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14㧚Current status of Nuclear Reaction Data File for Astrophysics (NRDF/A)
T. Yoshida, N. Furutachi, M. Kimura, M. Asano, T. Togashi, H. Murakami and K. Kato

Nuclear Research Data Centre, Hokkaido University (JCPRG)
N. Otuka

Nuclear Data Section, International Atomic Energy Agency
Abstract
Recent activities in JCPRG for compilations of EXFOR and Nuclear Reaction Data File (NRDF)
have been introduced. As an extension of such activities, a preparation of new nuclear data libraries:
Nuclear Reaction Data File for Astrophysics (NRDF/A) has been planned. The framework of thedata table has been almost built. As the next step, evaluations by using cluster models have beenplanned.

Introduction
The main activity of JCPRG is compilation of experimental nuclear reaction data. Compilation
works of observed data are done in the following steps: compilers input bibliography, experimental
condition and numerical data from experiment and complete the EXFOR compilations. This is
usually done within few weeks after publications of the articles if they agree with JCPRG
responsibility of compilations. If the numerical data are not available from authors, we makedigitization of the figures of experimental data. As the next step, we transmit compiled data to IAEA
Nuclear Data Section. After that, EXFOR reviewers check the compiled data and obtain author’s
proof. Finally, the nuclear data in the articles will be released about six month after publication. The
total number of charged particle reaction experiments for EXFOR compilation is about 3000. Ourcompilations contribute about 10 percent of the whole EXFOR data.

Besides EXFOR, we have been developing the original format, Nuclear Reaction Data File (NRDF).
Recently, the charged-particle nuclear data become more and more important, due to the increase ofastrophysical interest and medical use. By using NRDF, we can specifically treat physical quantity
even if they correspond to the integrated cross section (which astrophysical and medical applications
usually use) or nuclear structure data (typically differential cross section). The NRDF format has
flexibility which does not much depend on characteristic data in fields of study because of its large
capacity of construction of compilation codes.

Astrophysical nuclear reaction is one of the applications of NRDF where the nuclear network
calculation plays an important role [1]. For such reactions, we focus on neutrons, protons, alpha,gamma, or neutrino as incident or emitted particles. To study the evolution of the early universe, the㧙㧙,#'#%QPH

reactions concerning with light nuclei below the pf shell are important. Some of these astrophysicalreactions occur at very low temperature, which are difficult to reproduce by experiments because ofthe very small reaction rates. The evaluations based on the theoretical calculations are indispensible
to make up for the experiments. NACRE (Nuclear Astrophysics Compilation of Reaction rates) is
one of the most widely used evaluated astrophysical nuclear reaction data base [2]. However, it
becomes much better to take into account the most recent experimental data and use moresophisticated calculation in order to obtain more reliable evaluation.

Construction of the data table

We construct a new database for this study: we call this file as Nuclear Reaction Data File for
Astrophysics (NRDF/A). In the previous version of NRDF/A (2006), we have assembled only 31
reactions for nuclei from C to Mg. In the present new version (2008), the astrophysical importantlight nuclei up to Si are included to achieve the coverage for NACRE. As a result, the number ofreactions to be compiled is about 200.

We are planning to use cluster model calculations for evaluation. As one of such models, we use Antisymmetric Molecular Dynamics (AMD) [3]. This can be a good candidate for the models because ofits wide scope of application below the pf shell nuclei. Here, we can treat two important pictures,shell model like configuration and cluster configuration by taking proper parameters for effective
nuclear interactions.

Before making the evaluation, we are now preparing the data table. For each reaction, we search forthe corresponding articles in order to obtain the numerical data for future works of evaluation. Here,
we utilize the bibliographic information from Nuclear Science References (NSR) of National
Nuclear Data Center (NNDC). The data table consists of reaction information, energy range,
information of physical quantity and bibliographic information.

