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Number of Results: 1965 Search : ion

fusion 1, 2, 3) iveš; 3) godâz (#) Fr.: fusion 1) The act or process of fusing; the state of being
→ From M.Fr. Verbal noun form of → |

fuzzification porzvâreš Fr.: fuzzification The first step carried out in a → |

galactic rotation carxeš-e kahkešân Fr.: rotation galactique The revolving of the gaseous and stellar content of a galaxy around its central nucleus. The rotation is not uniform, but differential. One revolution of the Sun within our own Galaxy takes about 220 million years, or one cosmic year. |

galactic rotation problem parâse-ye carxeš-e kahkešâni Fr.: problème de la rotation galactique The discrepancy between observed galaxy → |

galaxy formation diseš-e kahkešân Fr.: formation de galaxies The study dealing with the processes that gave rise to galaxies in a remarkably
→ |

Galilean transformation tarâdis-e Gâlile-yi (#) Fr.: transformation galiléenne The method of relating a measurement in one
→ → |

galvanization gâlvâneš Fr.: galvanisation The coating of steel or iron with → Verbal noun of → |

Gamow condition butâr-e Gamow Fr.: condition de Gamow The constraint on the → n is the baryon number density,
σ is the cross section for the reaction
at relative → _{b}velocity v,
and t the expansion time-scale for the
→ Universe. This means that the time-scale for the
above reaction is comparable to the expansion time. From this condition the baryon
number density at the start of element buildup is found to be
n ~ (σ_{b}vt)^{-1} ~ 10^{18} cm^{-3} at
T = 10^{9} K (P. J. E. Peebles, 2013,
Discovery of the Hot Big Bang: What happened in 1948,
arXiv.1310.2146).→ |

gas equation hamugeš-e gâz Fr.: équation des gaz An equation that links the pressure and volume of a quantity of gas with the absolute temperature.
For a gram-molecule of a perfect gas, |

gaseous diffusion paxš-e gâzi Fr.: diffusion gazeuse An → |

gauge transformation tarâdis-e gaz (#) Fr.: transformation de jauge A change of the fields of a gauge theory that does not change the value of any measurable quantity. → |

Gaussian distribution vâbâžeš-e Gaussi (#) Fr.: distribution gaussienne A theoretical frequency distribution for a set of variable data, usually represented by a bell-shaped curve with a mean at the center of the curve and tail widths proportional to the standard deviation of the data about the mean. → |

Gaussian elimination osâneš-e Gaussi Fr.: élimination de Gauss A method of solving a matrix equation of the form
A → |

Gaussian function karyâ-ye Gauss Fr.: fonction de Gauss The function |

Gaussian gravitational constant pâyâ-ye gerâneši-ye Gauss Fr.: constante gravitationnelle de Gauss The constant, denoted L .
Its value is: ^{3}M ^{-1}T ^{-2}k = 0.01720209895.→ |

general precession pišâyân-e harvin Fr.: précession générale The secular motions of the → → |

general precession in longitude pišâyân-e harvin-e derežnâ Fr.: précession générale en longitude The secular displacement of the → → |

general precession in right ascension pišâyân-e harvin-e râst afrâz Fr.: précession générale en ascension droite The secular motion of the → → |

generalization harvinkard, harvineš Fr.: généralisation The act or process of generalizing; → Verbal noun of → |

generation âzâneš Fr.: génération 1) A coming into being. Verbal noun of → |

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