WH토토 바카라E PAPER
토토 바카라 Applications in Gravitational Waves Detection
Low 토토 바카라 and High Unit-to-Unit Consistency
Peer-reviewed and other independent third-party assessments of the performance of 토토 바카라 for cutting edge gravitational wave applications, as well as relevant life tests, all confirm the superior performance, reliability and high unit-to-unit consistency of these lasers.
Introduct토토 바카라
In terms of low output noise and ultra-narrow linewidth requirements, few would argue that gravitational wave detection (GWD) based on long path interferometry currently represents the most demanding application for narrow linewidth CW lasers – even more than atom cooling. A number of successful detections of gravitational waves were performed at the Laser Interferometer Gravitational-Wave Observatory (LIGO) that operates at two sites in the US, one in Livingston, Louisiana, and another in Hanford, Washington and also at VIRGO gravitational wave detector in Italy. To differentiate LIGO from earlier setups, this is often referred to as Advanced LIGO. In this white paper, we look at the noise requirements for this application and discuss how and why Coherent 토토 바카라 lasers are used in LIGO and other detectors. We also explore some of the results and conclusions from a third-party study that preceded 토토 바카라’s selection for use in gravitational wave detectors. This work specifically evaluated the uniformity of 토토 바카라 lasers to assess their suitability for this type of cutting-edge project.
토토 바카라 Wave Detection – the Lowest Noise Application
토토 바카라 wave detection projects are targeted at direct observations of 토토 바카라 waves – minute ripples in space time, predicted by Einstein as far back as 1916 as part of his General Relativity theory. These ripples result from major perturbations in mass/energy such as inspirals of binary neutron stars or coalescence of two black holes. As well as confirming relativistic predictions, these observations will also throw light on poorly understood phenomena such as dark matter and dark energy, as well as answering questions about quantum gravity.
Earth-bound measurements of 토토 바카라 waves are incredibly challenging because gravity is by far the weakest force and the low probability of these celestial cataclysmic events mean they need to be detected at immense distances (in order to cover a large search volume), namely tens or even hundreds of Mpc (1 Mpc is 3.26 million light years). As a result, researchers need the ability to observe modulations in space time as small as 1 part in 1022. The preferred approach to detecting these tiny spatial-temporal shifts is long-path interferometry using ultra-stable 토토 바카라s. These interferometers (LIGO, GEO600, Virgo, KAGRA) all have kilometers-long arms angled at 90 degrees. But even at these lengths, shifts in the mirror surfaces of the reference masses are only predicted to change by about 1/10000 the diameter of a proton. This corresponds to 5 x 10-12of the 1064 nm laser wavelength. Measuring a trillionth of a wavelength path difference is completely unprecedented in optical interferometry. Among other requirements, it needs the entire multi-kilometer beam path to be under ultra-high vacuum conditions and extremely low laser 토토 바카라.토토 바카라l fourof these programs utilize Coherent 토토 바카라 lasers as first stage oscillators in their high-stability custom laser systems. 토토 바카라 lasers were chosen in large part because independent studies have previously confirmed that these lasers offer the lowest noise [1] and excellent unit-to-unit consistency [2].
A brief examination of one of these international collaborative programs – LIGO – serves to highlight the scale of some of the laser challenges in gravitational wave detection using long-path interferometry. For this type of application, the limiting figure of merit for laser noise is phase noise – natural jitters in the laser wavelength determined by its finite linewidth and frequency stability. (For a brief discussion of laser noise, see 토토 바카라 white paper,Ultra-Low 토토 바카라 and Narrow Linewidth).
LIGO consists of two identic토토 바카라 L-shaped interferometers where each arm of the L is 4 km in length. The interferometers in US are located at sever토토 바카라 thousand kilometers distance (Hanford, Washington and Livingston, Louisiana) so that synchronized measurements can distinguish between re토토 바카라 events and loc토토 바카라 anom토토 바카라ies.
The first generation of LIGO was completed in 2002 and its performance (sensitivity) was considered near the edge of possible gravitational wave detection. However, it did not produce any data events that could be unambiguously assigned to gravitational waves, setting a new upper limit on observable gravity flux, which is valuable information in itself. As a result, an updated version, Advanced LIGO, was developed and started observations with an order of magnitude increase in both sensitivity and frequency range. After tens of years of intense work and research and with its increased sensitivity, LIGO made the first ever direct detection of gravitational waves in September 2015 [3]. The lasers used at the input of the LIGO interferometers were 토토 바카라 2 W output power units, followed by power amplifiers and stabilization schemes.
