Video wird geladen...

Video konnte nicht geladen werden

Beim Laden dieses Videos ist ein Problem aufgetreten. Dies könnte an einem vorübergehenden Netzwerkproblem liegen oder das Video ist möglicherweise nicht verfügbar.

ψ ⛧ ψ Hail satan ⛧ ψ ⛧

witchcraft

4,905 subscribers

124,602 Aufrufe • vor 3 Jahren •via X (Twitter)

Anya Rossi• Live Now

Private livecam show

5 Kommentare

Profilbild von Aerin

Aerinvor 3 Jahren

Just believe. There is no sin the blood of Jesus cannot wash

Profilbild von Alexander

Alexandervor 3 Jahren

Jesus saves. Satan steals, kills and destroys. I pray for all who are deceived by Satan. Hell is real is it's not going to be a party. Prayers and God bless.

Profilbild von ✝️ T̶o̴a̴s̸t̷e̵r̴W̴o̷l̵f̶9̸7̵🐇🇺🇲

✝️ T̶o̴a̴s̸t̷e̵r̴W̴o̷l̵f̶9̸7̵🐇🇺🇲vor 3 Jahren

How's 7th grade Timmy?

Profilbild von 🍵

🍵vor 3 Jahren

Willingly acknowledging evil and choosing to follow its path is extremely miserable and pathetic. I hope you find God, you're very lost. Focus on your studies btw, you sound very young and immature.

Profilbild von Smol Mike

Smol Mikevor 3 Jahren

Nah he ain’t shit. He throwin a piss fit before he gets what’s comin

Ähnliche Videos

◤ ◥ 𝕄𝕖𝕣𝕣𝕪 ℂ𝕙𝕣𝕚𝕤𝕥𝕞𝕒𝕤 Ψ・ω・Ψ ◣ ◢

◤ ◥ 𝕄𝕖𝕣𝕣𝕪 ℂ𝕙𝕣𝕚𝕤𝕥𝕞𝕒𝕤 Ψ・ω・Ψ ◣ ◢

Sena🏹ASMR

14,708 Aufrufe • vor 9 Monaten

⛧ D̴e̶m̷o̸n̷ ̴m̸a̷x̴i̷m̷a̶l̸i̶s̴t̶ ̴ ⛧

Sensitive content

⛧ D̴e̶m̷o̸n̷ ̴m̸a̷x̴i̷m̷a̶l̸i̶s̴t̶ ̴ ⛧

Trench Demons

49,793 Aufrufe • vor 1 Jahr

⛧──── ⋆⋅☆⋅⋆ ───⛧ 𝟚𝟘𝟚𝟞.𝟘𝟚.𝟘𝟝 『STGL LAND』 * ੈ✩‧₊ 𝕕𝕚𝕘𝕖𝕤𝕥 !! ⛧──── ⋆⋅☆⋅⋆ ───⛧

⛧──── ⋆⋅☆⋅⋆ ───⛧ 𝟚𝟘𝟚𝟞.𝟘𝟚.𝟘𝟝 『STGL LAND』 * ੈ✩‧₊ 𝕕𝕚𝕘𝕖𝕤𝕥 !! ⛧──── ⋆⋅☆⋅⋆ ───⛧

ストロボグリッター

15,663 Aufrufe • vor 8 Monaten

おはよーψ(｀∇´)ψ

おはよーψ(｀∇´)ψ

トニー大木

20,904 Aufrufe • vor 1 Monat

。 ♥ 。 †⛧ ♰.˚ ⛧+ ＼｜／。 ⛧ 눈 마주쳤지 - #밤비 ♰。／｜＼ + +。。 ♥

。 ♥ 。 †⛧ ♰.˚ ⛧+ ＼｜／。 ⛧ 눈 마주쳤지 - #밤비 ♰。／｜＼ + +。。 ♥

밤2

26,121 Aufrufe • vor 6 Tagen

⛧Española 🇪🇸 ⛧Music & game addicted ⛧Valorant/Lol player ⛧Recomienden animes ✩ ⛧Vivo de noche ⛧Chronically online, socially exhausted 🖤 ♡ & ↻ to be moots #nsfw #nsfwtwt #horny #esex #femalemoan #audio

Sensitive content

⛧Española 🇪🇸 ⛧Music & game addicted ⛧Valorant/Lol player ⛧Recomienden animes ✩ ⛧Vivo de noche ⛧Chronically online, socially exhausted 🖤 ♡ & ↻ to be moots #nsfw #nsfwtwt #horny #esex #femalemoan #audio

