1) radiant emittance
辐出度
1.
Using the statistical entropy of the spinning gravitation field of static spherically symmetric black hole,the radiant emittance of static spherically symmetric black hole is calculated,and we obtain a conclusin that the radiant emittance of black hole is proportionate to quartic power of temperature of the event horizon of the black hole.
利用静态球对称黑洞引力自旋场的统计熵,导出静态球对称黑洞引力自旋场的辐出度,得到了黑洞的辐出度与黑洞视界温度的四次方成正比的结论。
2.
By using the radiant emittance of Schwarzchild,the radiation spectrum of black hole are calcutated out.
利用史瓦西黑洞的辐出度,导出了黑洞费米子场和玻色子场的辐射谱及其对应的维恩位移定律, 并且得出二者的辐射谱及定律略有不同。
3.
By using statistical entropy of the Dirac field of static spherically symmetric black hole , the black hole s radiant emittance is educed and calculated, the conclusion that the radiant emittance of the black hole is in proportionate to the quartic power of the temperature of the black hole s event horizon is drawn.
利用静态球对称黑洞Dirac场的统计熵,导出黑洞的辐出度,得到了黑洞的辐出度与黑洞视界温度的四次方成正比的结论。
2) radiant exitance
辐出度
1.
The results of analysis show that we can acquire the radiant exitance of blackbody in bounded domain w.
通过分析可知,利用梯形法和辛普森法能够方便求出黑体在有界域内的辐出度值。
2.
Using radiant exitance of Schwarzschild black hole, the radiation spectrums of Fermion field and Boson field of black hole are calculated out, and Wien’s displacement laws are also obtained.
利用Schwarzschild黑洞的瞬时辐出度,导出黑洞Fermi子场和Bose子场的辐射谱及Wien位移定律。
3) radiant exitance
辐射出射度
1.
It is proved that radiant exitance M(T) = radiative capacity R = ractiant flux Φ 0(T), monochramat radiant exitance M λ(T) =emissive power ε γ,T (orελ,T) = spectrum-density(v).
分析了量子光学教材不同版本中关于发射本领与辐射本领两个概念的区别与联系 ,证明了辐射出射度M(T) =辐射本领R =辐射通量Ф0 (T) ,而单色辐出度Mλ(T) =发射本领εγ ,T(或ελ,T) =谱密度r(γ) ;从而澄清了极易混淆的 6个概念 ,并就量子光学教材建设提出了若干建议 。
4) instantaneous radiant exitance
瞬时辐出度
1.
Using entropy density of the rectilinearly accelerating non-stationary black hole with electric charges, the instantaneous radiant exitance is calculated,and a conclusion that the instantaneous radiant exitance of blank hole in a direction at any time is always proportional to quartic power of temperature of the event horizon of black hole on this direction is abtained.
利用变加速直线运动带电黑洞视界面附近的熵密度 ,导出黑洞的瞬时辐出度 ,得到了任一时刻黑洞沿某一方向的瞬时辐出度总是正比于在该方向上黑洞视界温度 4次方的结论。
2.
using entropy density near event horizon of the Vaidya-Bonner black hole,the instantaneous radiant exitance is calculated,and a conclusion that the instantaneous radiant exitance of black hole at any time is always proportional to quartic power of temperature of the event horizon of black hole is abtained.
利用Vaidya-Bonner黑洞视界面附近的熵密度,导出黑洞的瞬时辐出度,得到了任一时刻黑洞的瞬时辐出度总是正比于黑洞视界温度的四次方的结论。
5) instantaneous radiant emittance
瞬时辐出度
1.
Using entropy density near event horizon of the accelerating non-stationary black hole, the instantaneous radiant emittance is calculated, and we arrive at the conclusion that the instantaneous radiant emittance of black hole in a direction at any time is always proportional to the quartic power of temperature of the event horizon of black hole in that direction.
利用加速黑洞视界面附近的熵密度,导出黑洞的瞬时辐出度,得到了任一时刻黑洞沿某一方向的瞬时辐出度总是正比于在该方向上黑洞事件视界温度的四次方的结论。
2.
Using entropy density near event horizon of the Vaidya-Bonner-de Sitter black hole,the instantaneous radiant emittance is calculated out,and a conclusion that the instantaneous radiant emittance of black hole at any time is always proportional to quartic power of temperature of the event horizon of black hole is obtained.
利用Vaidya-Bonner-de S itter黑洞视界面附近的熵密度,导出黑洞的瞬时辐出度,得到了任一时刻黑洞的瞬时辐出度总是正比于黑洞视界温度四次方的结论。
3.
Selecting the advanced Eddington coordinates, and adopting the statistical method, the instantaneous radiant emittance of non-static black hole is calculated out.
选取超前爱丁顿坐标 ,采用统计的方法 ,计算出动态黑洞的瞬时辐出度 。
6) monochromat radiant exitance
单色辐出度
补充资料：最小辐亮度与最小辐照度(见核爆炸火球)
最小辐亮度与最小辐照度(见核爆炸火球)
minimum-brightness and minimum-irradiance
zuixiao fuliangdu yu zuixiaofu乙haodu最小辐亮度与最小辐照度(minimum-brightness and而nimum一irradianee)见核爆炸火球。
说明：补充资料仅用于学习参考，请勿用于其它任何用途。
参考词条