✦ LIBER ✦

Unified approach to structure factors and neutrino processes in nucleon matter

✍ Scribed by Lykasov, G. I.; Pethick, C. J.; Schwenk, A.

Book ID: 121681821
Publisher: The American Physical Society
Year: 2008
Tongue: English
Weight: 378 KB
Volume: 78
Category: Article
ISSN: 0556-2813
DOI: 10.1103/physrevc.78.045803

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

Unified approach for nucleon knock-out a

Unified approach for nucleon knock-out and coherent and incoherent pion production in neutrino interactions with nuclei

✍ Martini, M.; Ericson, M.; Chanfray, G.; Marteau, J. 📂 Article 📅 2009 🏛 The American Physical Society 🌐 English ⚖ 857 KB

Nucleon contribution to the induced char

Nucleon contribution to the induced charge of neutrinos in a matter background and a magnetic field

✍ Nieves, José F. 📂 Article 📅 2004 🏛 The American Physical Society 🌐 English ⚖ 159 KB

Unified Approach to Ion Transport and St

Unified Approach to Ion Transport and Structural Relaxation in Amorphous Polymers and Glasses

✍ Ingram, Malcolm D.; Imrie, Corrie T.; Ledru, Jacques; Hutchinson, John M. 📂 Article 📅 2008 🏛 American Chemical Society 🌐 English ⚖ 117 KB

On the absence of form factor in e2 corr

On the absence of form factor in e2 corrections to the amplitudes of neutrino and electron scattering on nucleons

✍ B.L. Ioffe; V.V. Sokolov 📂 Article 📅 1971 🏛 Elsevier Science 🌐 English ⚖ 218 KB

Statistical mechanical approach to secon

Statistical mechanical approach to secondary processes and structural relaxation in glasses and glass formers

✍ A. Crisanti; L. Leuzzi; M. Paoluzzi 📂 Article 📅 2011 🏛 Springer-Verlag 🌐 English ⚖ 774 KB

An analytic approach to the connection b

An analytic approach to the connection between stellar structure parameters and the neutrino emission rate in a simple stellar model

✍ H. J. Haubold; A. M. Mathai 📂 Article 📅 1986 🏛 John Wiley and Sons 🌐 English ⚖ 511 KB

In order to obtain the internal structurc of a main-sequence star such as the Suqusually one has to solve the detailed structure equations numerically. This paper is an attempt to construct analytic models for the stellar nuclear energy generation. We give closed-form analytic results for the stella