♰ SweetGhoul ♰

14,197 Aufrufe • vor 4 Monaten

₊˚♪ 𝄞𝄢₊˚⊹⋆˖⁺‧₊☽◯☾₊‧⁺˖⋆‧₊˚♪ 𝄞𝄢₊˚ ⁺‧₊˚ ཐི⋆♱ ˚₊‧⁺ ˚₊‧꒰ა ⛧°。 ⋆༺♱༻⋆。°⛧ ໒꒱ ‧₊˚

₊˚♪ 𝄞𝄢₊˚⊹⋆˖⁺‧₊☽◯☾₊‧⁺˖⋆‧₊˚♪ 𝄞𝄢₊˚ ⁺‧₊˚ ཐི⋆♱ ˚₊‧⁺ ˚₊‧꒰ა ⛧°。 ⋆༺♱༻⋆。°⛧ ໒꒱ ‧₊˚

bemboo ★ XDZ=6 🦔 mutiwhore 愛

23,276 Aufrufe • vor 4 Monaten

⛧°｡⋆ 𝐖𝐞𝐥𝐜𝐨𝐦𝐞 𝐭𝐨 𝐦𝐲 𝐚𝐜𝐜𝐨𝐮𝐧𝐭 ⋆｡°⛧

⛧°｡⋆ 𝐖𝐞𝐥𝐜𝐨𝐦𝐞 𝐭𝐨 𝐦𝐲 𝐚𝐜𝐜𝐨𝐮𝐧𝐭 ⋆｡°⛧

𓆰No𝜶hx🐥𓆪

15,043 Aufrufe • vor 1 Jahr

Why Does Quantum Mechanics Use a Complex Wavefunction? Schrödinger’s equation doesn’t start from mystery. It starts from a very specific bet. The state of a particle is a complex field ψ(x,t), and whatever time-evolution rule we choose has to move ψ forward while preserving total probability. So the basic question is simple. What equation should ψ satisfy so that |ψ|² behaves like a conserved density, the way mass density does in fluid flow? What is ψ? Think of ψ(x,t) as an amplitude attached to the statement the particle is at position x at time t. It’s not a probability. It’s the thing you add first, and only at the end do you square it: p(x,t) = |ψ(x,t)|² Because ψ is complex, it has magnitude and phase. Write it as ψ(x,t) = r(x,t) exp(i θ(x,t)) Then r² = |ψ|² is the density, and the phase θ ends up controlling the flow through the probability current. Where does Schrödinger’s equation come from? Start with two empirical inputs that tie waves to particles: E = ħ ω p = ħ k Here ħ is Planck’s constant divided by 2π. It’s the conversion factor between frequency and energy, and between wavenumber and momentum. A plane wave with angular frequency ω and wavevector k is ψ(x,t) = A exp(i(k·x − ωt)) Now watch what derivatives do to this wave: ∂ψ/∂t = −i ω ψ ∇ψ = i k ψ ∇²ψ = −|k|² ψ Multiply by ħ and you get: i ħ ∂ψ/∂t = ħ ω ψ = E ψ −i ħ ∇ψ = ħ k ψ = p ψ −ħ² ∇²ψ = ħ² |k|² ψ = p² ψ So for plane waves, the operators Ê = i ħ ∂/∂t p̂ = −i ħ ∇ act like energy and momentum. Now bring in the classical, nonrelativistic energy bookkeeping: E = p²/(2m) + V(x) Kinetic plus potential. That’s it. Turn it into an equation for ψ by replacing E and p with the operators above: Ê ψ = (p̂²/(2m) + V) ψ Since p̂² = (−i ħ ∇)·(−i ħ ∇) = −ħ² ∇², this becomes i ħ ∂ψ/∂t = ( −ħ²/(2m) ∇² + V(x) ) ψ That’s the time-dependent Schrödinger equation. This derivation is a controlled heuristic. Match the plane-wave identities to the measured relations E = ħω and p = ħk, then impose the same energy bookkeeping you trust in classical mechanics. Why this is the right kind of rule If ψ is the state, we need a rule that preserves total probability: ∫ |ψ(x,t)|² dx = 1 Schrödinger evolution does, and you can see it by deriving a continuity equation. Let ρ(x,t) = |ψ|² = ψ*ψ. Differentiate: ∂ρ/∂t = ψ* ∂ψ/∂t + ψ ∂ψ*/∂t Use Schrödinger and its complex conjugate. The potential terms cancel, and what’s left can be rearranged into ∂ρ/∂t + ∇·j = 0 with probability current j = (ħ/(2mi)) ( ψ* ∇ψ − ψ ∇ψ* ) That’s the cleanest way to say what ψ is. |ψ|² behaves like a conserved density, the phase drives a current, and the time evolution is fixed, up to V, by combining wave relations with energy bookkeeping: i ħ ∂ψ/∂t = ( −ħ²/(2m) ∇² + V ) ψ #QuantumMechanics #SchrodingerEquation #WaveFunction #BornRule #Physics #MathematicalPhysics

