Friday, 8 April 2022

āĻŽāĻšাāύ āφāϞ্āϞাāĻš āĻŦāϞāĻ›েāύ, āφāĻŽি āύিāϜ āĻšাāϤে āφāϏāĻŽাāύ āϏৃāώ্āϟি āĻ•āϰেāĻ›ি āĻāĻŦং āφāĻŽিāχ āĻāϰ āĻŦিāϏ্āϤৃāϤি āϘāϟাāχ। (āϏুāϰা : āϜাāϰি⧟াāϤ, āĻ†ā§ŸাāϤ : ā§Ēā§­)

āĻ…āύ্āϝ āĻ…āύুāĻŦাāĻĻ👇

āφāĻŽি āύিāϜ āĻšাāϤ āĻĻ্āĻŦাāϰা āφāϏāĻŽাāύ āϏৃāώ্āϟি āĻ•āϰেāĻ›ি āφāϰ āφāĻŽি āĻ…āĻŦāĻļ্āϝāχ āĻŽāĻšা āĻĒ্āϰāĻļāϏ্āϤāĻ•াāϰী। āϤাāχāϏিāϰুāϞ

āφāĻŽি āφāĻ•াāĻļ āύিāϰ্āĻŽাāĻŖ āĻ•āϰেāĻ›ি āφāĻŽাāϰ āĻ•্āώāĻŽāϤা āĻŦāϞে āĻāĻŦং āφāĻŽি āĻ…āĻŦāĻļ্āϝāχ āĻŽāĻšাāϏāĻŽ্āĻĒ্āϰāϏাāϰāĻŖāĻ•াāϰী, āĻŽুāϜিāĻŦুāϰ āϰāĻšāĻŽাāύ

And the heaven We constructed with strength, and indeed, We are [its] expander

Expansion of the universe - Wikipedia
The expansion of the universe is the increase in distance between any two given gravitationally unbound parts of the observable universe with time. [1] It is an intrinsic expansion whereby the scale of space itself changes. The universe does not expand "into" anything and does not require space to exist "outside" it. This expansion involves neither space nor objects in space "moving" in a traditional sense, but rather it is the metric (which governs the size and geometry of spacetime itself) that changes in scale. As the spatial part of the universe's spacetime metric increases in scale, objects become more distant from one another at ever-increasing speeds. To any observer in the universe, it appears that all of space is expanding, and that all but the nearest galaxies (which are bound by gravity) recede at speeds that are proportional to their distance from the observer . While objects within space cannot travel faster than light , this limitation does not apply to the effects of changes in the metric itself. [notes 1] Objects that recede beyond the cosmic event horizon will eventually become unobservable, as no new light from them will be capable of overcoming the universe's expansion, limiting the size of our observable universe . As an effect of general relativity , the expansion of the universe is different from the expansions and explosions seen in daily life. It is a property of the universe as a whole and occurs throughout the universe, rather than happening just to one part of the 
And the heaven We constructed with strength, and indeed, We are [its] expander
Expansion of the universe - Wikipedia
The expansion of the universe is the increase in distance between any two given gravitationally unbound parts of the observable universe with time. [1] It is an intrinsic expansion whereby the scale of space itself changes. The universe does not expand "into" anything and does not require space to exist "outside" it. This expansion involves neither space nor objects in space "moving" in a traditional sense, but rather it is the metric (which governs the size and geometry of spacetime itself) that changes in scale. As the spatial part of the universe's spacetime metric increases in scale, objects become more distant from one another at ever-increasing speeds. To any observer in the universe, it appears that all of space is expanding, and that all but the nearest galaxies (which are bound by gravity) recede at speeds that are proportional to their distance from the observer . While objects within space cannot travel faster than light , this limitation does not apply to the effects of changes in the metric itself. [notes 1] Objects that recede beyond the cosmic event horizon will eventually become unobservable, as no new light from them will be capable of overcoming the universe's expansion, limiting the size of our observable universe . As an effect of general relativity , the expansion of the universe is different from the expansions and explosions seen in daily life. It is a property of the universe as a whole and occurs throughout the universe, rather than happening just to one part of the universe. Therefore, unlike other expansions and explosions, it cannot be observed from "outside" of it; it is believed that there is no "outside" to observe from. Metric expansion is a key feature of Big Bang cosmology , is modeled mathematically with the Friedmann–LemaÃŽtre–Robertson–Walker metric and is a generic property of the universe we inhabit. However, the model is valid only on large scales (roughly the scale of galaxy clusters and above), because gravity binds matter together strongly enough that metric expansion cannot be observed on a smaller scale at this time. As such, the only galaxies receding from one another as a result of metric expansion are those separated by cosmologically relevant scales larger than the length scales associated with the gravitational collapse that are possible in the age of the universe given the matter density and average expansion rate. According to inflation theory , during the inflationary epoch about 10 −32 of a second after the Big Bang , the universe suddenly expanded, and its volume increased by a factor of at least 10 78 (an expansion of distance by a factor of at least 10 26 in each of the three dimensions). This would be equivalent to expanding an object 1 nanometer (10 −9 m , about half the width of a molecule of DNA ) in length to one approximately 10.6 light years (about 10 17 m or 62 trillion miles) long. A much slower and gradual expansion of space continued after this, until at around 9.8 billion years

