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焦耳定律作为理想气体的能态方程,是热力学一般能态方程在理想气体物态方程约束下的特殊解,本质上不独立于物态方程.但焦耳定律却是理想气体温标等于热力学温标的充分必要条件,以理想气体温标表述理想气体定义时,物态方程和焦耳定律缺一不可. 相似文献
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关于玻意耳定律和焦耳定律相互独立性讨论的小结 总被引:1,自引:1,他引:0
玻意耳定律和焦耳定律相互独立,是热力学中早已有的论断.文献[1]以(δU/δp)θ→∞违反热力学为由,从玻意耳定律导出了焦耳定律,从而说明二者并非相互独立.文献[2]指出(δU/δp)θ→∞是可能的,并不违反热力学.该文还写出了遵从焦耳定律的气体物态方程的普遍形式(此式在前人的文献中已出现过)。 相似文献
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关于理想气体定义的再认识 总被引:5,自引:4,他引:1
本文指出:只需玻意耳定律和阿伏伽德罗定律即可定义理想气体.玻意耳定律和焦耳定律不是相互独立的,遵守玻意耳定律的气体必然服从焦耳定律,反之则不然.最后,作者对今日热力学教材中如何定义理想气体提出了建议. 相似文献
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关于焦耳效应与焦汤效应的关系,有的教科书中有如下的分析[1] 把焦汤系数aJT写成两项之和:aJT=第一项表示实际气体与焦耳定律偏离引起的贡献,第二项表示实际气体与玻意耳定律偏离引起的贡献.对焦耳定律的偏离使实际气体在节流膨胀后变冷;对玻意耳定律的偏离则既能致冷也能致温. 实际气体对玻意耳定律和焦耳定律的偏离井不独立,因此不宜把(1)式右方第一项看作焦耳效应在焦汤效应中的贡献. 焦耳实验研究气体绝热自由膨胀时的温度效应,焦汤实验研究气体绝热节流膨胀时的温度效应.两种过程的差别是前者气体的内能不变,后者气体的内能有变化.所… 相似文献
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证明在相对论热力学理论系统中,焦耳定律是玻意耳定律的推论,但玻意耳定律不是焦耳定律的推论. 相似文献
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针对新、旧人教版高中物理教材均缺少对焦耳定律实验探究的问题,利用DISLab设计相应实验内容,并自制配套的实验装置,实验过程操作简单,数据图像清晰明了,实现了对焦耳定律的科学定量探究. 相似文献
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气体的内能、焦耳-汤姆逊系数与理想气体 总被引:1,自引:1,他引:0
本文拟就满足焦耳定律的气体与焦耳-汤姆逊系数μ=0的气体的性质以及理想气体的定义作一些讨论.一、焦耳定律与物态方程 焦耳通过实验研究了气体的内能,得到了气体的内能U仅是温度的函数而与体积无关的结论,即 U=U(T)(l)这就是焦耳定律.式中T是用理想气体绝对温标量度的温度.精确的实验表明,一切实陈的气体,并不严格遵守焦耳定律,只有非常稀薄的气体才较好地服从式(1).假设绝对热力学温标量度的温度θ与T相等,即 T= (2)则由热力学第一定律和第二定律得到的能方程[1]可以证明。凡满足理想气体物态方程 PV=RT(4)的气体,一定满足焦耳定律… 相似文献
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H. Dandache 《Il Nuovo Cimento D》1989,11(10):1501-1506
Summary The semi-empirical Hugoniot equation of state is obtained by using the third-order tangency between the isentropic and the
Hugoniot curves at the origin of coordinates. The results of this model are in good agreement with Carter’s experimental data
for fourteen elements from the lanthanides series in the lower phase only.
