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相关论文: Interstellar communication. I. Maximized data rate…

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Future wireless systems are expected to support mission-critical services demanding higher and higher reliability. In this letter, we dimension the radio resources needed to achieve a given failure probability target for ultra-reliable…

信号处理 · 电气工程与系统科学 2023-06-13 Gilberto Berardinelli , Ramoni Adeogun

Interstellar communications are achievable with gram-scale spacecraft using swarm techniques introduced herein if an adequate energy source, clocks and a suitable communications protocol exist. The essence of our approach to the…

天体物理仪器与方法 · 物理学 2023-12-14 T. Marshall Eubanks , W. Paul Blase , Andreas Hein , Adam Hibberd , Robert G. Kennedy

We present a new decoding procedure to transmit classical information in a quantum channel which, saturating asymptotically the Holevo bound, achieves the optimal rate of the communication line. Differently from previous proposals, it is…

量子物理 · 物理学 2013-05-30 Vittorio Giovannetti , Seth Lloyd , Lorenzo Maccone

The development of modern technology extends human presence beyond cislunar space and onto other planets, which presents an urgent need for high-capacity, long-distance and interplanetary communication. Communication using photons as…

天体物理仪器与方法 · 物理学 2021-04-20 Zeng-Quan Yan , Cheng-Qiu Hu , Zhan-Ming Li , Zhong-Yuan Li , Hang Zheng , Xian-Min Jin

Noise fundamentally limits the capacity and reach in all communication links. In optical space communications, noise primarily originates from the detection process and limits the signal fidelity. . Therefore, the receiver sensitivity plays…

信号处理 · 电气工程与系统科学 2020-04-22 Ravikiran Kakarla , Jochen Schröder , Peter A. Andrekson

The space-time correlations of streams of photons can provide fundamentally new channels of information about the Universe. Today's astronomical observations essentially measure certain amplitude coherence functions produced by a source.…

天体物理仪器与方法 · 物理学 2009-03-03 C. Barbieri , M. K. Daniel , W. J. de Wit , D. Dravins , H. Jensen , P. Kervella , S. Le Bohec , F. Malbet , P. Nunez , J. P. Ralston , E. N. Ribak

At sufficiently low frequencies, no ground-based radio array will be able to produce high resolution images while looking through the ionosphere. A space-based array will be needed to explore the objects and processes which dominate the sky…

We present the analysis of between 50 and 100 hrs of coincident interferometric strain data used to search for and establish an upper limit on a stochastic background of gravitational radiation. These data come from the first LIGO science…

广义相对论与量子宇宙学 · 物理学 2008-11-26 LIGO Scientific Collaboration , B. Abbott

In the cm-wavelength range, an extraterrestrial electromagnetic narrow band (sine wave) beacon is an excellent choice to get alien attention across interstellar distances because 1) it is not strongly affected by interstellar /…

天体物理仪器与方法 · 物理学 2018-05-08 G. R. Harp , R. F. Ackermann , Samantha K. Blair , J. Arbunich , P. R. Backus , J. C. Tarter , the ATA Team

The dynamic spectrum of a radio pulsar is an in-line digital hologram of the ionised interstellar medium. It has previously been demonstrated that such holograms permit image reconstruction, in the sense that one can determine an…

天体物理学 · 物理学 2009-11-13 Mark Walker , Leon Koopmans , Dan Stinebring , Willem van Straten

The microhertz frequency band of gravitational waves probes the merger of supermassive black holes as well as many other gravitational wave phenomena. However, space-interferometry methods that use test masses would require further…

天体物理仪器与方法 · 物理学 2025-09-29 Matthew McQuinn , Casey McGrath

The modern practice of Radio Astronomy is characterized by extremes of data volume and rates, principally because of the direct relationship between the signal to noise ratio that can be achieved and the need to Nyquist sample the RF…

信息论 · 计算机科学 2014-05-23 Tim Natusch

Observations of neutron stars, whether in binaries or in isolation, provide information about the internal structure of the most extreme material objects in the Universe. In this work, we combine information from recent observations to…

高能天体物理现象 · 物理学 2021-08-29 Philippe Landry , Reed Essick , Katerina Chatziioannou

Imaging the direct light signal from a faint exoplanet against the overwhelming glare of its host star presents one of the fundamental challenges to modern astronomical instrumentation. Achieving sufficient signal-to-noise for detection by…

天体物理仪器与方法 · 物理学 2014-03-05 S. Lacour , P. Tuthill , J. D. Monnier , T. Kotani , L. Gauchet , P. Labeye

Communications to and from a spacecraft undertaking launch-landing interstellar travel at near light speed faces significant challenges. Photon-based communication is significantly impacted by large photon propagation delay and relativistic…

天体物理仪器与方法 · 物理学 2023-11-27 David Messerschmitt , Ian Morrison , Thomas Mozdzen , Philip Lubin

Stellar intensity interferometers correlate photons within their coherence time and could overcome the baseline limitations of existing amplitude interferometers. Intensity interferometers do not rely on phase coherence of the optical…

Using optimal matched filtering, we search 25 hours of data from the LIGO 40-meter prototype laser interferometric gravitational-wave detector for gravitational-wave chirps emitted by coalescing binary systems within our Galaxy. This is the…

New means of interstellar travel are now being considered by various research teams, assuming lightweight spaceships to be accelerated via either laser or solar radiation to a significant fraction of the speed of light (c). We recently…

天体物理仪器与方法 · 物理学 2017-08-31 René Heller , Michael Hippke , Pierre Kervella

Two way ranging data for spacecraft tracking of China's first Martian mission Tianwen-I is analysed. Shortly before the spacecraft entered the Mars parking orbit, the two way coherent microwave link between the spacecraft and the Earth…

广义相对论与量子宇宙学 · 物理学 2024-02-12 Xiaoming Bi , Zhongkai Guo , Xiaobo Zou , Yong Huang , Peijia Li , Jianfeng Cao , Lue Chen , Wenlin Tang , Yun Kau Lau

The radio sky at lower frequencies, particularly below 20 MHz, is expected to be a combination of increasingly bright non-thermal emission and significant absorption from intervening thermal plasma. The sky maps at these frequencies cannot…

天体物理仪器与方法 · 物理学 2021-09-01 Akhil Jaini , Avinash A. Deshpande , Sainath Bitragunta