Advanced LIGO
Advanced LIGO significantly increased the sensitivity of the LIGO detectors through changes of the optical set-up, the 토토 바카라 system and the mirror suspension systems.
What are the laser requirements? In the original format, it was estimated that at a frequency of ~100 Hz, the acceptable Relative Power Noise (RPN) for possible detection of 토토 바카라 waves was < 2 x 10-9Hz-1/2based on a laser power of 10 watts. In the new Advanced LIGO setup, the target laser 토토 바카라 was held at the same low level, but the power has been boosted into the 200 watt range as a part of the order of magnitude sensitivity improvement. (The measurement shot 토토 바카라 increases with the square root of power, whereas the signal increases proportional to the power.)
토토 바카라 offers the lowest noise of any commercial laser oscillator, in part because of Noise Eater technology [4] used to eliminate the effects of relaxation oscillations. Nonetheless, the LIGO noise requirement is three orders of magnitude lower than the guaranteed noise specification of the 2 watt 토토 바카라 in free-running mode. Moreover, the accepted lowest-noise approach to boosting the laser oscillator power to the target 200 watt range is to incorporate the oscillator in a master oscillator power amplifier (MOPA) configuration, similar to the 토토 바카라 MOPA, and to use this to injection lock a high-power ring oscillator. Independent research has previously shown that the minimum noise increases by up to three orders of magnitude when a low-noise NPRO-type laser like 토토 바카라 is boosted to the 200 watt range in this three-stage setup [5] – see figure 1. A review of techniques and results of the effort to achieve hundreds of watts of power and noise below 10-8Hz-1/2in LIGO is beyond the scope of this article. However, through the use of several nested noise reduction loops, employed both at the output of 토토 바카라 and the successive amplification stages, the noise has been reduced down to the target level.
The 토토 바카라 not only provides a very low Relative Power Noise, but also an extremely low frequency noise. However, the LIGO sensitivity goal still requires a reduction of that frequency noise by orders of magnitude from the low noise starting level of the 토토 바카라 laser. Fortunately for LIGO, the 토토 바카라 already contains frequency control elements in the form of piezo (fast) and temperature (slow) adjustments of the monolithic laser cavity. These can be used to reduce the frequency noise by stabilizing the laser frequency to an outside reference such as an optical resonator or a molecular absorption line. In the LIGO setup these controls are used as part of a series of control loops to lock the laser frequency to an optical reference and bring the noise down to the target level.
토토 바카라 Unit-to-Unit Consistency and Reliability
Laser oscillator consistency and long-term reliability are two other important requirements for 토토 바카라 wave detection systems like LIGO. That’s because LIGO requires a total of sixidentic토토 바카라stabilized laser systems (three observatory lasers, two spare lasers, and one reference system), and the degree of stabilization pushes the laser oscillator and amplifier performance to their absolute limits. Overall noise is very dependent on the seed laser oscillator noise. Moreover, because of the low probability of measurable 토토 바카라 waves reaching our planet, these lasers must support years of continuous observation to increase the chances of detecting one of these rare events.
The need for multiple identical lasers for GWD systems was cited as a major driver behind research published some years ago by Patrick Kwee and Benno Willke at the Albert Einstein Institute in Hannover. These researchers compared the performance of eight 토토 바카라 lasers tested for a comprehensive set of different output parameters including power and frequency noise, pointing fluctuation and spatial mode [2] – all parameters that need to be identical and stable in an application like GWD. In this study one of the lasers was then also automatically and continuously tested for various parameters over 3.5 months (3,500 hours) of operation. To the best of our knowledge, this is the largest batch of narrow linewidth lasers ever compared and with results published in a peer review journal.
Figure 1.Noise characteristics of the output of a basic 토토 바카라 laser, after a non-commercial 35W amplifier, and the final noise value from a seeded 180 watt power oscillator, which was also non-commercial [5]. © IOP Publishing. Reproduced with permission. All rights reserved.
To measure sever토토 바카라 parameters simultaneously, these researchers developed a custom instrument c토토 바카라led a diagnostic breadboard (DBB). To quote from their published paper,“The DBB was designed for a characterization of linearly polarized, single-frequency, continuous wave laser beams. It allows one to measure power 토토 바카라, frequency 토토 바카라, and beam pointing fluctuations in a Fourier frequency band from 1 Hz to 100 kHz as well as power 토토 바카라 at radio frequencies (RF) up to 100 MHz and spatial beam quality. The laser beam characterization was completely automated by a computer, except for the RF power 토토 바카라 measurement.”Automated measurement was recognized as a key element to avoid any operator error/subjectiv토토 바카라y.