⧧⧝⧍ā§Ļ-ā§§ā§¯ā§Šā§Ļ āϏাāϞ āĻĒāϰ্āϝāύ্āϤ āĻ—āĻŦেāώāĻŖা āĻ•āϰে āĻŦিāϜ্āĻžাāύী āĻšাāĻŦāϞ āφāĻŦিāώ্āĻ•াāϰ āĻ•āϰেāύ āϝে āĻ—্āϰāĻš āύāĻ•্āώāϤ্āϰāĻ—ুāϞো āĻĒāϰāϏ্āĻĒāϰ āĻĨেāĻ•ে āϏāϰে āϝাāϚ্āĻ›ে।āϤāĻ–āύ āϤিāύি āϏিāĻĻ্āϧাāύ্āϤ āύেāύে āĻŽāĻšাāĻŦিāĻļ্āĻŦ āϏāĻŽ্āĻĒ্āϰāϏাāϰāĻŖāĻļীāϞ।

https://www.pnas.org/content/112/11/3173#%3A~%3Atext%3DIn%20his%20short%20paper%2C%20Hubble%2Crecede%20faster%20than%20nearby%20galaxies

āĻŽāĻšাāύāĻŦী(āϏ) āϏāĻŽ্āĻ­āĻŦāϤ āϟাāχāĻŽ āϟ্āϰাāĻ­েāϞ āĻ•āϰে ā§§ā§¯ā§Šā§Ļ āĻ āĻāϏে āĻšাāĻŦāϞেāϰ āĻ•্āϞাāϏ āĻ•āϰে āϤাāϰāĻĒāϰ āĻāϟা āĻ•ুāϰāφāύ āĻ āϞিāĻ–েāĻ›েāύ।

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āφāϞ্āϞাāĻš āϤা⧟াāϞা āĻĒāĻŦিāϤ্āϰ āĻ•োāϰāφāύে āĻŦāϞেāĻ›েāύ, āĻŽাāύুāώ āĻ•ি āĻŽāύে āĻ•āϰে āϝে, āφāĻŽি (āφāϞ্āϞাāĻš) āϤাāϰ āĻ…āϏ্āĻĨিāϏāĻŽূāĻš āĻāĻ•ে āĻ…āύ্āϝāϰ āϏাāĻĨে āĻāĻ•āϤ্āϰিāϤ āĻ•āϰāĻŦ? āϤাāĻšāϞে āϤাāĻĻেāϰ āĻŦāϞো āĻ•েāĻŦāϞ āĻāχ āύ⧟, āφāĻŽি āϤাāϰ āφāĻ™্āĻ—ুāϞেāϰ āĻĄāĻ—া (āφāĻ™্āĻ—ুāϞেāϰ āĻ›াāĻĒ) āĻĒāϰ্āϝāύ্āϤ āφāϞাāĻĻা āĻ•āϰāϤে āϏāĻ•্āώāĻŽ। (āϏূāϰা āĻ•ি⧟াāĻŽাāϤ, ā§Ļā§Š : ā§Ļā§Ē)

ā§§ā§¯ā§Žā§Ļ āϏাāϞে āĻĢ্āϰাāύ্āϏি āĻ—াāϞāϟāύ āĻĢিāĻ™্āĻ—াāϰāĻĒ্āϰিāύ্āϟ āφāĻŦিāώ্āĻ•াāϰ āĻ•āϰেāύ āĻ“ āĻĢāϰেāύāϏিāĻ• āĻĄিāĻĒাāϰ্āϟāĻŽেāύ্āϟ āĻ āϤা āĻŦ্āϝāĻŦāĻšাāϰেāϰ āĻ•াāϰ্āϝāĻ•āϰিāϤা āĻŦāϞেāύ।