Why Does Quantum Mechanics Use a Complex Wavefunction? Schrödinger’s equation doesn’t start from mystery. It starts from a very specific bet. The state of a particle is a complex field ψ(x,t), and whatever time-evolution rule we choose has to move ψ forward while preserving total probability. So the basic question is simple. What equation should ψ satisfy so that |ψ|² behaves like a conserved density, the way mass density does in fluid flow? What is ψ? Think of ψ(x,t) as an amplitude attached to the statement the particle is at position x at time t. It’s not a probability. It’s the thing you add first, and only at the end do you square it: p(x,t) = |ψ(x,t)|² Because ψ is complex, it has magnitude and phase. Write it as ψ(x,t) = r(x,t) exp(i θ(x,t)) Then r² = |ψ|² is the density, and the phase θ ends up controlling the flow through the probability current. Where does Schrödinger’s equation come from? Start with two empirical inputs that tie waves to particles: E = ħ ω p = ħ k Here ħ is Planck’s constant divided by 2π. It’s the conversion factor between frequency and energy, and between wavenumber and momentum. A plane wave with angular frequency ω and wavevector k is ψ(x,t) = A exp(i(k·x − ωt)) Now watch what derivatives do to this wave: ∂ψ/∂t = −i ω ψ ∇ψ = i k ψ ∇²ψ = −|k|² ψ Multiply by ħ and you get: i ħ ∂ψ/∂t = ħ ω ψ = E ψ −i ħ ∇ψ = ħ k ψ = p ψ −ħ² ∇²ψ = ħ² |k|² ψ = p² ψ So for plane waves, the operators Ê = i ħ ∂/∂t p̂ = −i ħ ∇ act like energy and momentum. Now bring in the classical, nonrelativistic energy bookkeeping: E = p²/(2m) + V(x) Kinetic plus potential. That’s it. Turn it into an equation for ψ by replacing E and p with the operators above: Ê ψ = (p̂²/(2m) + V) ψ Since p̂² = (−i ħ ∇)·(−i ħ ∇) = −ħ² ∇², this becomes i ħ ∂ψ/∂t = ( −ħ²/(2m) ∇² + V(x) ) ψ That’s the time-dependent Schrödinger equation. This derivation is a controlled heuristic. Match the plane-wave identities to the measured relations E = ħω and p = ħk, then impose the same energy bookkeeping you trust in classical mechanics. Why this is the right kind of rule If ψ is the state, we need a rule that preserves total probability: ∫ |ψ(x,t)|² dx = 1 Schrödinger evolution does, and you can see it by deriving a continuity equation. Let ρ(x,t) = |ψ|² = ψψ. Differentiate: ∂ρ/∂t = ψ ∂ψ/∂t + ψ ∂ψ/∂t Use Schrödinger and its complex conjugate. The potential terms cancel, and what’s left can be rearranged into ∂ρ/∂t + ∇·j = 0 with probability current j = (ħ/(2mi)) ( ψ ∇ψ − ψ ∇ψ* ) That’s the cleanest way to say what ψ is. |ψ|² behaves like a conserved density, the phase drives a current, and the time evolution is fixed, up to V, by combining wave relations with energy bookkeeping: i ħ ∂ψ/∂t = ( −ħ²/(2m) ∇² + V ) ψ #QuantumMechanics #SchrodingerEquation #WaveFunction #BornRule #Physics #MathematicalPhysics

