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螺旋是自然界中普遍存在的一类精美且有序的结构实体。研究分子的螺旋自组装不仅能够助力我们理解天然手性的形成,也为我们制备手性传感器、手性催化剂、手性光学器件提供有效方法。然而,目前大多数通过自下而上构建螺旋型组装形态的报道都是采用传统后组装的方法,即将分子合成和分子组装的过程从时间尺度上隔离开,但这类方法存在溶液处理步骤繁琐、组装浓度低的缺点。
In 2006, Caltech's Paul Rothemund (BS '94)—now research professor of bioengineering, computing and mathematical sciences, and computation and neural systems—developed a method to fold a long strand of...
2016年5月26日,美国工程院院士、加州大学伯克利分校Lisa Alvarez-Cohen教授应邀访问北京大学环境与能源学院并进行了学术交流。
Associate Professor Lisa Kaltenegger,Department of Astronomy at Cornell University,A decade of exoplanet search has led to surprising discoveries, from giant planets close to their star, to planets or...
Lisa’s interdisciplinary studies center on natural resource extraction by transnational firms and the political ecology of land use primarily in Indonesia and Brazil. Lisa employs diverse methods to a...
Lisa Elfring,Associate Professor,Email: elfring@email.arizona.edu,Building: LSS 252 ,Phone: 520-621-1671,Education and Appointments:B.A. in Biology 1987, University of California, Santa Cruz;Ph.D. in ...
We quantify the potential for testing MOdified Newtonian Dynamics (MOND) with LISA Pathfinder (LPF), should a saddle point flyby be incorporated into the mission. We forecast the expected signal to no...
One of the atom interferometer gravitational wave missions proposed by Dimopoulos et al.1 in 2008 was called AGIS-Sat. 2. It had a suggested gravitational wave sensitivity set by the atom state detect...
In this article we give a brief review of the fundamental physics that can be done with the future space-based gravitational wave detector LISA. This includes detection of gravitational wave bursts co...
In this article we give a brief review of the fundamental physics that can be done with the future space-based gravitational wave detector LISA. This includes detection of gravitational wave bursts co...
We discuss strong gravitational lensing of gravitational waves from merging of massive black hole binaries in the context of the LISA mission. Detection of multiple events would provide invaluable inf...
In this article we give a brief review of the fundamental physics that can be done with the future space-based gravitational wave detector LISA. This includes detection of gravitational wave bursts co...
Coalescing massive Black Hole binaries are the strongest and probably the most important gravitational wave sources in the LISA band. The spin and orbital precessions bring complexity in the waveform ...
In order to attain the requisite sensitivity for LISA - a joint space mission of the ESA and NASA- the laser frequency noise must be suppressed below the secondary noises such as the optical path nois...
The inspiral of stellar compact objects into massive black holes, usually known as extreme-mass-ratio inspirals (EMRIs), is one of the most important sources of gravitational-waves for the future Lase...

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