āĻ•িāύ্āϤু āĻ•ুāϰāφāύ āϝিāύি āϞিāĻ–āϏেāύ āϤিāύি āĻ•িāĻ­াāĻŦে āϜাāύāϞেāύ āφāĻ™ুāϞেāϰ āĻ…āĻ—্āϰāĻ­াāĻ— āĻĻি⧟ে

Francis Galton - Wikipedia
Sir Francis Galton , FRS FRAI ( / ˈ ÉĄ ɔː l t ən / ; 16 February 1822 – 17 January 1911), was an English Victorian era polymath : a statistician , sociologist , psychologist , [1] anthropologist , tropical explorer , geographer , inventor , meteorologist , proto- geneticist , psychometrician and a proponent of social Darwinism , eugenics and scientific racism . He was knighted in 1909. Francis Galton Born ( 1822-02-16 ) 16 February 1822 Died 17 January 1911 (1911-01-17) (aged 88) Resting place Claverdon , Warwickshire, England Nationality British Alma mater King's College, London Trinity College, Cambridge Known for Eugenics Behavioural genetics Regression toward the mean Standard deviation Anticyclone Isochrone map Weather map Galton board Galton distribution Galton–Watson process Galton's problem Galton's whistle Awards Royal Geographical Society's Founder's Medal (1853) Royal Medal (1886) Huxley Memorial Medal (1901) Darwin–Wallace Medal (Silver, 1908) Copley Medal (1910) Scientific career Fields Anthropology , Sociology, Psychology , Statistics Institutions Meteorological Council Royal Geographical Society Academic advisors William Hopkins Notable students Karl Pearson Galton produced over 340 papers and books. He also created the statistical concept of correlation and widely promoted regression toward the mean . He was the first to apply statistical methods to the study of human differences and inheritance of intelligence , and introduced the use of questionnaires and surveys for collecting data on human communities, which he needed for genealogical and biographical works and for his anthropometric studies. He was a pioneer of eugenics , coining the term itself in 1883, and also coined the phrase " nature versus nurture ". [2] His book Hereditary Genius (1869) was the first social scientific attempt to study genius and greatness . [3] As an investigator of the human mind, he founded psychometrics (the science of measuring mental faculties) and differential psychology , as well as the lexical hypothesis of personality. He devised a method for classifying fingerprints that proved useful in forensic science . He also conducted research on the power of prayer , concluding it had none due to its null effects on the longevity of those prayed for. [4] His quest for the scientific principles of diverse phenomena extended even to the optimal method for making tea. [5] As the initiator of scientific meteorology , he devised the first weather map , proposed a theory of anticyclones , and was the first to establish a complete record of short-term climatic phenomena on a European scale. [6] He also invented the Galton Whistle for testing differential hearing ability. [7] He was Charles Darwin 's half-cousin. [8] Early life Edit Galton was born at "The Larches", a large house in the Sparkbrook area of Birmingham , England, built on the site of "Fair Hill", the former home of Joseph Priestley , which the botanist William Withering had renamed. He was Charle

Number Miracle in Quran👇

ā§§।āĻ•োāϰāφāύে āϘāύ্āϟা āĻ…āϰ্āĻĨে ‘āϏাāϝ়াāϤ’ āĻļāĻŦ্āĻĻāϟি āĻŦ্āϝāĻŦāĻšৃāϤ āĻšāϝ়েāĻ›ে āĻŽোāϟ ⧍ā§Ē āĻŦাāϰ।

āĻ•োāϰāφāύে ‘āĻĻিāύ’ āĻļāĻŦ্āĻĻāϟি āĻŦ্āϝāĻŦāĻšৃāϤ āĻšāϝ়েāĻ›ে āĻŽোāϟ ā§Šā§Ŧā§Ģ āĻŦাāϰ। (āĻāĻ•āĻŦāϚāύে)