Mathelirium

20,911 Aufrufe • vor 8 Monaten

I love it when. Tyranny TRex 🜏⛧ ℭ𝔥𝔢𝔳𝔢𝔩𝔩𝔢 ⛧🜏

Sensitive content

I love it when. Tyranny TRex 🜏⛧ ℭ𝔥𝔢𝔳𝔢𝔩𝔩𝔢 ⛧🜏

Shenanigans

39,083 Aufrufe • vor 11 Monaten

lu 🇦🇷°⛧° ｡ﾟ･ ˘ᵌ˘ * °⛧｡ﾟ･° ⛧ Here is a FULL tutorial on How to Record and Mass-Produce Songs on Vinyl Records

lu 🇦🇷°⛧° ｡ﾟ･ ˘ᵌ˘ * °⛧｡ﾟ･° ⛧ Here is a FULL tutorial on How to Record and Mass-Produce Songs on Vinyl Records

່

172,381 Aufrufe • vor 1 Jahr

Lecture 2 on our Quantum Mechanics Series Schrödinger’s equation doesn’t start from mystery. It starts from a very specific bet…the state of a particle is a complex field ψ(x,t), and whatever dynamics we write down must move ψ forward in time in a way that preserves total probability. We ask a basic question…what equation should ψ satisfy so that |ψ|² behaves like a conserved density, the way mass density does in fluid flow? What is ψ? Think of ψ(x,t) as the amplitude assigned to “the particle is at position x at time t”. It’s not a probability. It’s the object you add first, and only at the end do you square p(x,t) = |ψ(x,t)|² Because ψ is complex, it has magnitude and phase. Write it in polar form ψ(x,t) = r(x,t) exp(i θ(x,t)) Then r² = |ψ|² is the density, and θ will end up controlling flow (the probability current). Where does Schrödinger’s equation come from? Start with two empirical inputs about waves and particles: E = ħ ω p = ħ k Here ħ (“h-bar”) is Planck’s constant divided by 2π. It’s the unit conversion factor between the wave description (frequency ω, wavevector k) and the particle description (energy E, momentum p). In units, ħ has units of joule-seconds, so multiplying ω (1/seconds) gives energy (joules), and multiplying k (1/meters) gives momentum (kg·m/s). It’s the number that tells you how much energy or momentum you get per unit frequency or wavenumber. A plane wave with angular frequency ω and wavevector k is ψ(x,t) = A exp(i(k·x − ω t)) Now notice what derivatives do to this wave: ∂ψ/∂t = −i ω ψ ∇ψ = i k ψ ∇²ψ = −|k|² ψ Multiply those identities by ħ: i ħ ∂ψ/∂t = ħ ω ψ = E ψ −i ħ ∇ψ = ħ k ψ = p ψ −ħ² ∇²ψ = ħ² |k|² ψ = p² ψ So for plane waves, the operators Ê = i ħ ∂/∂t p̂ = −i ħ ∇ act like energy and momentum! Now use the classical nonrelativistic energy relation: E = p²/(2m) + V(x) This is bookkeeping for a particle moving slow enough that relativity can be ignored. The term p²/(2m) is kinetic energy. If p = mv, then p²/(2m) = (m²v²)/(2m) = (1/2)mv². The term V(x) is potential energy. It depends on position because forces come from spatially varying energy. A slope in V pushes the particle. Examples: for a charged particle in an electric potential φ(x), V(x) = q φ(x). Near Earth, V(z) = mgz. The point is total energy equals kinetic plus potential. Turn that into an equation for ψ by replacing E and p with the operators above: Ê ψ = (p̂²/(2m) + V) ψ Compute p̂² = (−i ħ ∇)·(−i ħ ∇) = −ħ² ∇², so we get i ħ ∂ψ/∂t = ( −ħ²/(2m) ∇² + V(x) ) ψ That is the time-dependent Schrödinger equation. The derivation here is a controlled heuristic: we matched the plane-wave identities to the measured relations E = ħω and p = ħk, then imposed the same energy bookkeeping as classical mechanics. Why this equation is the right kind of rule If ψ is the state, we need a rule that preserves total probability: ∫ |ψ(x,t)|² dx = 1 Schrödinger evolution does. You can see it by deriving a continuity equation. Let ρ(x,t) = |ψ|² = ψ* ψ. Take a time derivative: ∂ρ/∂t = ψ* ∂ψ/∂t + ψ ∂ψ*/∂t Use Schrödinger and its complex conjugate: ∂ψ/∂t = (1/(i ħ)) ( −ħ²/(2m) ∇²ψ + Vψ ) ∂ψ*/∂t = (−1/(i ħ)) ( −ħ²/(2m) ∇²ψ* + Vψ* ) Plug in. The V terms cancel exactly, and what remains can be rearranged into a divergence: ∂ρ/∂t + ∇·j = 0 where the probability current is j = (ħ/(2mi)) ( ψ* ∇ψ − ψ ∇ψ* ) This is the best way to explain ehat ψ is: |ψ|² behaves like a conserved density, and the phase of ψ is what drives the current j. So in this series, ψ isn’t a slogan. It’s the object whose modulus squared is the density, whose phase generates flow, and whose time evolution is fixed (up to V) by matching wave relations to energy bookkeeping: i ħ ∂ψ/∂t = ( -ħ²/(2m) ∇² + V ) ψ #QuantumMechanics #SchrodingerEquation #WaveFunction #BornRule #Physics #MathematicalPhysics

