Electroweak epoch
In physical cosmology, the electroweak epoch was the period in the evolution of the early universe when the temperature of the universe had fallen enough that the strong force separated from the electroweak interaction, but was high enough for electromagnetism and the weak interaction to remain merged into a single electroweak interaction above the critical temperature for electroweak symmetry breaking (159.5±1.5 GeVin the Standard Model of particle physics). Some cosmologists place the electroweak epoch at the start of the inflationary epoch, approximately 10−36 seconds after the Big Bang. Others place it at approximately 10−32 seconds after the Big Bang when the potential energy of the inflaton field that had driven the inflation of the universe during the inflationary epoch was released
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Electroweak epoch
In physical cosmology, the electroweak epoch was the period in the evolution of the early universe when the temperature of the universe had fallen enough that the strong force separated from the electroweak interaction, but was high enough for electromagnetism and the weak interaction to remain merged into a single electroweak interaction above the critical temperature for electroweak symmetry breaking (159.5±1.5 GeVin the Standard Model of particle physics). Some cosmologists place the electroweak epoch at the start of the inflationary epoch, approximately 10−36 seconds after the Big Bang. Others place it at approximately 10−32 seconds after the Big Bang when the potential energy of the inflaton field that had driven the inflation of the universe during the inflationary epoch was released
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A Era eletro-fraca foi uma era ...... so era composto por quarks e .
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En cosmologia física, l'època ...... ons de la teoria electrofeble.
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En cosmologie et en physique d ...... ron 10−36 s après le Big Bang.
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En cosmología física, la época ...... ad) adicional.[cita requerida]
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In physical cosmology, the ele ...... uire additional CP violation).
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Ve fyzikální kosmologii byla e ...... orie elektroslabých interakcí.
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В физической космологии электр ...... тренным электрослабой теорией.
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У фізичній космології електрос ...... аченим електрослабкою теорією.
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حقبة الكهروضعيفة (بالإنجليزية: ...... يضًا خرق تناظر الشحنة السوية).
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電弱時代(Electroweak epoch)は、初期宇宙の ...... 証され、また電弱理論による別の予測も実験的に検証されている。
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A Era eletro-fraca foi uma era ...... so era composto por quarks e .
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En cosmologia física, l'època ...... n prou energètiques per crear
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En cosmologie et en physique d ...... ron 10−36 s après le Big Bang.
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En cosmología física, la época ...... ía conducido la inflación cósm
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In physical cosmology, the ele ...... nflationary epoch was released
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Ve fyzikální kosmologii byla e ...... tím jak se vesmír plnil hustý
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В физической космологии электр ...... зон Хиггса и W-бозон, Z-бозон.
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У фізичній космології електрос ...... татньо енергетичною, щоб створ
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حقبة الكهروضعيفة (بالإنجليزية: ...... لازما كوارك-غلوون كثيفة ساخنة.
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電弱時代(Electroweak epoch)は、初期宇宙の ...... 証され、また電弱理論による別の予測も実験的に検証されている。
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Electroweak epoch
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Elektroslabá éra
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Era Eletrofraca
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Època electrofeble
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Ère électrofaible
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Época electrodébil
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Електрослабка епоха
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Электрослабая эпоха
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حقبة الكهروضعيفة
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電弱時代
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