āĻāĻ­াāĻŦে āĻŦāĻšুāĻŦāϚāύে āĻĻিāύ (days) āĻļāĻŦ্āĻĻāϟি āĻāϏেāĻ›ে ā§Šā§Ļ āĻŦাāϰ।

āĻŽাāϏ āĻļāĻŦ্āĻĻāϟি āĻāϏেāĻ›ে ⧧⧍ āĻŦাāϰ।

⧍। āϚাঁāĻĻ āĻļāĻŦ্āĻĻāϟি āĻāϏেāĻ›ে ⧍⧭ āĻŦাāϰ।āĻĒৃāĻĨিāĻŦীāϰ āϚাāϰāĻĻিāĻ•ে āϚাঁāĻĻেāϰ āĻāĻ•āĻŦাāϰ āφāĻŦāϰ্āϤāύে ⧍⧭ āĻĻিāύ āϏāĻŽā§Ÿ āϞাāĻ—ে।āĻāĻ–াāύে āĻ…āύেāĻ•ে āĻŦিāĻ­্āϰাāύ্āϤিāϤে āĻĒāϰāϤে āĻĒাāϰেāύ, āĻĒূāϰ্āĻŖāϚāύ্āĻĻ্āϰেāϰ āϏāĻŽāϝ (⧍⧝.ā§Ģā§Š āĻĻিāύ) āĻāϰ āϏাāĻĨে। āĻāχ āϏāĻŽāϝ়āϟা āϞাāĻ—ে āϚাāĻĻেāϰ āĻāĻ• āĻĒূāϰ্āύিāĻŽা āĻĨেāĻ•ে āφāϰেāĻ• āĻĒুāϰ্āĻŖিāĻŽা āĻĒāϰ্āϝāύ্āϤ āĻĒৌāĻ›āϤে।

ā§Š।āĻļাāϏ্āϤি-ā§§ā§§ā§­ āĻŦাāϰ, āĻ•্āώāĻŽা- ā§¨ā§Šā§Ē (⧍*ā§§ā§§ā§­) āĻŦাāϰ।

āĻĻাāϰিāĻĻ্āϰāϤা- ā§§ā§Š āĻŦাāϰ, āĻĒ্āϰাāϚুāϰ্āϝ- ⧍ā§Ŧ (ā§§ā§Š*⧍) āĻŦাāϰ।

āφāĻļা āĻāĻŦং āĻ­āϝ় āĻļāĻŦ্āĻĻ āĻĻুāϟি āĻāϏেāĻ›ে = ā§Ž āĻŦাāϰ।

āĻ—āϰāĻŽ āĻāĻŦং āĻ াāύ্āĻĄা = ā§Ē āĻŦাāϰ।

āĻĻুāύিāϝ়া āĻāĻŦং āφāĻ–েāϰাāϤ = ā§§ā§§ā§Ģ āĻŦাāϰ।

āĻĒāĻŦিāϤ্āϰ āĻāĻŦং āĻ…āĻĒāĻŦিāϤ্āϰ = ā§­ āĻŦাāϰ।

āωāĻĒāĻ•াāϰ āĻāĻŦং āĻ…āĻĒāĻ•াāϰ = ⧍ā§Ļ āĻŦাāϰ।

āĻ—āύ্āϤāĻŦ্āϝāĻšীāύ āĻāĻŦং āύিāϰ্āĻĻিāώ্āϟ āĻ—āύ্āϤāĻŦ্āϝāϏ্āĻĨāϞ = ā§¨ā§Ž āĻŦাāϰ।

āĻŦিāĻļ্āĻŦাāϏ āĻāĻŦং āĻ…āĻŦিāĻļ্āĻŦাāϏ = ⧍ā§Ģ āĻŦাāϰ।

āϏূāϰ্āϝ āĻāĻŦং āφāϞো = ā§Šā§Š āĻŦাāϰ।

āϏুāĻŦিāϚাāϰ āĻāĻŦং āĻ…āĻŦিāϚাāϰ = ā§§ā§Ģ āĻŦাāϰ।

āϞাāĻ­ āĻāĻŦং āĻ•্āώāϤি = ⧝ āĻŦাāϰ।

āĻ•াāϞু (āϤাāϰা āĻŦāϞāϞো) āĻāĻŦং āĻ•ুāϞ (āϤুāĻŽি āĻŦāϞ) = ā§Šā§Šā§¨ āĻŦাāϰ।

āĻŦীāϜ āĻāĻŦং āϚাāϰা āĻāĻŦং āĻĢāϞ = ā§§ā§Ē āĻŦাāϰ।

āĻ…āĻļ্āϞিāϞāϤা āĻāĻŦং āĻĒāĻĨāĻ­্āϰāώ্āϟ āĻāĻŦং āϏীāĻŽাāϞংāϘāύāĻ•াāϰী = ⧍ā§Ē āĻŦাāϰ। āĻĒাāĻĒ = ā§Ēā§Ž (⧍ā§Ē*⧍) āĻŦাāϰ।