In the reaction information, energy ranges are given in addition to reaction equations. We also
compile how the physical quantities (cross section, reaction rate, S-factor, spectrum,electro-magnetic transition strength and log(ft)) are obtained. Here, we must notice that thenumerical values have not been compiled at the present stage. In compensation, we distinguish theanalyzed, deduced, measured and calculated data. The bibliographic information consists ofkey-number, journal name, volume number, publications year and author name. For the convenience,
we make the link to pdf files of articles by using digital object identifier (D.O.I.) if it is available.

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In order to choose the articles which are needed to assemble the numerical data for the evaluation,
we check the NRDF/A against EXFOR. This is because that we would like to directly use thenumerical values which is already appears in EXFOR. For this purpose, we put the coverage
information against EXFOR into each data set. After construction of the data table including
numerical values, the evaluation based on cluster model will be performed.

References[1] E. M. Burbidge et al., Rev. Mod. Phys. 29, 547 (1957).
[2] Angulo et al., Nucl. Phys. A 656, 3 (1999).
[3]Y. Kanada En'yo, H. Horiuchi and A. Ono, Phys. Rev. C 52, 628 (1995).

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Table 1 Example of data table in NRDF/A㫉㪼㪸㪺㫋㫀㫆㫅㪼㫅㪼㫉㪾㫐㪄㫄㫀㫅㩷㪼㫅㪼㫉㪾㫐㪄㫄㪸㫏㩷㪺㫉㫆㫊㫊㪄㫊㪼㪺㫋㫀㫆㫅 