
    HR-e                        d Z ddlZddlmZmZ  G d de          Z G d dee          Z ed	d
dddd          Z edddddd          Z	 edddddd          Z
 edddddd          Z eddd d!d"d          Z ed#d$d%d&dd          Z ed'd(d)d*d+d          Z ed,d-d.d*d+d          Z ed/d0d1d*d2d          Z ed3d4d5d*d6d          Z ed7d8d9d:d;d          Z ed<d=d>d?d@d          Z edAdBdCdDdd          Z edEdFdGdHdId          Z edJdKdLdMdNd          Z edOdPdQdRdSd          Z edTdUdVdWdXd          Z edYdZd[d\d]d          Z ed^d_d`dadbd          Z edcdddedfdd          Z edgdhdiej        z  djdd          Z edkdldmdndod          Z edpdqdrdsdtd          Z eej         ej!        ej"        ej"        z  duz  dvej#        ej"        z  duz  dw          Z$ eej         ej!        ej"        dxz  dyej#        dxz  dz          Z% eej         ej!        ej"        ej"        z  duz  d{ej#        ej"        z  duz  d|          Z&dS )}z
Astronomical and physics constants in SI units.  See :mod:`astropy.constants`
for a complete listing of constants defined in Astropy.
    N   )Constant
EMConstantc                   *    e Zd ZdZi Z e            ZdS )
CODATA2014zCODATA 2014N)__name__
__module____qualname__default_reference	_registryset_has_incompatible_units     <lib/python3.11/site-packages/astropy/constants/codata2014.pyr   r      s'        %I!ceer   r   c                       e Zd Zej        ZdS )EMCODATA2014N)r   r	   r
   r   r   r   r   r   r   r      s        $IIIr   r   hzPlanck constantgW9zJ sgfkehZf7si)systemhbarzReduced Planck constantgx# 8g}Z <7k_BzBoltzmann constantg^t0;zJ / (K)gUd9czSpeed of light in vacuumg   JxޱAzm / (s)g        GzGravitational constantg7^wX=zm3 / (kg s2)gn<g0z Standard acceleration of gravityg:#@zm / s2m_pzProton massgq祭`:kggL+8m_nzNeutron massgr`:m_ezElectron massgay9gՓ8uzAtomic massgUtq`:gz8sigma_sbzStefan-Boltzmann constantgB*Kqn>zW / (K4 m2)gnb]KB=ezElectron chargegp%ڤ<CgC0iS:eps0zElectric constantg.Hvx=zF/mN_AzAvogadro's numberggK҅Dz	1 / (mol)g VBJ:CRzGas constantg;  @zJ / (K mol)gv!>RydzRydberg constantg71rDdAz1 / (m)gC8
?a0zBohr radiusgRԁ=mgU;muBzBohr magnetongͻUl&;zJ/Tghe99alphazFine-structure constantg,)}? gΎ}=atmzStandard atmospherei͋ Pamu0zMagnetic constantgHך>zN/A2sigma_Tz Thomson scattering cross-sectiong@:m2g%7>8b_wienz)Wien wavelength displacement law constantgg?zm Kg9u׭4>g      $@statCesu
   abCemuFrgauss)'__doc__numpynpconstantr   r   r   r   r   r   r   r   r   r   r   r   r   r    r!   r"   r$   r%   r&   r'   r(   r*   r+   r-   pir/   r0   r2   abbrevnamevalueuncertaintye_esue_emue_gaussr   r   r   <module>rF      s   
     * * * * * * * *
$ $ $ $ $ $ $ $% % % % %:z % % % J	OUOD   z
	   j	NSW   J	#[)S  
 J	!;TX   Z
,gxT   j	=/4   j	>?D/$   j	?ND.   JsM?D/RVWWW:   L	,c3CD   |
%T   j	^TX   JsNI}iPTUUUj		8D   Z-*C1B4   j	?OUK   	
	 	 	 j-vtSNNNj+Vbe^VSQUVVV
*&   
/	
 
 
 	HFGagMAGd"	 	 	 	HafaglE1=2+=e	 	 	 ,HFGagMAGd"  r   