18+ Lise Tacizi

18+ Lise Tacizi
29 окт. 2025 г.
1 июн. 2025 г.
22 дек. 2024 г.
Zonguldak'ta, lise öğrencisi kız, internette tanıştığı adam tarafından buluştukları sırada cinsel tacize uğradı. Tehdit edildiği için susan genç kız, televizyonda cinsel istismar haberi izlerken, annesine kendi yaşadığı tacizi anlattı.
Cinsel taciz suçuna sebebiyet veren haller, soruşturma ve yargılama aşamaları, bu süreçte başvurulabilecek kanun yollarını ceza avukatımız yazdı.
10 окт. 2024 г.
ÖZET 5237 sayılı Türk Ceza Kanunu (TCK) m. 105'te cinsel taciz suçu düzenlenmiştir. Bu hükme göre bir kimseyi cinsel amaçlı olarak taciz etmek cinsel taciz suçunu oluşturur. Ancak "cinsel taciz" kavramından anlaşılması gereken ne olmalıdır? Öncelikle söz konusu durum açıklığa kavuşturulmalıdır. Çalışmada bu suçun TCK m. 105'teki kanuni düzenleniş ...
28 июн. 2024 г.
Cinsel taciz bir kimsenin bir başkasını cinsel amaçlı olarak taciz etmesi suçu için kullanılan bir kavramdır. Türk Ceza Kanunu uyarınca cinsel taciz yasal olarak suç kabul edilir ve cezai yaptırımı bulunmaktadır. Cinsel taciz suçu, TCK 105 maddesinde 2 fıkra halinde düzenlenmiştir. 1. Fıkrada suçun basit hali, 2.fıkrada ise nitelikli hali hükme bağlanmıştır ...
İZMİR TUMED on Instagram: "#Tacizi bu sözlerle savundu: Yaşını 19 sandım! İzmir'de #lise #öğrencisi D.A. (15) adlı kıza cinsel istismarda bulunduğu gerekçesiyle yargılanan taksi şoförü Umut Can Kader, (27), savunmasında kız çocuğunun yaşını 19 sandığını söyledi. D.A.'nın babası A.A. ise taksi şoförü ile kızının buluşmadan önce mesajlaştığını ...
Space-based gravitational wave detectors such as TianQin, LISA, and TaiJi have the potential to outperform themselves through joint observation. To achieve this, it is desirable to practice joint data analysis in advance on simulated data that encodes the intrinsic correlation among the signals found in different detectors that operate simultaneously. In this paper, we introduce GWSpace, a ...
We explore a potential LISA-Taiji network to fast and accurately localize the coalescing massive black hole binaries. For an equal-mass binary located at redshift of 1 with a total intrinsic mass of 105M⊙, the LISA-Taiji network may achieve almost four orders of magnitude improvement on the source localization region compared to an individual detector. The precision measurement of sky ...
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The spaceborne gravitational wave (GW) detectors LISA and TAIJI are planned to be launched in the 2030s. The dual detectors with comparable sensitivities will form a network observing GWs with significant advantages. In this work, we investigate the three possible LISA-TAIJI networks for the different location and orientation compositions of the LISA orbit ($+60\\ifmmode^\\circ\\else ...
Taiji is a gravitational-wave space facility proposed by the Chinese Academy of Sci-ences [3]. The University of the Chinese Academy of Sciences and other institutes of Chinese Academy of Sciences are involved in building it. Like LISA, Taiji is composed of a triangle of three spacecraft with a separation distance of 3 million kilometers in a heliocentric orbit ahead of the Earth by about 20 ...
12 апр. 2025 г.
'Taiji Program' is the ELISA Program proposed by ESA, and the predecessor of the ELISA Program is the LISA Program cooperated by ESA and NASA. Similar to the configuration of the three networking satellites in the LISA Program, the three satellites in the Taiji Program also rotate around their centroid. The centroid also revolves in orbit around the Sun. The difference is that the phases of ...