㪪㪄㪽㪸㪺㫋㫆㫉 㫂㪼㫐㪄㫅㫌㫄㪹㪼㫉㪸㫉㫋㫀㪺㫃㪼㪍㪣㫀㩿㫇㪃㪾㪀㪎㪙㪼 㪁㪏㪜㪂㪇㪊㪁㪈㪅㪊㪜㪂㪇㪌㪍㪣㫀㩿㫇㪃㪾㪀㪎㪙㪼 㪁㪈㪜㪂㪇㪊㪁㪈㪜㪂㪇㪎㪸㫅㪸㪍㪣㫀㩿㫇㪃㪾㪀㪎㪙㪼 㪁㪏㪜㪂㪇㪌㫄㪼㫊㪍㪣㫀㩿㫇㪃㪾㪀㪎㪙㪼 㪁㪏㪜㪂㪇㪋㪁㪈㪅㪈㪜㪂㪇㪌㪍㪣㫀㩿㫇㪃㪾㪀㪎㪙㪼㪍㪣㫀㩿㫇㪃㪾㪀㪎㪙㪼 㪥㫆㫋㩷㪾㫀㫍㪼㫅 㪁㪉㪜㪂㪇㪍㪍㪣㫀㩿㫇㪃㪾㪀㪎㪙㪼 㪥㫆㫋㩷㪾㫀㫍㪼㫅㪍㪣㫀㩿㫇㪃㪾㪀㪎㪙㪼㪁㪏㪜㪂㪇㪋㪍㪣㫀㩿㫇㪃㪾㪀㪎㪙㪼 㪁㪊㪜㪂㪇㪋㪁㪈㪅㪏㪜㪂㪇㪌 㫄㪼㫊㪍㪣㫀㩿㫇㪃㪾㪀㪎㪙㪼 㪁㪋㪜㪂㪇㪋㪁㪈㪅㪏㪜㪂㪇㪌㪍㪣㫀㩿㫇㪃㪾㪀㪎㪙㪼 㪁㪋㪜㪂㪇㪋㪁㪈㪅㪏㪜㪂㪇㪌㪍㪣㫀㩿㫇㪃㪾㪀㪎㪙㪼㪺㪸㫃㪍㪣㫀㩿㫇㪃㪾㪀㪎㪙㪼 㪁㪌㪜㪂㪇㪌㪁㪈㪜㪂㪇㪍㪍㪣㫀㩿㫇㪃㪾㪀㪎㪙㪼 㪥㫆㫋㩷㪾㫀㫍㪼㫅㪍㪣㫀㩿㫇㪃㪾㪀㪎㪙㪼 㪁㪋㪜㪂㪇㪌㪁㪈㪅㪈㪜㪂㪇㪍 㪁㫄㪼㫊㩷㪁㪺㪸㫃㪍㪣㫀㩿㫇㪃㪾㪀㪎㪙㪼 㪁㪉㪜㪂㪇㪌㪁㪈㪅㪉㪜㪂㪇㪍 㪁㫄㪼㫊㪍㪣㫀㩿㫇㪃㪾㪀㪎㪙㪼 㪁㪉㪜㪂㪇㪌㪁㪈㪅㪉㪜㪂㪇㪍 㫄㪼㫊㪍㪣㫀㩿㫇㪃㪾㪀㪎㪙㪼 㫃㫆㫎㪺㪸㫃㪍㪣㫀㩿㫇㪃㪸㪀㪊㪟㪼 㪁㪐㪜㪂㪇㪋㪁㪌㪅㪏㪜㪂㪇㪌 㫄㪼㫊㪍㪣㫀㩿㫇㪃㪸㪀㪊㪟㪼 㫃㫆㫎㪸㫅㪸㪍㪣㫀㩿㫇㪃㪸㪀㪊㪟㪼 㫃㫆㫎㪸㫅㪸㪍㪣㫀㩿㫇㪃㪸㪀㪊㪟㪼㪈㪜㪂㪇㪍㪍㪣㫀㩿㫇㪃㪸㪀㪊㪟㪼㪁㪉㪜㪂㪇㪍㪍㪣㫀㩿㫇㪃㪸㪀㪊㪟㪼㪌㪜㪂㪇㪌㪍㪣㫀㩿㫇㪃㪸㪀㪊㪟㪼 㪥㫆㫋㩷㪾㫀㫍㪼㫅㪍㪣㫀㩿㫇㪃㪸㪀㪊㪟㪼 㪈㪜㪂㪇㪋㪈㪅㪇㪇㪋㪜㪂㪇㪍 㪁㫄㪼㫊㪍㪣㫀㩿㫇㪃㪸㪀㪊㪟㪼 㪁㪈㪅㪏㪜㪂㪇㪌 㪁㪉㪅㪏㪜㪂㪇㪌㪍㪣㫀㩿㫇㪃㪸㪀㪊㪟㪼 㪁㪈㪅㪍㪏㪜㪂㪇㪏 㪁㪉㪅㪇㪈㪜㪂㪇㪏 㪁㫄㪼㫊㪍㪣㫀㩿㫇㪃㪸㪀㪊㪟㪼 㪁㪋㪅㪎㪏㪜㪂㪇㪎 