Pair neutrino energy loss for nuclei <SUP>56</SUP>Fe at the late stages of stellar evolution

LIU Jing-Jing; LUO Zhi-Quan

doi:10.1088/1674-1137/32/8/005

Chinese Physics C> 2008, Vol. 32> Issue(8) : 617-619 DOI: 10.1088/1674-1137/32/8/005

Pair neutrino energy loss for nuclei ⁵⁶Fe at the late stages of stellar evolution

LIU Jing-Jing ^, ,
LUO Zhi-Quan

Abstract
HTML
Reference
Related

PDF

Abstract：
Based on the Weinberg-Salam theory, the pair neutrino energy loss rates for nuclei ⁵⁶Fe are canvassed for the wide range of density and temperature. The results of ours (Q_LJ) are compared with those of Beaudet G, Petrosian V and Salpeter E. E's (Q_BPS), and it shows that the pair neutrino energy loss rates of Q_BPS are always larger than Q_LJ .The Q_BPS is 12.57%, 12.86%, 14.99%, 19.80% times higher than Q_LJ corresponding to the temperature T₉=0.385, 1.0, 5.0, 10, respectively.

References

[1]

. Weinberg S. Phys. Rev. Lett., 1967, 19: 12642. Salam A. In Elementary Particle Physics. Ed. SvartholmN. Stockholm: Almqvist and Wiksells. 1968, 3673. Dicus D A. Phys. Rev. D, 1972, 6: 9414. Pinave Soviet V. S. Phys-J.E.T.P, 1964, 18: 3775. Beaudet G, Petrosian V, Salpeter E E. Astrophys. J., 1967,150: 9796. Munakata H, Kohyama Y, Itoh N. Astrophys. J., 1985, 296:1977. Itoh N, Adachi T, Nakagawa M et al. Astrophys. J., 1989,339: 3548. Itoh N, Hayashi H, Nishikawa A et al. Astrophys. J., 1996,102: 4119. Esposito S, Mangano G, Miele G et al. Nucl. Phys. B, 2003,658: 21710. LIU J J, LUO Z Q. Chinese Physics Lett., 2007, 7: 1861