āĻ…āĻĒāĻŦিāϤ্āϰāϤা āĻāĻŦং āύোংāϰাāĻŽী = ā§§ā§Ļ āĻŦাāϰ।

āĻ–োāϞাāĻŽেāϞা āĻāĻŦং āϜāύāϏāĻŽ্āĻŽুāĻ–ে = ā§§ā§Ŧ āĻŦাāϰ।

āĻĢেāϰেāĻļāϤা āĻāĻŦং āĻļāϝ়āϤাāύ = ā§Žā§Ļ āĻŦাāϰ।

āϝাāĻĻু āĻāĻŦং āĻĒ্āϰāϞুāĻŦ্āϧāĻ•াāϰী = ā§Ŧā§Ļ āĻŦাāϰ।

āĻ­াāώা āĻāĻŦং āωāĻĒāĻĻেāĻļ = ⧍ā§Ģ āĻŦাāϰ।

āĻ•্āώāĻŽা āĻāĻŦং āĻĒāĻĨ-āĻĒ্āϰāĻĻāϰ্āĻļāĻ• = ⧭⧝ āĻŦাāϰ।

āύ্āϝাāϝ়āύিāώ্āϟ āĻāĻŦং āĻĒুāϰুāϏ্āĻ•াāϰ = ⧍ā§Ļ āĻŦাāϰ।

āύāĻŦী āĻāĻŦং āϏাāϧাāϰāĻŖ āĻŽাāύুāώ = ā§Šā§Ŧā§Ž āĻŦাāϰ।

āĻ•েāϝ়াāĻŽāϤেāϰ āĻĒ্āϰāĻĨāĻŽ āĻĢুā§ŽāĻ•াāϰ āĻāĻŦং āĻĻ্āĻŦিāϤীāϝ় āĻĢুā§ŽāĻ•াāϰ āĻļāĻŦ্āĻĻ āĻĻুāϟি āĻāϏেāĻ›ে = ā§Ģ āĻŦাāϰ।

āωāύ্āύāϤি (āύাāĻĢ) āĻāĻŦং āĻĻুāϰ্āύীāϤি (āĻĢাāϏাāĻĻ) āĻ িāĻ• ā§Ģā§Ļ āĻŦাāϰ āĻ•āϰে āφāĻ›ে।

ā§Ē।āĻŽাāύুāώ āĻļāĻŦ্āĻĻāϟি āĻāϏেāĻ›ে ā§Ŧā§Ģ āĻŦাāϰ। āĻŽাāύুāώ = ( āĻŽাāϟি- ā§§ā§­ āĻŦাāϰ + āĻŦীāϰ্āϝ āĻĢোāϟা- ⧧⧍ āĻŦাāϰ + āĻ­্āϰুāύ- ā§Ŧ āĻŦাāϰ + āĻŽাংāϏāĻĒিāύ্āĻĄ- ā§Š āĻŦাāϰ + āĻšা⧜- ā§§ā§Ģ āĻŦাāϰ + āĻŽাংāϏ- ⧧⧍ āĻŦাāϰ) = ā§Ŧā§Ģ। āĻ…āϰ্āĻĨাā§Ž āĻŽাāύুāώ āϤৈāϰীāϰ āĻŦিāĻ­িāύ্āύ āωāĻĒাāĻĻাāύāĻ—ুāϞো āĻ•োāϰāφāύে āϝāϤāĻŦাāϰ āĻ•āϰে āĻāϏেāĻ›ে āĻāχ āϰিāĻĒিāϟেāϏāύেāϰ(Repetition)āϏংāĻ–্āϝাāϰ āϝোāĻ—āĻĢāϞ āφāϰ āĻŽাāύুāώ āĻļāĻŦ্āĻĻāϟিāϰ āĻļāĻŦ্āĻĻāϟাāϰ āϰিāĻĒিāϟেāϏāύেāϰ(Repetition) āϏāĻŽাāύ(āĻŽাāύুāώ=āĻŽাāϟি+āĻŦীāϰ্āϝāĻĢোāϟা+āĻ­্āϰুāύ+āĻŽাংāϏāĻĒিāύ্āĻĄ+āĻšা⧜+āĻŽাংāϏ)