㪁㪍㪅㪉㪌㪜㪂㪇㪎 㪁㫄㪼㫊㪍㪣㫀㩿㫇㪃㪸㪀㪊㪟㪼 㪁㪋㪜㪂㪇㪐㪁㫄㪼㫊㪍㪣㫀㩿㫇㪃㪸㪀㪊㪟㪼 㪁㪈㪜㪂㪇㪍㪁㪉㪅㪍㪜㪂㪇㪍 㪁㫄㪼㫊㪍㪣㫀㩿㫇㪃㪸㪀㪊㪟㪼 㪁㪋㪅㪌㪜㪂㪇㪎㪁㫄㪼㫊㪍㪣㫀㩿㫇㪃㪸㪀㪊㪟㪼 㪁㪋㪅㪌㪜㪂㪇㪎㪁㫄㪼㫊㪍㪣㫀㩿㫇㪃㪸㪀㪊㪟㪼 㪁㪈㪅㪌㪈㪜㪂㪇㪌 㪁㪊㪅㪈㪎㪜㪂㪇㪌 㪁㫄㪼㫊㩷㪻㪼㪻㪍㪣㫀㩿㫇㪃㪸㪀㪊㪟㪼 㪁㪈㪅㪌㪈㪜㪂㪇㪌 㪁㪊㪅㪈㪎㪜㪂㪇㪌 㪁㫄㪼㫊㩷㪻㪼㪻㪍㪣㫀㩿㫇㪃㪸㪀㪊㪟㪼 㪁㪋㪅㪌㪜㪂㪇㪎㪁㫄㪼㫊㪍㪣㫀㩿㫇㪃㪸㪀㪊㪟㪼 㪁㪋㪅㪌㪜㪂㪇㪎㪁㫄㪼㫊㩷㪻㪼㪻㪍㪣㫀㩿㫇㪃㪸㪀㪊㪟㪼 㪁㪍㪅㪍㪌㪜㪂㪇㪏㫄㪼㫊㪍㪣㫀㩿㫇㪃㪸㪀㪊㪟㪼 㪁㪍㪅㪍㪌㪜㪂㪇㪏㫄㪼㫊㪍㪣㫀㩿㫇㪃㪸㪀㪊㪟㪼 㪁㪈㪅㪊㪍㪜㪂㪇㪍㫄㪼㫊㪍㪣㫀㩿㫇㪃㪸㪀㪊㪟㪼 㪁㪉㪅㪊㪜㪂㪇㪋 㪁㪌㪜㪂㪇㪋㪁㫄㪼㫊㪍㪣㫀㩿㪸㪃㪾㪀㪈㪇㪙 㪩㪼㫊㫆㫅㪸㫅㪺㪼㪍㪣㫀㩿㪸㪃㪾㪀㪈㪇㪙 㪁㪈㪅㪈㪎㪜㪂㪇㪍 㪁㪈㪅㪈㪏㪌㪜㪂㪇㪍㪍㪣㫀㩿㪸㪃㪾㪀㪈㪇㪙㪁㪉㪜㪂㪇㪍㪍㪣㫀㩿㪸㪃㪾㪀㪈㪇㪙 㪥㫆㫋㩷㪾㫀㫍㪼㫅㪍㪣㫀㩿㪸㪃㪾㪀㪈㪇㪙 㪁㪈㪅㪇㪏㪌㪜㪂㪇㪍 㪁㪈㪅㪈㪎㪌㪜㪂㪇㪍 㪁㫄㪼㫊㪍㪣㫀㩿㪸㪃㪾㪀㪈㪇㪙 㪁㪈㪅㪉㪎㪍㪜㪂㪇㪍㫄㪼㫊㪍㪣㫀㩿㪸㪃㪾㪀㪈㪇㪙 㪁㪈㪜㪂㪇㪍㪁㪈㪏㪜㪂㪇㪍㪍㪣㫀㩿㪸㪃㪾㪀㪈㪇㪙㪁㪊㪅㪎㪜㪂㪇㪍 㪸㫅㪸㪍㪣㫀㩿㪸㪃㪾㪀㪈㪇㪙 㪩㪼㫊㫆㫅㪸㫅㪺㪼㪍㪣㫀㩿㪸㪃㪾㪀㪈㪇㪙 㪁㪈㪅㪇㪊㪜㪂㪇㪍 㪁㪈㪅㪉㪜㪂㪇㪍㪍㪣㫀㩿㪸㪃㪾㪀㪈㪇㪙 㪩㪼㫊㫆㫅㪸㫅㪺㪼㪍㪣㫀㩿㪸㪃㪾㪀㪈㪇㪙 㪁㪈㪅㪈㪋㪜㪂㪇㪍 㪁㪈㪅㪉㪌㪂㪜㪇㪍 㪁㫄㪼㫊㫉㪼㪽㪼㫉㪼㫅㪺㪼㫊㩷㫆㪽㩷㪸㫉㫋㫀㪺㫃㪼㪻㪼㪻㪺㪸㫃㪻㪼㪻㫄㪼㫊㪻㪼㪻㪻㪼㪻㪸㫅㪸㪸㫅㪸㪻㪼㪻㫍㫆㫃㫌㫄㪼 㫇㪸㪾㪼㪉㪇㪇㪋㪧㪩㪇㪐 㪧㪩㪆㪚㪎㪇㪉㪇㪇㪋㪤㪬㪱㪯 