGill at that time. NRC provided its staff and initial funding for the operation of the facility and McGill provided the graduate students to do frontier research using it. One student obtained a master’s degree and another student obtained a Ph.D. degree under Dr. Gupta, both from McGill, for their work done at the facility. The research continued on the facility five years term for the use of the facility by Macronix. During the course of this work multiple research papers were published.
Macronix also provided consulting to industry and government in the field of finite element modelling of electrical and magneto-hydrodynamics devices in the eighties and nineties. More recently the focus has been on process and product development, quality assurance, database development, IT security, etc.
The company’s consulting staff has over 100 years of cumulative research, teaching, and consulting experience in diversified fields with close to 100 publication, including 15 patents, and possess Ph.D. and Master’s degrees and other advanced qualifications in science and engineering.
© macronix.ca 2016-2021
Our Work
Macronix provides world leading expertise in design and development of products, plants and machines. We engage with our customers in R&D phase of the project which include product design, design validation and process qualification. We provide turnkey solutions for New Product Introduction (NPI), Design for Manufacturing (DFM), Statistical Process Control (SPC) during production, Reliability tests, and Failure Analysis (FA). Our goal is to provide our customers with high-quality robust solutions. Our consulting staff has comprehensive experience in a wide range of industries such as Food Technology, Information Services, and Semiconductor Manufacturing.
In addition, Macronix performs high-quality technical research work for our clients. Some of the areas of our interest are Database management, IT security, Quantum computing and its applications, Block-Chain technology, and Mesh networks.
We have developed advanced cosmological models and made predictions for their testing by ELT (Extremely Large Telescope) that is being built in Chile, and by other astronomical facilities of the future on ground and in space. Some of our recent publications in Cosmology, are listed below:
Will ΛCDM Model Survive the High Redshift Data Generated by ELT?
Abstract: Today, the most reliable data for testing cosmological theories is based on the redshift z vs. distance modulus µ measurements of supernovae Ia in the redshift range of about 0.015 < z < 1.5. Several models can fit the data admirably well in this range, the most accepted one being the ΛCDM model using the Einstein’s cosmological constant Λ for dark energy. However, there is discrepancy between various models near the redshift of 1.5. Due to significant error and scatter in the data, it is not possible to ascertain the best fit model with high confidence level. We have proposed a hybrid model according to which the redshift is caused by expansion of the universe as per Einstein-de Sitter model as well as by the tired light phenomenon due to Mach effect. The prediction of our single parameter hybrid model, dubbed EDSM (Einstein-de Sitter-Mach) model, that requires an unaccounted luminosity flux loss proportional to 1/sqrt(1+z), due possibly to the nonadiabatic nature of the universe, can be easily tested by extending the supernovae redshift data well beyond z = 1.5. This EDSM model in nonadiabatic universe yields Hubble constant of 68.28 km/s/Mpc that is almost right at the weighted average of 68.1 km/s1/Mpc reported from WMAP and Plank data points without any adjustable parameter other than the Hubble constant. We will present our model’s prediction against that of ΛCDM model in the high z range for testing them by future observations with Extremely Large Telescope. For example, two parameter ΛCDM model projects µ = 51.11 at z = 15 whereas one parameter nonadiabatic EDSM model projects µ = 52.13 at z = 15. Will ΛCDM model survive the high redshift data generated by Extremely Large Telescope?
SNe Ia Redshift in a Nonadiabatic Universe
Universe 2018, 4(10), 104; https://doi.org/10.3390/universe 4100104.
Determination of the Mach effect contribution to the red shift
International Conference – COSMOLOGY ON SMALL SCALES 2018: Dark Matter Problem and Selected Controversies in Cosmology, September 26–29, 2018, Institute of Mathematics, Czech Academy of Sciences, Zitna 25, Prague, Czech Republic.
Static and Dynamic Components of the Redshift
International Journal of Astronomy and Astrophysics
Vol.08 No.03(2018), Article ID:86524, 11 pages, 10.4236/ijaa.2018.83016.
Mass of the Universe and the Redshift
International Journal of Astronomy and Astrophysics, 8, 68-78, doi: 10.4236/ijaa.2018.81005.
The complete list of our work can be found here.
Contact
You can reach us either via email at contact@macronix.ca or by telephone at (613) 302-1595.