Gravitational Radiation from Primordial Helical Inverse Cascade MHD Turbulence

التفاصيل البيبلوغرافية
العنوان: Gravitational Radiation from Primordial Helical Inverse Cascade MHD Turbulence
المؤلفون: Kahniashvili, Tina, Campanelli, Leonardo, Gogoberidze, Grigol, Maravin, Yurii, Ratra, Bharat
المصدر: Phys.Rev.D78:123006,2008; Erratum-ibid.D79:109901,2009
سنة النشر: 2008
المجموعة: Astrophysics
مصطلحات موضوعية: Astrophysics
الوصف: We consider the generation of gravitational waves by primordial helical inverse cascade magnetohydrodynamic (MHD) turbulence produced by bubble collisions at the electroweak phase transition. We extend the previous study \cite{kgr08} by considering both currently discussed models of MHD turbulence. For popular electroweak phase transition parameter values, the generated gravitational wave spectrum is only weakly dependent on the MHD turbulence model. Compared to the unmagnetized electroweak phase transition case, the spectrum of MHD-turbulence-generated gravitational waves peaks at lower frequency with larger amplitude and can be detected by the proposed Laser Interferometer Space Antenna
Comment: 13 pages, 4 figures; typos corrected
نوع الوثيقة: Working Paper
DOI: 10.1103/PhysRevD.78.123006
DOI: 10.1103/PhysRevD.79.109901
URL الوصول: http://arxiv.org/abs/0809.1899
رقم الأكسشن: edsarx.0809.1899
قاعدة البيانات: arXiv
الوصف
DOI:10.1103/PhysRevD.78.123006