㪠㪥㪛㪚㩿㪡㪧㪥㪀㪆㪬 㪈㪐㪉㪉㪇㪇㪇㪪㪢㪇㪉 㫉㪼㪽㪲㪸㪴㪌㪉㪇㪇㪇㪢㪜㪱㪰 㫉㪼㪽㪲㪹㪴㪉㪇㪇㪇㪙㪘㪇㪐 㪧㪩㪆㪚㪍㪈㪈㪐㪐㪎㪥㪦㪇㪋 㪧㪩㪆㪚㪌㪍㪈㪐㪐㪍㪩㪜㪈㪍 㪘㪧㪧㪆㪙㪉㪎㪈㪐㪐㪍㪣㪘㪈㪇 㪧㪩㪆㪚㪌㪊㪈㪐㪐㪊㪙㪩㪱㪨 㫉㪼㪽㪲㪺㪴㪈㪐㪐㪉㪚㪜㪇㪉 㪥㪧㪆㪘㪌㪊㪐㪈㪐㪐㪈㪚㪜㪱㪱 㪙㪘㪧㪊㪍㪈㪐㪐㪇㪢㪬㪱㪮 㫉㪼㪽㪲㪻㪴㪈㪐㪏㪎㪫㪠㪇㪌 㪘㪡㪧㪋㪇㪈㪐㪏㪊㪪㪜㪱㪫 㪙㪘㪧㪉㪏㪈㪐㪏㪊㪦㪪㪇㪋 㪥㪚㪆㪘㪎㪍㪈㪐㪎㪐㪪㪮㪇㪉 㪥㪧㪆㪘㪊㪊㪈㪈㪐㪎㪏㪪㪮㪱㪱 㪩㪜㪧㪫㩷㪬㪤㪄㪧㪏㪏㪈㪐㪎㪋㪙㪘㪯㪘 㪩㪜㪧㪫㩷㪚㪦㪥㪝㪎㪋㪇㪉㪈㪏㪉㪇㪇㪏㪚㪩㪇㪉 㪡㪧㪆㪞㪊㪌㪉㪇㪇㪊㪪㪧㪇㪉 㪥㪧㪆㪘㪎㪈㪐㪉㪇㪇㪉㪙㪘㪎㪎 㪥㪧㪆㪘㪎㪇㪎㪈㪐㪐㪏㪘㪥㪈㪏 㪥㪧㪆㪘㪍㪊㪐㪈㪐㪐㪎㪥㪦㪇㪋 㪧㪩㪆㪚㪌㪍㪈㪐㪐㪎㪙㪦㪈㪉 㪥㪧㪆㪘㪍㪈㪎㪈㪐㪐㪎㪙㪘㪐㪌 㪥㪧㪆㪘㪍㪉㪎㪈㪐㪐㪉㪜㪥㪇㪈 㪧㪣㪆㪙㪉㪎㪐㪈㪐㪐㪈㪙㪬㪈㪋 㪥㪠㪤㪆㪘㪊㪇㪈㪈㪐㪏㪎㪙㪠㪱㪰 㫉㪼㪽㪲㪼㪴㪈㪐㪏㪋㪥㪜㪇㪌 㪰㪝㪋㪇㪈㪐㪎㪐㪝㪩㪈㪉 㪧㪩㪆㪚㪉㪇㪈㪐㪎㪎㪣㪠㪇㪈 㪥㪧㪆㪘㪉㪎㪌㪈㪐㪎㪉㪛㪜㪇㪈 㪥㪧㪆㪘㪈㪎㪏㪈㪐㪎㪉㪙㪬㪈㪍 㪡㪚㪧㪌㪇㪈㪐㪎㪈㪪㪧㪇㪌 㪥㪧㪆㪘㪈㪍㪋㪈㪐㪎㪈㪪㪧㪇㪌 㫉㪼㪽㪲㪽㪴㪈㪐㪍㪈㪐㪎㪈㪙㪬㪉㪋 㪥㪧㪆㪘㪈㪎㪏㪈㪐㪎㪈㪙㪩㪈㪉 㪧㪩㪆㪚㪊㪈㪐㪎㪇㪢㪦㪉㪌 㪰㪝㪈㪈㪈㪐㪎㪇㪢㪦㪉㪌 㪪㫆㫍㪅㪡㪅㪥㫌㪺㫃㪅㪧㪿㫐㫊 㪈㪈㪈㪐㪍㪐㪣㪜㪇㪏 㪥㪠㪤㪍㪐㪈㪐㪍㪎㪝㪠㪇㪌 㪥㪧㪆㪘㪐㪍㪉㪇㪇㪋㪞㪰㪱㪱 㫉㪼㪽㪲㪾㪴㪉㪇㪇㪋㪞㪰㪇㪉 㪜㪧㪡㪆㪘㪉㪈㪈㪐㪐㪎㪥㪦㪇㪋 㪧㪩㪆㪚㪌㪍㪈㪐㪐㪍㪩㪜㪈㪍 㪘㪧㪧㪆㪙㪉㪎㪈㪐㪏㪐㪙㪘㪉㪋 㪥㪧㪆㪘㪋㪐㪐㪈㪐㪏㪎㪤㪬㪈㪊 㪧㪩㪣㪌㪐㪈㪐㪏㪍㪤㪰㪱㪱 