ā§Ģ। āϝাāϰা āφāĻŽাāϰ āϏুāϏ্āĻĒāώ্āϟ āφāϝ়াāϤāϏāĻŽূāĻš āĻ…āϏ্āĻŦীāĻ•াāϰ āĻ•āϰে āϤাāĻĻেāϰ āωāĻĻাāĻšāϰāĻŖ āĻšāϚ্āĻ›ে āĻ•ুāĻ•ুāϰেāϰ āĻŽāϤ”। (āϏূāϰা āφāϰাāĻĢ) āϝাāϰা āφāĻŽাāϰ āϏুāϏ্āĻĒāώ্āϟ āφāϝ়াāϤ āϏāĻŽূāĻš āĻ…āϏ্āĻŦীāĻ•াāϰ āĻ•āϰে āĻŦাāĻ•্āϝāϟি āĻ•োāϰāφāύে āĻāϏেāĻ›ে ā§Ģ āĻŦাāϰ। āφāĻŦাāϰ āĻ•ুāĻ•ুāϰ āĻļāĻŦ্āĻĻāϟিāĻ“ āĻ•োāϰāφāύে āĻāϏেāĻ›ে ā§Ģ āĻŦাāϰ।

ā§Ŧ।āĻ•োāύ āĻ•াāϜ āĻ•āϰāϞে āϏেāχ āĻ•াāϜেāϰ āĻ…āĻŦāĻļ্āϝāĻŽ্āĻ­াāĻŦী āĻĢāϞাāĻĢāϞ āϏāĻŽ্āĻĒāϰ্āĻ•িāϤ āϰিāĻĒিāϟেāĻļāύ āϏāĻŽাāύ āϏংāĻ–্āϝাāϝ় āĻāϏেāĻ›ে āĻ•োāϰāφāύে।1. āϝাāĻ•াāϤ āĻĻিāϞে āĻŦāϰāĻ•āϤ āφāϏে। āϤাāχ āϝাāĻ•াāϤ āĻ“ āĻŦāϰāĻ•āϤ āĻļāĻŦ্āĻĻ āĻĻুāϟি āĻāϏেāĻ›ে ā§Šā§¨ āĻŦাāϰ āĻ•āϰে।
2. āĻŽাāύুāώ āϏৃāώ্āϟিāϰ āωāĻĻ্āĻĻেāĻļ্āϝ āĻšāϞো āφāϞ্āϞাāĻšāϰ āχāĻŦাāĻĻ āĻ•āϰা। āϤাāχ “āĻŽাāύুāώ āϏৃāώ্āϟি” āĻ“ “āχāĻŦাāĻĻāϤ” āĻļāĻŦ্āĻĻ āĻĻুāϟি āĻāϏেāĻ›ে ā§§ā§Ŧ āĻŦাāϰ āĻ•āϰে।
3. āĻ—োāϞাāĻŽেāϰ āĻ•াāϜ āĻšāϞো āĻ—োāϞাāĻŽী āĻ•āϰা। āĻ—োāϞাāĻŽ āĻ“ āĻ—োāϞাāĻŽী āĻļāĻŦ্āĻĻ āĻĻুāϟি āĻāϏেāĻ›ে ā§§ā§Ģ⧍ āĻŦাāϰ āĻ•āϰে।
4. āύেāĻļা āĻ•āϰāϞে āĻŽাāϤাāϞ āĻšāϝ়। “āύেāĻļা” āĻ“ “āĻŽাāϤাāϞ” āĻļāĻŦ্āĻĻ āĻĻুāϟি āĻāϏেāĻ›ে ā§Ŧ āĻŦাāϰ āĻ•āϰে।
5. āĻšাāϝ়াāϤ āϞাāĻ­ āĻ•āϰāϞে āĻŽāωāϤ āĻšāĻŦেāχ। āϤাāχ āĻšাāϝ়াāϤ āĻ“ āĻŽāωāϤ āĻļāĻŦ্āĻĻ āĻĻুāϟি āĻāϏেāĻ›ে āĻŽোāϟ ā§§ā§Ŧ āĻŦাāϰ āĻ•āϰে।
6. āĻŽাāύুāώ āĻšেāĻĻাāϝ়েāϤ āĻĒেāϞে āϤাāϰ āωāĻĒāϰ āϰāĻšāĻŽāϤ āĻŦāϰ্āώিāϤ āĻšāϝ়। āĻšেāĻĻাāϝ়েāϤ āĻ“ āϰāĻšāĻŽāϤ āĻļāĻŦ্āĻĻ āĻĻুāϟি āĻāϏেāĻ›ে āĻŽোāϟ ⧭⧝ āĻŦাāϰ āĻ•āϰে।
7. āĻ•াāϜ āĻ•āϰāϞে āĻ•াāϜেāϰ āĻĢāϞাāĻĢāϞ āĻšāĻŦে। āĻ•াāϜ – ā§§ā§Ļā§Ž āĻŦাāϰ āĻĢāϞাāĻĢāϞ ā§§ā§Ļā§Ž āĻŦাāϰ।

