Bremsstrahlung neutrino energy loss for 24Mg, 28Si, 32S, 40Ca, 56Fe in strong electron screening

LIU Jing-Jing

doi:10.1088/1674-1137/34/2/003

Chinese Physics C> 2010, Vol. 34> Issue(2) : 171-176 DOI: 10.1088/1674-1137/34/2/003

Bremsstrahlung neutrino energy loss for ²⁴Mg, ²⁸Si, ³²S, ⁴⁰Ca, ⁵⁶Fe in strong electron screening

LIU Jing-Jing ^,

Department of Physics, University of Qiongzhou, Sanya 572022, China

Abstract
HTML
Reference
Related

PDF

Abstract：
Based on Weinberg-Salam theory the bremsstrahlung neutrino energy loss for nuclei ²⁴Mg, ²⁸Si, ³²S, ⁴⁰Ca and ⁵⁶Fe are investigated in strong electron screening. Our results are compared with those of Dicus' and show that the latter are higher by 2 orders of magnitude in the density-temperature region of 10⁸ g/cm³≤ρ/μ_e≤10¹¹ g/cm³ and 2.5≤T₉≤4.5. On the other hand, the factor C shows that the maximum differences are 99.16%, 99.13%, 99.12%, 99.055%, 99.040% corresponding to the nuclei ²⁴Mg, ²⁸Si, ³²S, ⁴⁰Ca and ⁵⁶Fe.

References

[1]

. Gamow G, Schonberg M. Phys. Rev., 1941, 59: 5392. LIU J J, LUO Z Q., LIU H L, LAI X J. International Jour-nal of Modern Physics A, 2007, 22: 33053. LIU J J, LUO Z Q. Chinese Physics, 2007, 16: 36244. LIU J J, LUO Z Q. Chinese Physics C, 2008, 32: 1085. LIU J J, LUO Z Q. China Phys. Lett., 2007, 24: 18616. LIU J J. Chinese Physics C, 2009, 33: 157. Beaudet G, Petrosian V, Salpeter E E. Astrophys. J., 1967,150: 9798. Feynman R P, Gell-Mann M. Phys. Rev., 1958, 109: 1939. Weinberg S. Phys. Rev. Lett., 1967, 19: 126410. Dicus D A. Phys. Rev. D, 1972, 6: 94111. Flowers E. Astrophys. J., 1973, 180: 91112. Haensel P, Kaminker A D, Yakovlev D G. Astron. Astro-phys., 1996, 314: 32813. Itoh N, Adachi T, Nakagawa M, Kohyama Y, Munakata H.Astrophys. J., 1989, 339: 35414. Itoh N, Hayashi H, Nishikawa A, Kohyama Y. Astrophys.J., 1996, 102: 41115. Dicus D A, Kolb E W, Schramm D N, Tubbs D L. Astro-phys. J., 1976, 210: 481