㪙㪘㪧㪊㪈㪈㪐㪏㪍㪚㪜㪇㪌 㪥㪠㪤㪆㪘㪉㪋㪌㪈㪐㪏㪌㪥㪜㪇㪌 㪧㪩㪆㪚㪊㪈㪈㪐㪏㪋㪥㪘㪇㪎 㪥㪧㪆㪘㪋㪈㪎㪈㪐㪏㪊㪥㪘㪱㪱 㪙㪘㪧㪉㪏㪈㪐㪎㪐㪪㪧㪇㪈 㪥㪧㪆㪘㪊㪈㪏㫐㪼㪸㫉 㪽㫀㫉㫊㫋㩷㪸㫌㫋㪿㫆㫉㪌㪌㪏㪇㪈㪉㪇㪇㪋 㪩㪅㪤㪅㪧㫉㫀㫆㫉㪈㪌㪍㪉㪇㪇㪋 㪫㪅㪤㫌㫉㪸㫋㪸㪈㪐㪏㪉㪇㪇㪇 㪜㪅㪪㫂㫉㪼㫋㫀㪋㪉㪉㪇㪇㪇 㪡㪅㪟㪅㪢㪼㫃㫃㪼㫐㪉㪌㪏㪇㪈㪉㪇㪇㪇 㪛㪅㪙㪸㫐㪼㪈㪈㪋㪋㪈㪐㪐㪎 㪢㪅㪤㪅㪥㫆㫃㫃㪼㫋㫋㪉㪊㪈㪈 㪍 㪟㪅㪩㪼㪹㪼㫃㪐㪐㪈㪐㪎㪎㪈㪐㪐㪍 㪚㪅㪤㪅㪣㪸㫐㫄㫆㫅㪈㪍㪐㪈㪐 㪊 㪩㪅㪙㫉㫌㫊㫊㪐㪎㪌㪈㪐㪐㪉 㪝㪅㪜㪅㪚㪼㪺㫀㫃㪥㫆㪅㪋㪃㩷㪈㪉㪋㪉㪃㩷㪙㪈㪇㩷㪈㪉㩷 㪈㪐㪐㪈 㪝㪅㪜㪅㪚㪼㪺㫀㫃㪐㪇㪈㪐㪐㪇 㪧㪅㪛㪅㪢㫌㫅㫑㪊㪈㪐㪈㪐㪏㪎 㪚㪅㪠㪅㪮㪅㪫㫀㫅㪾㫎㪼㫃㫃㪥㫆㪅㪎㪃㪐㪍㪌㪃㪘㪙㪎㪈㪐㪏㪊 㪩㪅㪞㪅㪪㪼㫐㫃㪼㫉㪎㪊㪈㪐㪏㪊 㪩㪅㪦㫊㫋㫆㫁㫀㪺㪌㪇㪈㪐㪎㪐 㪱㪅㪜㪅㪪㫎㫀㫋㫂㫆㫎㫊㫂㫀㪉㪊㪈㪐㪎㪏 㪪㫎㫀㫋㫂㫆㫎㫊㫂㫀㪊㪍㪈㪐㪎㪋㪈㪋㪇㪇㪋㪉㪇㪇㪏 㪡㪅㪚㫉㫌㫑㪐㪐㪺㪉㪇㪇㪊 㩷㪚㪅㪪㫇㫀㫋㪸㫃㪼㫉㫀㪉㪎㪎㪉㪇㪇㪉 㪝㪅㪚㪅㪙㪸㫉㫂㪼㫉㪎㪊㪊㪈㪐㪐㪏 㪚㪅㪘㫅㪾㫌㫃㫆㪈㪈㪋㪋㪈㪐㪐㪎 㪢㪅㪤㪅㪥㫆㫃㫃㪼㫋㫋㪌㪎㪈㪐㪐㪎 㪰㪅㪙㫆㫌㪻㫆㫌㫄㪸㪊㪉㪋㪈㪐㪐㪎 㪘㪅㪙㪅㪙㪸㫃㪸㫅㫋㪼㫂㫀㫅㪉㪇㪈㪐㪐㪉 㪪㪅㪜㫅㪾㫊㫋㫃㪼㫉㪊㪏㪊㪈㪐㪐㪈 㪣㪅㪙㫌㪺㪿㫄㪸㫅㫅㪜㪏㪉㪈㪐㪏㪎 㪣㪅㪙㫀㫄㪹㫆㫋㪋㪊㪈㪐㪏㪋 㪦㪅㪝㪅㪥㪼㫄㪼㫋㫊㪉㪉㪌㪎㪈㪐㪎㪐 㪪㪅㪝㫉㪸㫅㫂㪼㫃㪐㪊㪈㪐㪎㪎 㪚㪅㪄㪪㪅㪣㫀㫅㪋㪈㪎㪈㪐㪎㪉 㪩㪅㪤㪅㪛㪼㫍㫉㫀㪼㫊㪈㪉㪐㪌㪈㪐㪎㪉 㪪㪅㪥㪅㪙㫌㫅㫂㪼㪈㪈㪐㪎㪈 㪟㪅㪪㫇㫀㫅㫂㪸㪍㪊㪋㪈㪐㪎㪉 㪟㪅㪪㫇㫀㫅㫂㪸㪈㪐㪏㪊 