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particular solution luyeš-e pâruli Fr.: solution particulière Of partial differential equations, the solution which can be obtained from the general solution by particular choice of the arbitrary functions. → general solution; → singular solution. → particular; → solution. |
partition 1) parke; 2) parkeš 3) parkidan Fr.: 1, 2) parition, cloison, division; 3) cloisonner, diviser 1a) A division into or distribution in portions or shares. M.E., from O.Fr. particion, from L. partition- "division, partition, distribution," from p.p. stem of partire "to part, divide," from PIE root *per- "to grant, allot," related to → part and akin to pake, as below. Parke, from Kermâni parke "piece, part, fragmant," related to pâr "→ part;" parkidan, infinitive from parke; parkeš, verbal noun of parkidan. |
partition function karâ-ye parkeš Fr.: fonction de partition See → integer partition. |
partition ratio vâbar-e parkeš Fr.: rapport de partition The ratio of the → concentration of a → solute in a single definite form in the stationary phase to its concentration in the same form in the other phase at equilibrium. |
partitioning parkebandi Fr.: partition A chemical separation process whereby a solute is distributed between two phases. |
partitionment parkebandi Fr.: The act or fact of being partitioned. |
parton pârton (#) Fr.: parton In particle physics, a constituent of the hadron originally postulated in the theoretical analysis of high-energy scattering of particles off hadrons. In modern usage, the term parton is often used to mean a quark or a gluon. Coined by the American physicist Richard Feynman (1918-1988), from part, from → particle + → -ion |
parts per million (ppm) pâr dar milion Fr.: partie par million A fraction of a whole number in units of 1/1000,000. It is usually used to describe chemical concentrations, very small amounts of pollutants in air, water, body fluids, and uncertainty. For example 30 ppm is 3 x 10-5 or 0.003%. |
passive component hamne-y akâr Fr.: composante passive An electronic component which contains no source of power, in contrast to active components. |
Pauli exclusion principle parvaz-e sokolân-e Pauli Fr.: principe d'exclusion de Pauli A quantum mechanical principle according to which no two identical → fermions can share the same → quantum state. Also known as → exclusion principle. In honor of Wolfgang Pauli (1900-1958), Austrian theoretical physicist, who formulated the principle in 1925; → exclusion; → principle. |
pebble accretion farbâl-e rig Fr.: accrétion de galets A planet formation concept that concerns the → accretion of small objects of negligible gravitational mass (ranging from centimeters up to meters in diameter) onto large, gravitating bodies: → planetesimals, → protoplanets, or → planets. In a more narrow sense, pebble accretion is an accretion process where (gas) drag and gravity play major roles. Simply put, this means that the pebble has to be aerodynamically small and the planet to be gravitationally large (C. W. Ormel, in Formation, Evolution, and Dynamics of Young Solar Systems, p. 197, eds. M. Pessah, O. Gressel, Springer, 2017). |
peculiar motion jonbeš-e afd Fr.: mouvement particulier 1) The true motion of a star with respect to the Local Standard
of Rest. → proper motion. |
pejoration pastâeš Fr.: péjoration 1) Depreciation; a lessening in worth, quality, etc. Verbal noun of → pejorate. |
peony payoniyâ Fr.: pivoine Any plant of the genus Paeonia, having showy, pink, red, or white, globular flowers. Originally cultivated in the temperate regions of Asia, China, Europe, and the northwest parts of North America. M.E., from M. Fr. peonie, pioiné, from L.L. peonia, from L. pæonia, from Gk. paionia, perhaps from Paion, physician of the gods. The plant was recognized to possess many remedial properties, and was thus given an association with the gods. Payoniyâ, loan from Gk, as above. |
Peony star Setâre-ye Payoniyâ Fr.: Etiole Pivoine A peony-shaped nebula around the → Wolf-Rayet star WR 102ka as shown by the → Spitzer Space Telescope image at 24 μm. The formation of this infrared bright nebula is attributed to the recent evolutionary history of WR 102ka during → LBV-type eruptions and/or its strong → stellar wind (see, e.g., A. Barniske et al. 2008, A&A 486, 971). |
perception âgerteš Fr.: perception The process of recognizing or identifying something. Usually employed of sense perception, when the thing which we recognize or identify is the object affecting a sense organ. Verbal noun of → perceive. |
perfection farsâxtegi, farsâzeš Fr.: perfection The state or quality of being or becoming perfect. |
perfectionism farsâxtgerâyi, farsâxtgari Fr.: perfectionisme 1) Any of various doctrines holding that religious, moral, social, or political
perfection is attainable. → perfection; → -ism. |
perfectionist farsâxtgerâ, farsâxtgar Fr.: perfectioniste 1) A person who adheres to or believes in → perfectionism. → perfection; → -ist. |
periastron pirâaxtar Fr.: périastre In a binary system, the point in the orbit where a component is nearest the other component; opposite of → apastron. |
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