[1]	Cui Zhu , Xia Zhou , Na Wang . Rotational energy conversion and thermal evolution of neutron stars. Chinese Physics C, 2017, 41(12): 125104. doi: 10.1088/1674-1137/41/12/125104
[2]	Li-Hua Song , Lin-Wan Yan , Chun-Gui Duan . Energy loss effect of incoming gluons from J/ψ production in p-A collisions. Chinese Physics C, 2017, 41(2): 023102. doi: 10.1088/1674-1137/41/2/023102
[3]	E. Ya. Paryev , M. Hartmann , Yu. T. Kiselev . Medium effects in ΛK⁺ pair production by 2.83 GeV protons on nuclei. Chinese Physics C, 2017, 41(12): 124108. doi: 10.1088/1674-1137/41/12/124108
[4]	Lianrong Dai , Feng Pan , J. P. Draayer . A nucleon-pair and boson coexistent description of nuclei. Chinese Physics C, 2017, 41(7): 074103. doi: 10.1088/1674-1137/41/7/074103
[5]	LI Rong-Hua , LI Zhan-Kui , YANG Lei , LI Dong-Mei , LI Hai-Xia , WANG Zhu-Sheng , CHEN Cui-Hong , TAN Ji-Lian , LIU Feng-Qiong , RONG Xin-Juan , WANG Xiu-Hua , LI Chun-Yan , ZU Kai-Ling , LU Zi-Wei . Phonon contribution to nonionizing energy loss in silicon detectors. Chinese Physics C, 2015, 39(6): 066004. doi: 10.1088/1674-1137/39/6/066004
[6]	LI Yan-Jing , ZHANG Dong-Hai , YAN Shi-Wei , WANG Li-Chun , CHENG Jin-Xia , LI Jun-Sheng . Projectile fragment emission in the fragmentation of ⁵⁶Fe on C, Al and CH₂ targets at 471 A MeV. Chinese Physics C, 2014, 38(1): 014001. doi: 10.1088/1674-1137/38/1/014001
[7]	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
[8]	HOU Pei-You , SUN Xiao-Jun , YU Cheng-Gang , LU Xiao . Theoretical analysis of double-differential neutron emission cross sections for n+⁵⁶Fe reactions at incident energies of 7-13 MeV. Chinese Physics C, 2011, 35(1): 35-39. doi: 10.1088/1674-1137/35/1/008
[9]	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
[10]	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
[11]	LIU Jing-Jing . Bremsstrahlung neutrino energy loss for ²⁴Mg, ²⁸Si, ³²S, ⁴⁰Ca, ⁵⁶Fe in strong electron screening. Chinese Physics C, 2010, 34(2): 171-176. doi: 10.1088/1674-1137/34/2/003
[12]	LIU Jing-Jing . Plasma neutrino energy loss due to the axial-vector current at the late stages of stellar evolution. Chinese Physics C, 2009, 33(10): 834-837. doi: 10.1088/1674-1137/33/10/003
[13]	LIU Jing-Jing . The competition of neutrino energy loss due to the pair, photo-, plasma process at the late stages of stellar evolution. Chinese Physics C, 2009, 33(1): 15-19. doi: 10.1088/1674-1137/33/1/004
[14]	SHEN Shui-Fa , HUANG Ya-Wei , ZHENG Shi-Jie , XU Fu-Rong . Rotational to vibrational evolution in some rotational-like nuclei. Chinese Physics C, 2008, 32(S2): 146-149.
[15]	, , , , , , , . Energy loss correction for a crystal calorimeter. Chinese Physics C, 2008, 32(4): 269-274. doi: 10.1088/1674-1137/32/4/006
[16]	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
[17]	Yuan Jian , Lu Ming , Lu Daoru , Chen Quan , Sun Zuxun . Study of Stretched States Populated by ^56,57Fe,⁵⁹Co(α,d)^58,59Co,⁶¹Ni Reactions. Chinese Physics C, 1996, 20(1): 32-37.
[18]	Gao Yonghua , He Zhenmin , Huang Ruiwang , Peng Hong'an . The Influence of Nuclear Target on “Small” Mass Lepton Pair Production of High Energy Hadron-Nuclei Collision. Chinese Physics C, 1992, 16(S3): 281-289.
[19]	SHEN WEN-QING . NEUTRON RICH ISOTOPES ⁵⁴Ti, ⁵⁶V, ⁵⁷V, ⁵⁸Cr PRODUCED IN BOMBARDMENT OF ⁵⁶Fe TARGET WITH 79OMeV ¹³⁶Xe IONS. Chinese Physics C, 1982, 6(4): 462-465.
[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 and LUO Zhi-Quan. Pair neutrino energy loss for nuclei ⁵⁶Fe at the late stages of stellar evolution[J]. Chinese Physics C, 2008, 32(8): 617-619. doi: 10.1088/1674-1137/32/8/005

LIU Jing-Jing and LUO Zhi-Quan. Pair neutrino energy loss for nuclei ⁵⁶Fe at the late stages of stellar evolution[J]. Chinese Physics C, 2008, 32(8): 617-619. doi: 10.1088/1674-1137/32/8/005 shu

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

Received: 2007-08-13
Revised: 2007-09-23

Article Metric

Article Views(4258)
PDF Downloads(631)
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

Pair neutrino energy loss for nuclei ⁵⁶Fe at the late stages of stellar evolution

Corresponding author: LIU Jing-Jing,

Received Date: 2007-08-13

Accepted Date: 2007-09-23

Available Online: 2008-08-05

Abstract:

Based on the Weinberg-Salam theory, the pair neutrino energy loss rates for nuclei ⁵⁶Fe are canvassed for the wide range of density and temperature. The results of ours (Q_LJ) are compared with those of Beaudet G, Petrosian V and Salpeter E. E's (Q_BPS), and it shows that the pair neutrino energy loss rates of Q_BPS are always larger than Q_LJ .The Q_BPS is 12.57%, 12.86%, 14.99%, 19.80% times higher than Q_LJ corresponding to the temperature T₉=0.385, 1.0, 5.0, 10, respectively.

HTML

Reference (1)

Pair neutrino energy loss for nuclei ⁵⁶Fe at the late stages of stellar evolution

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article

Pair neutrino energy loss for nuclei ⁵⁶Fe at the late stages of stellar evolution

Corresponding author: LIU Jing-Jing,

HTML

目录

Pair neutrino energy loss for nuclei 56Fe at the late stages of stellar evolution

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article

Pair neutrino energy loss for nuclei 56Fe at the late stages of stellar evolution

Corresponding author: LIU Jing-Jing,

HTML

目录

Pair neutrino energy loss for nuclei ⁵⁶Fe at the late stages of stellar evolution

Pair neutrino energy loss for nuclei ⁵⁶Fe at the late stages of stellar evolution