14 мар. 2024 г.
We explore a potential LISA-Taiji network to fast and accurately localize the coalescing massive black hole binaries. For an equal-mass binary located at redshift of 1 with a total intrinsic mass of 105M⊙, the LISA-Taiji network may achieve almost four orders ...
14 мар. 2024 г.
25 мар. 2025 г.
The space-borne gravitational wave (GW) detectors, LISA and TAIJI, are planned to be launched in the 2030s. The dual detectors with comparable sensitivities will form a network observing GW with significant advantages. In this work, we investigate the three possible LISA-TAIJI networks for the different location and orientation compositions of LISA orbit (+60 inclination and trailing the Earth ...
arXiv:2311.07116v1 [astro-ph.CO] 13 Nov 2023 The ability of Lisa, Taiji, and their networks to detect the stochastic gravitational wave background generated by Cosmic Strings
27 мар. 2025 г.
al of GW standard sirens from the Taiji-TianQin-LISA network in constraining cosmological parameters. For the optimistic scenario in which electromagnetic (EM) counterparts can be detected, we predict the number of d tectable bright sirens based on ff a constraint precision of 0.9% for the Hubble constant, meeting the standard of precision ...
INSPIRE ... INSPIRE
In the coming decades, the space-based gravitational-wave (GW) detectors such as Taiji, TianQin, and LISA are expected to form a network capable of detecting millihertz GWs emitted by the mergers of massive black hole binaries (MBHBs). In this work, we investigate the potential of GW standard sirens from the Taiji-TianQin-LISA network in constraining cosmological parameters. For the optimistic ...
y are theoretically possible [17, 18]. LISA (Laser Interferometer Space Antenna) is a space-borne gravitational wave detector scheduled for launch in the late 2030s, with a planned nominal mission duration of 4 ears, extendable to 10 years [19, 20]. TAIJI, similar to LISA, is expected
The LISA-Taiji network To the Editor — The Laser Interferometer Space Antenna (LISA), a space-based gravitational-wave observatory, was proposed in the 1990s to detect gravitational waves with ...
The simulations and analyses for LISA have shown that the confusion noise is dominant over the instrument noise around 1 mHz [25{27]. Since the detection fre-quency band of TianQin is slightly higher than that of LISA and Taiji, the e ect of the galactic confusion noise can be largely ignored for TianQin [31].
14 мар. 2024 г.
Three spacecraft of LISA/TAIJI mission follow their respective geodesic trajectories, and the arm lengths formed by the pairs of spacecraft are unequal due to solar system dynamics. Time delay interferometry is proposed to suppress the laser frequency noise raised by the unequal-arm-ness. By employing a set of numerical mission obit achieved from an ephemeris framework, we investigate the ...
The vector and scalar polarization modes of gravitational waves do not exist in General Relativity, and their detection would have signi cant impacts on fundamental physics. In this paper, we explored the detectability of these anomalous polarization modes in a gravitational wave background around 1 mHz with the future LISA-Taiji network. The inherent geometrical symmetry of the network ...
detection projects domestically, "Taiji Project" and "Tian-Qin Project", while internationally, there is the LISA project. Similar to ground-based GW detectors, if space-based detec-tors form a network, it can significantly improve the local-ization accuracy of GW sources. The prospects of the Taiji-LISA network have been carefully studied [2, 3]. Recently, Jin et al. [4] have explored ...
The joint observations by the planned space-borne gravitational wave detectors, LISA and TAIJI, will offer a unique opportunity to observe such effects in the millihertz (mHz) band. This study evaluates the detectability of parity violation in the SGWB using two network configurations: LISA-TAIJIp and LISA-TAIJIm.
14 мар. 2024 г.
24 дек. 2025 г.
In this paper, we explore the feasibility of detecting the SGWB generated by the loops arising throughout the cosmological evolution of the cosmic string network, using both individual space detectors (LISA and TAIJI) and joint space detectors (LISA-TAIJI).
