Peppa 1000001 Piggy Sonic Roblox Part 2
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SONIC Y CHUCKY:
/ @sonicychucky
SONIC AND CHUCKY PLAY:
/ channel
VIDEOS DE:
/ @robloxanimationsshort...
PLAYING WITH SUBS:
/ @gorangerman
BUSINESS MAIL: gpopspider@gmail.com
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😂
Vuen video bro que sigas así
SONIC
Like
🔃
Mm
Sonic
Yuju
sd
T
I like sonic y chucky
W
You like being weird
Me too 😱😍
Y
Son videos violentos y los niños quieren hacer lo mismo son sus hermanos. No deberíamos permitir estos tipos de videos xq son malos para nuestros hijos/as.
𝕖𝕩𝕒𝕔𝕥𝕒𝕞𝕖𝕟𝕥𝕖
Rws
I LOOOVE YOU SONIC Y CHUCKY 😘😘😘😍😍🥰🥰
Dude literally says his videos are over 13 but what kind of people over 13 would wanna watch this?
It’s so the channel can’t get in trouble 😐
Uik
ーーーーーーーーーーーーーー
sonic i cuky
9
L un ok un gol ok
YES QUEEN
Rhj
Peppa 1000001 Piggy Sonic Roblox Part 2
D só u y
E
Funny video
Holi me encantan sus videos son los maximo👏👏
Kehygasgeyweggege2f🥳😐😙👩😇🧅🥕
Fxa
😍😍
In,
H4
SONIC Y CHUCKY
0
I’m scared
Iiugfew
The Titanic is fun
Jjmggm
Jggjm
II÷
I.
Jggjgg II
Five Nights At Freddy's Vs Friday Night Funkin', Peppa
. .... ..,
BALLON PIGGY
ZiK
NO
Bbbb
Cartoon cat ys peppa
Not bad:)
First again
Congratulations
Congratulations friend!!!!
@@GoranGerman g/
@@GoranGerman u
@@GoranGerman uy g
!
88iiiu78
The Unruh effect (also known as the Fulling-Davies-Unruh effect) is a kinematic prediction of quantum field theory that an accelerating observer will observe a thermal bath, like blackbody radiation, whereas an inertial observer would observe none. In other words, the background appears to be warm from an accelerating reference frame; in layman's terms, an accelerating thermometer (like one being waved around) in empty space, removing any other contribution to its temperature, will record a non-zero temperature, just from its acceleration. Heuristically, for a uniformly accelerating observer, the ground state of an inertial observer is seen as a mixed state in thermodynamic equilibrium with a non-zero temperature bath. The Unruh effect was first described by Stephen Fulling in 1973, Paul Davies in 1975 and W. G. Unruh in 1976. It is currently not clear whether the Unruh effect has actually been observed, since the claimed observations are disputed. There is also some doubt about whether the Unruh effect implies the existence of Unruh radiation. Unruh demonstrated theoretically that the notion of vacuum depends on the path of the observer through spacetime. From the viewpoint of the accelerating observer, the vacuum of the inertial observer will look like a state containing many particles in thermal equilibrium-a warm gas. The Unruh effect would only appear to an accelerating observer. And although the Unruh effect would initially be perceived as counter-intuitive, it makes sense if the word vacuum is interpreted in the following specific way. In quantum field theory, the concept of "vacuum" is not the same as "empty space": Space is filled with the quantized fields that make up the universe. Vacuum is simply the lowest possible energy state of these fields. The energy states of any quantized field are defined by the Hamiltonian, based on local conditions, including the time coordinate. According to special relativity, two observers moving relative to each other must use different time coordinates. If those observers are accelerating, there may be no shared coordinate system. Hence, the observers will see different quantum states and thus different vacua. In some cases, the vacuum of one observer is not even in the space of quantum states of the other. In technical terms, this comes about because the two vacua lead to unitarily inequivalent representations of the quantum field canonical commutation relations. This is because two mutually accelerating observers may not be able to find a globally defined coordinate transformation relating their coordinate choices. An accelerating observer will perceive an apparent event horizon forming. The existence of Unruh radiation could be linked to this apparent event horizon, putting it in the same conceptual framework as Hawking radiation. On the other hand, the theory of the Unruh effect explains that the definition of what constitutes a "particle" depends on the state of motion of the observer. The free field needs to be decomposed into positive and negative frequency components before defining the creation and annihilation operators. This can only be done in spacetimes with a timelike Killing vector field. This decomposition happens to be different in Cartesian and Rindler coordinates (although the two are related by a Bogoliubov transformation). This explains why the "particle numbers", which are defined in terms of the creation and annihilation operators, are different in both coordinates. The Rindler spacetime has a horizon, and locally any non-extremal black hole horizon is Rindler. So the Rindler spacetime gives the local properties of black holes and cosmological horizons. It is possible to rearrange the metric restricted to these regions to obtain the Rinder metric. The Unruh effect would then be the near-horizon form of Hawking radiation. The Unruh effect is also expected to be present in de Sitter space. It is worth stressing that the Unruh effect only says that, according to uniformly-accelerated observers, the vacuum state is a thermal state specified by its temperature, and one should resist reading too much into the thermal state or bath. Different thermal states or baths at the same temperature need not be equal, for they depend on the Hamiltonian describing the system. In particular, the thermal bath seen by accelerated observers in the vacuum state of a quantum field is not the same as a thermal state of the same field at the same temperature according to inertial observers. Furthermore, uniformly accelerated observers, static with respect to each other, can have different proper accelerations a (depending on their separation), which is a direct consequence of relativistic red-shift effects. This makes the Unruh temperature spatially inhomogeneous across the uniformly accelerated frame. In special relativity, an observer moving with uniform proper acceleration a through Minkowski spacetime is conveniently described with Rindler coordinates.
😔
Cho tôi biết rồi nhưng chưa thấy Cho em một ☝️ của em có thể làm được gì hết mem em có 👍 thôi em đi đâu chơi à em
11-
😊
Aw
1❤😂🎉😢😮😅😊❤😂🎉😢😮😅😊😊❤😂⅔
Eagu
b a l l o o n s
Uny
All the money that this dude is making is going straight to therapy
Варит? Lkklmkmmmlkkааппритттттт
p😮
Yeah probaly for him
what in gods green and blue world is this
Ddsw8qlslkgbi
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@@liliiane aa
IDK Man
Ddrt
So this is inflation
Ol
7uuuu7uii
Ahahahh
@SONIC Y CHUCKY What program did you use for making Animations? Please give me the program name :)
Ppp
9
@@JuanCarlos-bn5qh ?
@@mehmetruzgar5485 ?
@@JuanCarlos-bn5qh zpllp
Where is the iceberg the titanic
Based
The information contained in
oh my god what in the world is this
X 5m
Cringe
V
😂
Funny video
Ufff 😮🤗🤗😊😊🤗🤗🤗🤗🤗🤗🤗😮😮🤐
🇧🇩🇧🇩🇧🇩
@@enerofebrero2582 9
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Peppa 1000001 Piggy Sonic Roblox Part 2