ā§­।āĻŦāϰ্āϤāĻŽাāύ āĻŦিāϜ্āĻžাāύ āύিāϰীāĻ•্āώāύেāϰ āĻŽাāϧ্āϝāĻŽে āĻĻেāĻ–িāϝ়েāĻ›ে āĻĒৃāĻĨিāĻŦীāϤে āϏ্āĻĨāϞāĻ­াāĻ—েāϰ āĻŽোāϟ āφāϝ়āϤāύেāϰ ⧍⧝ āĻ­াāĻ— āφāϰ āϜāϞāĻ­াāĻ—েāϰ āĻĒāϰিāĻŽাāύ ā§­ā§§ āĻ­াāĻ— āĻĒ্āϰাāϝ়। āϚāϞুāύ āĻĻেāĻ–ি āĻ•োāϰāφāύ āĻ•ি āĻŦāϞে- āĻ•োāϰāφāύে āϏāĻŽুāĻĻ্āϰ āĻŦা āϜāϞাāϧাāϰ āĻļāĻŦ্āĻĻāϟি āĻāϏেāĻ›ে ā§Šā§¨ āĻŦাāϰ। āĻ­ুāĻŽি āĻŦা āϜāĻŽি āĻļāĻŦ্āĻĻāϟি āĻāϏেāĻ›ে ā§§ā§Š āĻŦাāϰ। āĻāĻĻেāϰ āϰিāĻĒিāϟেāĻļāύ(repetition) āĻāϰ āĻĒāϰিāĻŽাāύāĻ•ে āĻ…āύুāĻĒাāϤে āĻĒ্āϰāĻ•াāĻļ āĻ•āϰāϞে āĻĒাāĻ“āϝ়া āϝাāϝ় -

āϏ্āĻĨāϞāĻ­াāĻ—েāϰ āĻĒāϰিāĻŽাāĻŖ = (ā§§ā§Š/(ā§§ā§Š+ā§Šā§¨)*ā§§ā§Ļā§Ļ%=ā§¨ā§Ž.ā§Žā§Žā§Ž%
āϜāϞāĻ­াāĻ—েāϰ āĻĒāϰিāĻŽাāύ = (ā§Šā§¨/(ā§§ā§Š+ā§Šā§¨)*ā§§ā§Ļā§Ļ%=ā§­ā§§.ā§§ā§§ā§§%

ā§Ž। āφāϏāĻšাāĻŦে āĻ•াāĻšাāĻĢ āĻŦা āĻ—ুāĻšাāϰ āĻ…āϧিāĻŦাāϏিāĻĻেāϰ āĻŦāϰ্āĻŖāύা āĻĨেāĻ•ে āϜাāύা āϝাāϝ় āĻ“āϰা āĻ—ুāĻšাāϰ āĻ­িāϤāϰ ā§Šā§Ļ⧝ āĻŦāĻ›āϰ āϘুāĻŽāύ্āϤ āĻ›িāϞ। āĻāχ āĻ—ুāĻšাāϰ āĻ…āϧিāĻŦাāϏিāĻĻেāϰ āĻŦāϰ্āĻŖāύা āφāĻ›ে, āĻ•োāϰāφāύেāϰ āϏূāϰা āĻ•াāĻšাāĻĢেāϰ ⧝ āĻĨেāĻ•ে ⧍ā§Ģ āύং āφāϝ়াāϤে। āĻāχ āφāϝ়াāϤ āĻ•āϝ়āϟিāϰ āĻŽোāϟ āĻļāĻŦ্āĻĻেāϰ āϏংāĻ–্āϝা āĻ—āĻŖāύা āĻ•āϰুāύ ā§Šā§Ļ⧝ āϟি āĻļāĻŦ্āĻĻ āĻĒাāĻŦেāύ!