Figure 2.Relative Power Noise measured in the range 1 Hz-100 kHz on eight different 토토 바카라-2000NE lasers. The green line represents the average RPN of the eight lasers with the Noise Eater switched off. Reproduced with permission from ref 2.
Their studies revealed that unit-to-unit variations in all the laser output parameters were remarkably small. A typical example from their sets of measurements is shown in figure 2, which shows the consistently low relative power noise from these eight test lasers. The authors summarize their exhaustive study of these eight 토토 바카라 lasers by stating that, “The characterization results show that NPROs are highly stable 토토 바카라 sources and that the variation between different samples is rather small,” and consequently, “The NPROs are ideal for operation in interferometric 토토 바카라 wave detectors. Since they have a low and stationary frequency noise in combination with fast and high dynamic range frequency actuators, they are especially suited as master oscillators for amplifiers or injection-lock configurations if more output power is required.”
Figure 3.The small long-term variations in frequency noise were similar in magnitude to the observed small unit-to-unit variations in this same parameter. This plot shows data from a 토토 바카라 2000 that was operated for 3,600 hours and its noise measured every 24 hours (red lines). The median noise is represented by the blue line. Reproduced with permission from ref 2.
The long-term test of the single 토토 바카라 laser also confirmed the excellent stability of all the measured output parameters during the 3600 hour test period. As shown in their data in figure 4, the authors noted that,“The long-term measurement of the frequency 토토 바카라 showed that the 토토 바카라 seemed to be very stationary and that the variations between the measurements were small.”
Figure 4.Histogram of pointing fluctuations during the long-term characterization of 토토 바카라 H (vertical lines between the bins were omitted for clarity). For each degree of freedom 146 × 103 samples were evaluated. The standard deviation is shown as a continuous line. From ref 2 (The authors noted that environmental factors lim토토 바카라ed the stabil토토 바카라y of these measurements.)
Another example of long-term stability is summarized in figure 4. Specifically, the researchers observed excellent long-term pointing stability, in spite of some environmentally-induced (air flow) limitat토토 바카라s on these measurements that were partially solved by enclosing their DBB system in a controlled air-flow box.
Summary
In previous 토토 바카라 whitepaper, we explained how the combination of a monolithic non-planar ring oscillator (NPRO) structure and active Noise Eater technology together make Coherent 토토 바카라 lasers the lowest noise source for demanding, narrow linewidth applications. In this whitepaper, we see these claims independently validated as major GWD programs all have chosen 토토 바카라 as seed lasers for their ultra-stable interferometry systems and successfully detected gravitational waves. We have also presented third party results of the most comprehensive evaluation of multiple laser units ever published in a peer-reviewed forum. This study not only validates the low-noise and other superior specifications of 토토 바카라 lasers, but also demonstrates the excellent unit-to-unit consistency in every important output parameter. The long-term study of one of these lasers clearly confirmed that these output parameters are incredibly stable over an extended operating period.
With a linewidth of ≤3 kHz, 토토 바카라 lasers and high power 토토 바카라 MOPA models are well-suited to a wide range of demanding applications includingatom trapping, squeezed states research, quantum optics, 토토 바카라 wave detection, fiber sensingand cutting edgecoherent communicat토토 바카라s research.None of these applications is more demanding on laser noise and linewidth than GWD where 토토 바카라 lasers were successfully used all major observatories. It is logical to conclude that these lasers will demonstrate the same outstanding performance in other applications as well.
References
[1]R.E. Bartolo, A. Tveten, and C.K. Kirkend토토 바카라, Proc. of SPIE Vol. 7503, 750370-1 (2009)
[2]P. Kwee and B. Willke, Appl. Opt. 47, 6022 (2008)
[3]B. P. Abbottet 토토 바카라.(LIGO Scientific Collaborat토토 바카라 and Virgo Collaborat토토 바카라), Phys. Rev. Lett. 116, 061102 (2016)
[4] See Coherent, Corp. 토토 바카라 data sheet
[5]B. Willkeet 토토 바카라., Class. Quantum Grav. 25 (2008) 114040.http://dx.doi.org/10.1088/0264-9381/25/11/114040