Due to postal troubles with Lebanon, it was impossible to send proffs to the author as he requested. 相似文献
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超弹性碰撞演示实验是灵活运用大学物理知识的典型实验,本文对其最佳工作条件进行了分析,研究表明,当大球和小球的质量比为3时可以达到最佳的实验效果. 相似文献
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Nazmul Islam 《Molecular physics》2013,111(12):1533-1544
This study explored a new route for calculating the global hardness of atoms using spectroscopy. Working on a new definition of global hardness and relying on the Bohr model of the hydrogenic atom, a new formula for the global hardness of atoms was derived in terms of the wave number, reflecting the electron transition from the ground state to infinity. Since the spectral lines emitted from an atom bear the signature of all complex and complicated energetic effects, including relativity, in the internal constitution of the atom, it is expected that all such effects are automatically subsumed in the hardness data computed in terms of spectral lines. The hardness of the atoms of the 103 elements of the periodic table have been computed using spectral data and in terms of the new formula suggested in this work. The effect of relativity in pre- and post-lanthanoid elements is distinctly manifest. The express periodic behaviour and correlation of the most important physico-chemical properties of elements suggest that the present approach is an alternative scientifically meaningful method for evaluating the global hardness of atoms. 相似文献
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A technique to evaluate the accuracy with which the optical parameters of thin films are determined by the method of reflectance-spectrum extrema envelopes is presented. The general case of s-polarized light impinging obliquely on a weakly absorbing thin film formed on an absorbing substrate is discussed. Rather simple analytical expressions are derived which can easily be used in program realization on computers for calculating errors. On the basis of the error analysis, a procedure for determining the optical constants and thickness of thin films is proposed, which allows one to reach the maximum accuracy in solving the inverse problem of spectrophotometry. The optical constants and the thicknesses of the films of perylenetetracarboxylic acid and 2-[4-(4-aminophenyl)phenyliminomethyl]phenol formed on silicon substrates are found by the developed technique in the spectral range 550–900 nm. 相似文献
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利用物理力学定律对“和平号”空间站坠毁过程作了比较详细的计算和描述,旨在使读者在航天器有关知识有更多了解。 相似文献
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O. D. Ziganshina M. D. Él'kin V. V. Nechaev K. V. Berezin 《Journal of Applied Spectroscopy》2004,71(5):635-640
The structure and frequencies of the normal vibrations of the molecules of porphin, Mg-, Zh-, and Ni-porphin were calculated by the density-functional method in the B3LYP/6-31G(d) approximation, and correlation of their frequencies was made. The force fields have been obtained in dependent natural coordinates. It is shown that the majority of changes in the vibrational frequencies in transition from porphin to its metal complexes correlate with changes in the structure of the pyrrole and pyrrolenine rings of the porphin ligand. 相似文献
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Summary An analytical model, simulating the frictionless response of the sea contained in a rotating, rectangular channel of arbitrary
width to air pressure waves travelling at varying directions, is developed. Since planetary atmospheric waves are of primary
interest as forcing agents, a solution is found for subinertial frequencies. For an atmospheric wave travelling along a channel
whose width is close to the Rossby deformation radius, the model predicts sea levels and currents organized in two coastal
waves and a geostrophic current system prevailing in mid-basin. The right-hand coastal wave is more pronounced than the left-hand
wave. The structure is coupled to the atmospheric wave, and is resonantly driven when the phase velocity of the forcing wave
approaches the Kelvin wave velocity. Along the coasts a quasi-static adjustment occurs under off-resonant conditions. When
the atmospheric wave is moving across the channel at a sharp angle, the response of the sea is enhanced for the apparent along-channel
velocities below those of free shallow-water waves, due to reflections at channel boundaries. For the atmospheric wave that
travels at right angle across the channel, the resonance is not possible, and the sea level undershoots a simple inverted-barometer
response. Both travelling and standing waves appear in the channel. In the narrow-channel limit only a standing wave remains,
with a nodal line in the middle of the channel. In the central part of the channel the currents are almost geostrophic at
very low frequencies. The model is used to interpret some aspects of the response of the Mediterranean Sea to planetary-scale
atmospheric forcing. In particular, it is shown that resonant transfer of energy from the atmosphere to the sea is most unlikely,
since planetary atmospheric waves are rather slow and they travel along the main axis of the Mediterranean basin. 相似文献
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讨论了银道面内的引力场强分布和太阳在银河系中所受引力与到银心距离r的关系,指出引力场强g并不是与r的平方成反比,这是由于银河系的大小和形状不能忽略造成的.强调了万有引力定律的适用条件. 相似文献
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