二重パルサーとのVLBI距離の影響 J0737-3039A/B/B2パルサーとのVLBI距離の影響 J0737-3039A/B2パルサーとのVLBI距離の影響 J0737-3039A/B2パルサーとのVLBI距離の影響
A T Deller1, M Bailes, S J Tingay
1Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Mail H39, Post Office Box 218, Hawthorn, VIC 3122, Australia. adeller@astro.swin.edu.au
まとめ
二重パルサーJ0737-3039A/Bの正確な距離と運動測定は,VLBIを用いて得られた. これは重力理論の非常に正確なテストを可能にし,重力放射線のモデルを制限します.
科学分野:
- 天文学と天体物理学について
- 重力物理学 重力物理学
背景:
- ダブルパルサーJ0737-3039A/Bは,強いフィールド重力のテストに不可欠です.
- 正確な距離と相対運動データは,正確な重力テストに不可欠です.
研究 の 目的:
- ダブルパルサーシステムの正確な距離と横断速度を決定するために.
- パルサー・タイミングデータを用いて重力理論のテストの精度を高めること.
主な方法:
- 非常に長いベースラインインターフェロメトリー (VLBI) の観測が採用されました.
- パルサーのタイミングデータから,10年分のデータを利用した.
主要な成果:
- PSR J0737-3039A/Bまでの距離は,1150〜160〜+220パーセックスと決定されました.
- 約9km/sの低い横断速度が確認されました.
- これらの測定は,以前の推定値よりも大幅に改善しています.
結論:
- 精製されたデータは,重力放射線放射理論の0.01%の不確実性レベルのテストを可能にします.
- 二極重力放射線を予測する理論には厳しい制約が課せられる.
- システムの形成と高エネルギー排出源に関する新しい洞察が提供されています.
関連する概念動画
Doppler Effect - II
The Doppler effect has several practical, real-world applications. For instance, meteorologists use Doppler radars to interpret weather events based on the Doppler effect. Typically, a transmitter emits radio waves at a specific frequency toward the sky from a weather station. The radio waves bounce off the clouds and precipitation and travel back to the weather station. The radio frequency of the waves reflected back to the station appears to decrease if the clouds or precipitation are moving...
Schwarzschild Radius and Event Horizon
No object with a finite mass can travel faster than the speed of light in a vacuum. This fact has an interesting consequence in the domain of extremely high gravitational fields.
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape velocity with the...
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape velocity with the...
Detection of Black Holes
Although black holes were theoretically postulated in the 1920s, they remained outside the domain of observational astronomy until the 1970s.
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
Distance Problem
When an object's velocity changes over time, the total distance traveled can be determined by summing small displacement intervals over short increments. This approach approximates the true distance through numerical summation and the use of integral calculus. An estimate of the total displacement can be obtained by measuring velocity at regular intervals and multiplying each value by the corresponding time step.If a runner accelerates over the first three seconds of a race, speed measurements...
Doppler Effect - I
The Doppler effect and Doppler shift were named after the Austrian physicist and mathematician Christian Johann Doppler in 1842, who conducted experiments with both moving sources and moving observers. Consider an observer standing on a street corner, observing an ambulance with a siren sound passing by at a constant speed. The observer experiences two characteristic changes in the sound of the siren. Initially, the sound increases in loudness as the ambulance approaches and decreases in...
Gravitation Between Spherically Symmetric Masses
The gravitational potential energy between two spherically symmetric bodies can be calculated from the masses and the distance between the bodies, assuming that the center of mass is concentrated at the respective centers of the bodies.