㪪㪅㪥㪅㪙㫌㫅㫂㪼㫉㪈㪎㪎㪈㪈㪐㪎㪈 㪢㪅㪟㪅㪙㫉㪸㫐㪎㪈㪈㪈㪐㪎㪇 㪭㪅㪠㪅㪢㫆㫄㪸㫉㫆㫍㪊㪐㪐㪈㪐㪎㪇 㪭㪅㪠㪅㪢㫆㫄㪸㫉㫆㫍㪈㪈㪌㪈㪐㪍㪐 㪞㪅㪤㪅㪣㪼㫉㫅㪼㫉㪌㪈㪊㪈㪐㪍㪎 㪦㪅㪝㫀㪼㪻㫃㪼㫉㪉㪇㪇㪋 㪞㫐㪅㪞㫐㫌㫉㫂㫐㪊㪌㪌㪞㫐㪅㪞㫐㫌㫉㫂㫐㪈㪈㪋㪋㪈㪐㪐㪎 㪢㪅㪤㪅㪥㫆㫃㫃㪼㫋㫋㪉㪊㪈㪈 㪍 㩷㪟㪅㪩㪼㪹㪼㫃 㪐㪐㪊㪌㪊㪈㪐㪏㪐 㩷㪘㪅㪢㪅㪙㪸㫊㪸㫂㪈㪇㪏㪏㪈㪐㪏㪎 㪛㪅㪜㪅㪤㫌㫉㫅㫀㪺㫂㪥㫆㪅㪋㪃㩷㪎㪏㪎㪃㩷㪙㪠㪌㪈㪐㪏㪍 㪜㪅㪞㪅㪤㫐㪼㫉㫊㪌㪋㪎㪈㪐㪏㪍 㪝㪅㪜㪅㪚㪼㪺㫀㫃㪉㪉㪐㪌㪈㪐㪏㪌 㪡㪅㪜㪅㪥㪼㫃㫊㫆㫅㪉㪏㪐㪈㪐㪏㪋 㪡㪅㪥㪸㫇㫆㫃㫀㫋㪸㫅㫆㪥㫆㪅㪋㪃㩷㪍㪌㪇㪃㩷㪘㪞㪋㪈㪐㪏㪊 㪡㪅㪥㪸㫇㫆㫃㫀㫋㪸㫅㫆㪉㪈㪈㪐㪎㪐 㪩㪅㪟㪅㪪㫇㪼㪸㪲㪸㪴㩷㪫㫉㪸㫅㫊㪅㪙㫌㫃㪾㪅㪥㫌㪺㫃㪅㪪㫆㪺㪅㪲㪹㪴㩷㪫㫉㫀㪸㫅㪾㫃㪼㩷㪬㫅㫀㫍㪅㪥㫌㪺㫃㪼㪸㫉㩷㪣㪸㪹㪅㪃㩷㪘㫅㫅㪅㪩㪼㫇㫋㪅㪲㪺㪴㩷㪧㫉㫆㪺㪅㪉㫅㪻㩷㪠㫅㫋㪼㫉㫅㪅㪪㫐㫄㫇㫆㫊㫀㫌㫄㩷㫆㫅㩷㪥㫌㪺㫃㪼㪸㫉㩷㪘㫊㫋㫉㫆㫇㪿㫐㫊㫀㪺㫊㪃㩷㪥㫌㪺㫃㪼㫀㩷㫀㫅㩷㫋㪿㪼㩷㪚㫆㫊㫄㫆㫊㪃㩷㪢㪸㫉㫃㫊㫉㫌㪿㪼㪃㩷㪞㪼㫉㫄㪸㫅㫐㩷㩷㩷㩷㪍㪄㪈㪇㩷㪡㫌㫃㫐㪃㩷㪈㪐㪐㪉㪃㩷㪝㪅㪢㪸㫇㫇㪼㫃㪼㫉㪃㩷㪢㪅㪮㫀㫊㫊㪿㪸㫂㪃㩷㪜㪻㫊㪅㪃㩷㪠㪦㪧㩷㪧㫌㪹㫃㫀㫊㪿㫀㫅㪾㩷㪣㫋㪻㪅㪃㩷㪙㫉㫀㫊㫋㫆㫃㪃㩷㪜㫅㪾㫃㪸㫅㪻㪲㪻㪴㩷㪬㫅㫀㫍㪅㪚㫆㫃㫆㫉㪸㪻㫆㪃㩷㪥㫌㪺㫃㪅㪧㪿㫐㫊㪅㪣㪸㪹㪅㪃㩷㪫㪼㪺㪿㪅㪧㫉㫆㪾㪅㪩㪼㫇㫋㪅㪲㪼㪴㩷㪬㫅㫀㫍㪅㪧㪸㫉㫀㫊㪃㩷㪠㫅㫊㫋㪅㪧㪿㫐㫊㪅㪥㫌㪺㫃㪅㪃㩷㪈㪐㪏㪍㩷㪘㫅㫅㪅㪩㪼㫇㫋㪅㪲㪽㪴㩷㪜㫉㫉㪸㫋㫌㫄㩷㪥㫌㪺㫃㪅㪧㪿㫐㫊㪆㪘㪲㪾㪴㩷㫅㫌㪺㫃㪄㪼㫏㪆㪇㪋㪇㪉㪇㪉㪇㪃㪇㪉㪆㪉㪍㪆㪉㪇㪇㪋㩷㩿㪉㪇㪇㪋㪀㧙㧙