Due to the precise sky localizations of MBHBs by the Taiji-TianQin-LISA network, the constraint precision of the Hubble constant is expected to reach 1.2 %. In conclusion, the GW standard sirens from the Taiji-TianQin-LISA network will play a critical role in helping solve the Hubble tension and shedding light on the nature of dark energy.
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Both LISA and Taiji, planned space-based gravitational-wave detectors in orbit around the Sun, are expected to launch in 2030-2035. Assuming a one-year overlap, we explore a potential LISA-Taiji network to fast and accurately localize the gravitational-wave sources.
In Paper I, three TAIJI orbital deployments have been proposed to compose alternative LISA-TAIJI networks: TAIJIm (leading the Earth by 20° and - 6 0 ° inclined with respect to ecliptic plane), TAIJIp (leading the Earth by 20° and + 6 0 ° inclined), TAIJIc (colocated and coplanar with LISA) with respect to the LISA mission (trailing the Earth by 20° and + 6 0 ° inclined). And the LISA ...
We explore a potential LISA-Taiji network to fast and accurately localize the coalescing massive black hole binaries. For an equal-mass binary located at redshift of 1 with a total intrinsic mass of 10 5M⊙, the LISA-Taiji network may achieve almost four orders of magnitude improvement on the source localization region compared to an individual detector. The precision measurement of sky ...
To evaluate the detection capability of the LISA-Taiji network for chiral gravitational wave background (GWB), we estimate the spectral parameters and normalized model parameters of the chiral GWB generated by early cosmic axions using the Fisher information matrix.
5 дек. 2025 г.
In this paper, we explore the possibility of detecting circular polarization of an isotropic SGWB by cross-correlating two space-based detectors planned to be launched around 2034: LISA and Taiji. We compute the response of such a network to chirality and we perform a Fisher forecast analysis on the I and V Stokes parameters for the SGWB.
AbstractThe success of LISA Pathfinder in demonstrating the LISA drag-free requirement paved the way for using space interferometers to detect low-frequency and middle-frequency gravitational waves (GWs). The TAIJI GW mission and the new LISA GW mission propose using an arm length of 3Gm (1Gm = 106km) andanarm lengthof2.5Gm respectively.Fora spacelaser-interferometricGWantenna ...
Taiji providesthebestconstraintonbothdistancesandsky locations, due the its longest arm length. LISA ranks second, while TianQin has the worst constraint. The network enhances the accuracy of the distance uncer- taintybyafactorof2−3comparedtosingledetectors.
periodic data transmissions to Earth due to the limited storage capacity of the detector or adjustments in the orientation of antenna caused by changes in the pointing direction of the spacecraft. Additionally, GW detectors are subject to data interruptions and anomalies during scientific operation as shown by datas from satellites such as LISA Pathfinder [18], Taiji-1 [19], and TianQin-1 [20 ...
Abstract. Three spacecraft of LISA/TAIJI mission follow their respective geodesic trajectories, and their interferometric arms are unequal and time-varying due to orbital dynamics. Time-delay interferometry (TDI) is proposed to suppress the laser frequency noise caused by the unequal-arm.
2 LISA-Taiji detector network and detection of chirality ption of the LISA-Taiji detector network (see, e.g., [53] and refs. therein for more details). LISA is expected to move in an heliocentric (elliptical) orbit staying 20o behind the Earth, with
yond plus and cross is an impor-tant test of general relativity. In principle, one space-borne detector, like LISA, could measure the gravitational wave po arizations from a long time observation with its orbital motion. With the comparable sensitivities, the joint LISA and TAIJI missions will improve the observations on th
Mentioning: 29 - We explore a potential LISA-Taiji network to fast and accurately localize the coalescing massive black hole binaries. For an equal-mass binary located at redshift of 1 with a total intrinsic mass of 105M⊙, the LISA-Taiji network may achieve almost four orders of magnitude improvement on the source localization region compared to an individual detector. The precision ...
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