[1]	LÜ Li-Jun , BAI Hong-Bo , ZHANG Jin-Fu , DONG Hong-Fei . Mixed symmetry states and electromagnetic transition in the N=Z nucleus ²⁸Si. Chinese Physics C, 2014, 38(10): 104102. doi: 10.1088/1674-1137/38/10/104102
[2]	LIU Jing-Jing . Electron capture of nuclides ^{52,53,54, 55, 56}Fe in magnetars. Chinese Physics C, 2013, 37(8): 085101. doi: 10.1088/1674-1137/37/8/085101
[3]	LIU Jing-Jing , KANG Xiao-Ping , HE Zhong , Huai-Ren , SHI Huan-Yu , HUANG Hong-Chao , ZHONG Shan , FENG Hao , LI Chang-Wei . Gaussian modification of neutrino energy loss on strongly screening nuclides ⁵⁵Co and ⁵⁶Ni by electron capture in stellar interior. Chinese Physics C, 2011, 35(3): 243-247. doi: 10.1088/1674-1137/35/3/006
[4]	LIU Jing-Jing . Beta decay of nuclide ⁵⁶Fe, ⁵⁶Co, ⁵⁶Ni, ⁵⁶Mn, ⁵⁶Cr and ⁵⁶V due to strong electron screening in stellar interiors. Chinese Physics C, 2010, 34(11): 1700-1703. doi: 10.1088/1674-1137/34/11/006
[5]	Khudair Falih , ZHANG Jin-Fu , BAI Hong-Bo . Mixed symmetry states and isospin excitation in the N=Z nucleus ²⁸Si. Chinese Physics C, 2009, 33(S1): 46-48. doi: 10.1088/1674-1137/33/S1/015
[6]	LIU Jing-Jing , LUO Zhi-Quan . Neutrino energy loss by electron capture in magnetic field at the crusts of neutron stars. Chinese Physics C, 2008, 32(2): 108-111. doi: 10.1088/1674-1137/32/2/007
[7]	LÜ Li-Jun , BAI Hong-Bo , ZHANG Jin-Fu . Isospin and mixed symmetry structure in ²⁴Mg. Chinese Physics C, 2008, 32(3): 177-181. doi: 10.1088/1674-1137/32/3/003
[8]	LIU Jing-Jing , LUO Zhi-Quan . Pair neutrino energy loss for nuclei ⁵⁶Fe at the late stages of stellar evolution. Chinese Physics C, 2008, 32(8): 617-619. doi: 10.1088/1674-1137/32/8/005
[9]	SU Dan-Dan , ZENG Guo-Mo . α-Particle Cluster Structure and π-²⁴Mg,π-32S Elastic Scattering. Chinese Physics C, 2006, 30(S2): 124-126.
[10]	Di Yaomin , Lu Huaping . Correction of ²⁴Mg Collective States With Three-Body Non-diagonal Boson Interaction. Chinese Physics C, 1999, 23(6): 546-551.
[11]	Zhang Zhanjun , Shi Zhuyi , Liu Yong , Sang Jianping . Microscopic Foundation of sdgIBM-2 and Study of Low-Lying States of ²⁴Mg. Chinese Physics C, 1998, 22(2): 169-175.
[12]	An Zhu . Microscopic Analysis of Proton Scattering from ²⁸Si at 22MeV. Chinese Physics C, 1995, 19(10): 873-878.
[13]	JING Guiru , REN Guoxiao . Angular Distributions of Projectile Fragments Produced in Collisions of 200A GeV ³²S Beam with Cu. Chinese Physics C, 1993, 17(11): 976-978.
[14]	Zheng Jiwen , Zheng Pingzi , Liu Guoxing , Chen Keliang , Wang Sufang , Bai Xingping , Yu Xian , Zhang Huanqiao , Xu Jincheng , Liu Zuhua , Ruan Ming , Lu Jun , Xu Kan . Measurement of Complete Fusion Excitation Function of ¹⁶O + ²⁸Si Reaction. Chinese Physics C, 1992, 16(S3): 227-234.
[15]	Dou Zhiguo , Jing Xiaogong , Zhao Guoquan . Single-Particle and Single Hole Energies in the ⁴⁰Ca Region. Chinese Physics C, 1991, 15(S1): 85-92.
[16]	LING You-Guang , QIU Zhi-Hong . BOUND STATES OF ETA-²⁴Mg AND ETA-³²S. Chinese Physics C, 1989, 13(11): 1017-1022.
[17]	SHEN Qing-Biao , TIAN Ye , LIU Rui-Zhe . CALCULATIONS OF NUCLEON DENSITIES, KINETIC ENERGY DENSITIES, SPIN DENSITIES AND CHARGE DENSITY WITH SHELL MODEL FOR ⁴⁰Ca. Chinese Physics C, 1983, 7(4): 473-480.
[18]	YUAN JIAN , YUAN RONG-FANG , HUANG BING-YIN , WANG XIN-LIN , WANG YUAN-DA , ZHUANG FEI , JIANG SI-YUAN . STUDY OF ANOMALOUS LARGE ANGLE α-SCATTERING ON ²⁴Mg. Chinese Physics C, 1982, 6(3): 355-364.
[19]	Zhao Shu-ping . CALCULATION OF THE ELASTIC-SCATTERING CROSS-SECTION OF ENERGETIC ELECTRON BY ⁴⁰Ca NUCLEUS IN CONSIDERATION OF THE INFLUENCE OF“PION CONDENSATION”. Chinese Physics C, 1980, 4(5): 569-575.
[20]	LI CHI-CHOU , LU HAN-LIN , FAN PEI-KUO , MA HUNG-CHANG , LI YEH-SHA . CROSS SECTION MEASUREMENT FOR THE REACTION ⁵⁶Fe（n,p）⁵⁶Mn. Chinese Physics C, 1978, 2(6): 550-557.

Access

Get Citation

LIU Jing-Jing. Bremsstrahlung neutrino energy loss for ²⁴Mg, ²⁸Si, ³²S, ⁴⁰Ca, ⁵⁶Fe in strong electron screening[J]. Chinese Physics C, 2010, 34(2): 171-176. doi: 10.1088/1674-1137/34/2/003

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

Received: 2008-12-26
Revised: 2009-06-22

Article Metric

Article Views(2740)
PDF Downloads(834)
Cited by(0)

Policy on re-use

To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.

通讯作者: 陈斌, bchen63@163.com

1.
沈阳化工大学材料科学与工程学院沈阳 110142

Bremsstrahlung neutrino energy loss for ²⁴Mg, ²⁸Si, ³²S, ⁴⁰Ca, ⁵⁶Fe in strong electron screening

Corresponding author: LIU Jing-Jing,

Department of Physics, University of Qiongzhou, Sanya 572022, China

Received Date: 2008-12-26

Accepted Date: 2009-06-22

Available Online: 2010-02-05

Abstract:

Based on Weinberg-Salam theory the bremsstrahlung neutrino energy loss for nuclei ²⁴Mg, ²⁸Si, ³²S, ⁴⁰Ca and ⁵⁶Fe are investigated in strong electron screening. Our results are compared with those of Dicus' and show that the latter are higher by 2 orders of magnitude in the density-temperature region of 10⁸ g/cm³≤ρ/μ_e≤10¹¹ g/cm³ and 2.5≤T₉≤4.5. On the other hand, the factor C shows that the maximum differences are 99.16%, 99.13%, 99.12%, 99.055%, 99.040% corresponding to the nuclei ²⁴Mg, ²⁸Si, ³²S, ⁴⁰Ca and ⁵⁶Fe.

HTML

Reference (1)

Bremsstrahlung neutrino energy loss for ²⁴Mg, ²⁸Si, ³²S, ⁴⁰Ca, ⁵⁶Fe in strong electron screening

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article

Bremsstrahlung neutrino energy loss for ²⁴Mg, ²⁸Si, ³²S, ⁴⁰Ca, ⁵⁶Fe in strong electron screening

Corresponding author: LIU Jing-Jing,

HTML

目录