Predictive models of the galaxies’ movement speeds and accelerations of movement on applying the Doppler Effect

Skeivalas, Jonas; Turla, Vytautas; Jurevičius, Mindaugas

doi:10.1007/s12648-018-1264-7

Use this URL to cite this publication: https://hdl.handle.net/20.500.14911/121660

Predictive models of the galaxies’ movement speeds and accelerations of movement on applying the Doppler Effect

Details

Publication Type (CRIS)

Straipsnis Web of Science ir Scopus duomenų bazėje / Article in Web of Science and Scopus database (S1)

Publication Type (eLABa)

Straipsnis Web of Science DB / Web of Science DB article (S1)

VILNIUS TECH Research Priorities and Topics

Efektyvus išteklių ir energijos naudojimas / Efficient use of resources and energy (AE0101)

Lithuanian Intelligent Specialization

Energetika ir tvari aplinka / Energy and a sustainable environment (L102)

Author(s)

Author	Affiliation
Skeivalas, Jonas	Geodezijos ir kadastro katedra / Department of Geodesy and Cadastre (0323)
Turla, Vytautas	Mechatronikos, robotikos ir skaitmeninės gamybos katedra / Department of Mechatronics, Robotics and Digital Manufacturing (0450)
Jurevičius, Mindaugas	Mechanikos ir medžiagų inžinerijos katedra / Department of Mechanical and Material Engineering (0449)

Title

Predictive models of the galaxies’ movement speeds and accelerations of movement on applying the Doppler Effect

[en]

Jonas Skeivalas, Vytautas Turla, Mindaugas Jurevičius

Is part of

Indian journal of physics

Published In

Year	Volume	Issue	Start Page	End Page
2019	93	1	1	6

Publisher

Kolkata : Springer

Publisher (trusted)

Indian Association for the Cultivation of Science

Referenced in Database(s)(DBs)

ProQuest Central

OCLC Article First

Gale's Academic OneFile

INSPEC

SpringerLink

SCOPUS

Science Citation Index Expanded (Web of Science)

Extent

p. 1-6

URI

URI	Access Rights
https://hdl.handle.net/20.500.14911/121660
https://doi.org/10.1007/s12648-018-1264-7	Viso teksto dokumentas (prieiga prenumeratoriams) / Full Text Document (Access for Subscribers)

DOI

10.1007/s12648-018-1264-7

Cited references

Science / Art Area

Technologijos mokslai / Technological sciences (T)

Field of Science / Art

Matavimų inžinerija / Measurement engineering (T010)

Mechanikos inžinerija / Mechanical Engineering (T009)

Keywords (en)

Abstract (en)

This article discusses the theoretical assumptions for the development of a predictive model of galaxy movement speed and acceleration on applying the measurement data of the parameter z in the formula for the Doppler Effect. Galaxy movement speed and acceleration are understood as multidimensional continuous values when the values of vectors of speed and acceleration are calculated according to the redshift parameter z measurements in the relevant Universe time moments. Galaxy movement acceleration is obtained as a partial derivative of galaxy speed with respect to the time t of oscillations of the received redshift signal. The theoretical expressions of the functions of galaxy speed and acceleration are obtained by approximating in the form of a polynomial when the values of the polynomial parameters are established by the least squares method on applying operators of the Matlab set of programs.