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利用近红外到可见光的纳米等离子体技术预测低温氮解离催化剂

Prediction of a low-temperature N dissociation catalyst exploiting near-IR-to-visible light nanoplasmonics.

作者信息

Martirez John Mark P, Carter Emily A

机构信息

Department of Mechanical and Aerospace Engineering, Princeton University, Princeton, NJ 08544-5263, USA.

School of Engineering and Applied Science, Princeton University, Princeton, NJ 08544-5263, USA.

出版信息

Sci Adv. 2017 Dec 22;3(12):eaao4710. doi: 10.1126/sciadv.aao4710. eCollection 2017 Dec.

DOI:10.1126/sciadv.aao4710
PMID:29291247
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC5744471/
Abstract

Despite more than a century of advances in catalyst and production plant design, the Haber-Bosch process for industrial ammonia (NH) synthesis still requires energy-intensive high temperatures and pressures. We propose taking advantage of sunlight conversion into surface plasmon resonances in Au nanoparticles to enhance the rate of the N dissociation reaction, which is the bottleneck in NH production. We predict that this can be achieved through Mo doping of the Au surface based on embedded multireference correlated wave function calculations. The Au component serves as a light-harvesting antenna funneling energy onto the Mo active site, whereby excited-state channels (requiring 1.4 to 1.45 eV, near-infrared-to-visible plasmon resonances) may be accessed. This effectively lowers the energy barriers to 0.44 to 0.77 eV/N (43 to 74 kJ/mol N) from 3.5 eV/N (335 kJ/mol N) in the ground state. The overall process requires three successive surface excitation events, which could be facilitated by amplified resonance energy transfer due to plasmon local field enhancement.

摘要

尽管在催化剂和生产装置设计方面经过了一个多世纪的发展,但用于工业合成氨(NH₃)的哈伯-博施法仍需要能源密集型的高温高压条件。我们建议利用太阳光转化为金纳米颗粒中的表面等离子体共振来提高氮解离反应的速率,该反应是氨生产中的瓶颈。基于嵌入式多参考相关波函数计算,我们预测通过对金表面进行钼掺杂可以实现这一点。金组分充当光捕获天线,将能量导向钼活性位点,从而可以进入激发态通道(需要1.4至1.45电子伏特,近红外到可见光的等离子体共振)。这有效地将基态下从3.5电子伏特/氮原子(335千焦/摩尔氮原子)的能量势垒降低到0.44至0.77电子伏特/氮原子(43至74千焦/摩尔氮原子)。整个过程需要三个连续的表面激发事件,这可以通过等离子体局部场增强导致的共振能量转移放大来促进。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ffdd/5744471/c8c11a825fb2/aao4710-F3.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ffdd/5744471/3cc44b330177/aao4710-F1.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ffdd/5744471/7ae34ac63eeb/aao4710-F2.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ffdd/5744471/c8c11a825fb2/aao4710-F3.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ffdd/5744471/3cc44b330177/aao4710-F1.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ffdd/5744471/7ae34ac63eeb/aao4710-F2.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ffdd/5744471/c8c11a825fb2/aao4710-F3.jpg

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