⧝।āĻ•োāϰāφāύ āĻ…āύেāĻ• āϜাāϝ়āĻ—াāϝ় āϤুāϞāύা āĻ•āϰāϤে āĻĻেāĻ–া āϝাāϝ়। āĻāĻ•্āώেāϤ্āϰে āϝে āĻĻুāϟি āĻļāĻŦ্āĻĻেāϰ āĻŽাāĻে āϤুāϞāύা āĻ•āϰা āĻšāϝ়েāĻ›ে āϐ āĻĻুāϟি āĻļāĻŦ্āĻĻ āĻ•োāϰāφāύে āϏāĻŽāĻĒāϰিāĻŽাāύ āϏংāĻ–্āϝাāϝ় āĻāϏেāĻ›ে।āϝেāĻŽāύ-

“āφāϞ্āϞাāĻš āϤাāϝ়াāϞাāϰ āĻ•াāĻ›ে āψāϏাāϰ āϤুāϞāύা āĻšāϚ্āĻ›ে āφāĻĻāĻŽāϰে āĻŽāϤ”। (āφāϞ-āχāĻŽāϰাāύ : ā§Ģ⧝)।āφāĻĻāĻŽ(āφ) āĻ“ āψāϏা(āφ) ⧍ā§Ģ āĻŦাāϰ āϏংāĻ–্āϝāĻ•āĻŦাāϰ āĻ•ুāϰāφāύে āĻāϏেāĻ›ে।

āύাāϰী āĻ“ āĻĒুāϰুāώ āωāϭ⧟āχ ⧍⧭ āĻŦাāϰ āĻ•ুāϰāφāύে āĻāϏেāĻ›ে।(Feminism)

āĻāĻ–াāύে āφāϰো āĻŦিāϏ্āϤাāϰিāϤ āĻĒাāĻŦেāĻ¨đŸ‘‡

āĻĒāĻŦিāϤ্āϰ āĻ•ুāϰāφāύেāϰ āĻļāĻŦ্āĻĻāϏāĻŽূāĻšেāϰ āϏংāĻ–্āϝাāĻ—āϤ āĻĒāϰিāϏংāĻ–্āϝাāύ āĻĒাāĻ“ā§Ÿা āϝাāĻŦে āĻ•োāĻĨা⧟? āĻ Hasan Banna āĻāϰ āωāϤ্āϤāϰ

āĻ•ুāϰāφāύ āĻ…āĻŦāϤীāϰ্āĻŖ āĻšāĻ“ā§Ÿাāϰ āĻŽাāĻে āϝāĻĻি āĻŽāĻšাāύāĻŦী(āϏ) āĻŽাāϰা āϝেāϤো āϤাāĻšāϞে āĻāχ āĻļāĻŦ্āĻĻেāϰ āĻ­াāϰāϏাāĻŽ্āϝ āĻ­েāĻ™ে āϝেāϤো।

āĻāĻ•āϜāύ āύিāϰāĻ•্āώāϰ āĻāĻ­াāĻŦে āĻļāĻŦ্āĻĻ āĻ—ুāĻŖে āĻ—ুāĻŖে āĻ•āĻŦিāϤাāϰ āĻ­াāώা⧟ āĻāĻ•āϟা āĻ—্āϰāύ্āĻĨ āϞিāĻ–āĻŦে āϝাāϤে āĻ¤ā§ŽāĻ•াāϞীāύ āϏāĻŽā§Ÿেāϰ āϚে⧟ে āĻŦāĻšু āĻ…āĻ—্āϰāϏāϰ āĻŦিāϜ্āĻžাāύ āĻĨাāĻ•āĻŦে āĻāϟা āĻ•ি āϏāĻŽ্āĻ­āĻŦ?

āϰেāĻĢাāϰেāύ্āϏঃ Don’t Trust me Bro!

Mathematical Miracles of Quran
The inceridible balance of numbers