Lecture 2 on our Quantum Mechanics Series Schrödinger’s equation doesn’t start from mystery. It starts from a very specific bet…the state of a particle is a complex field ψ(x,t), and whatever dynamics we write down must move ψ forward in time in a way that preserves total probability. We ask a basic question…what equation should ψ satisfy so that |ψ|² behaves like a conserved density, the way mass density does in fluid flow? What is ψ? Think of ψ(x,t) as the amplitude assigned to “the particle is at position x at time t”. It’s not a probability. It’s the object you add first, and only at the end do you square p(x,t) = |ψ(x,t)|² Because ψ is complex, it has magnitude and phase. Write it in polar form ψ(x,t) = r(x,t) exp(i θ(x,t)) Then r² = |ψ|² is the density, and θ will end up controlling flow (the probability current). Where does Schrödinger’s equation come from? Start with two empirical inputs about waves and particles: E = ħ ω p = ħ k Here ħ (“h-bar”) is Planck’s constant divided by 2π. It’s the unit conversion factor between the wave description (frequency ω, wavevector k) and the particle description (energy E, momentum p). In units, ħ has units of joule-seconds, so multiplying ω (1/seconds) gives energy (joules), and multiplying k (1/meters) gives momentum (kg·m/s). It’s the number that tells you how much energy or momentum you get per unit frequency or wavenumber. A plane wave with angular frequency ω and wavevector k is ψ(x,t) = A exp(i(k·x − ω t)) Now notice what derivatives do to this wave: ∂ψ/∂t = −i ω ψ ∇ψ = i k ψ ∇²ψ = −|k|² ψ Multiply those identities by ħ: i ħ ∂ψ/∂t = ħ ω ψ = E ψ −i ħ ∇ψ = ħ k ψ = p ψ −ħ² ∇²ψ = ħ² |k|² ψ = p² ψ So for plane waves, the operators Ê = i ħ ∂/∂t p̂ = −i ħ ∇ act like energy and momentum! Now use the classical nonrelativistic energy relation: E = p²/(2m) + V(x) This is bookkeeping for a particle moving slow enough that relativity can be ignored. The term p²/(2m) is kinetic energy. If p = mv, then p²/(2m) = (m²v²)/(2m) = (1/2)mv². The term V(x) is potential energy. It depends on position because forces come from spatially varying energy. A slope in V pushes the particle. Examples: for a charged particle in an electric potential φ(x), V(x) = q φ(x). Near Earth, V(z) = mgz. The point is total energy equals kinetic plus potential. Turn that into an equation for ψ by replacing E and p with the operators above: Ê ψ = (p̂²/(2m) + V) ψ Compute p̂² = (−i ħ ∇)·(−i ħ ∇) = −ħ² ∇², so we get i ħ ∂ψ/∂t = ( −ħ²/(2m) ∇² + V(x) ) ψ That is the time-dependent Schrödinger equation. The derivation here is a controlled heuristic: we matched the plane-wave identities to the measured relations E = ħω and p = ħk, then imposed the same energy bookkeeping as classical mechanics. Why this equation is the right kind of rule If ψ is the state, we need a rule that preserves total probability: ∫ |ψ(x,t)|² dx = 1 Schrödinger evolution does. You can see it by deriving a continuity equation. Let ρ(x,t) = |ψ|² = ψ* ψ. Take a time derivative: ∂ρ/∂t = ψ* ∂ψ/∂t + ψ ∂ψ/∂t Use Schrödinger and its complex conjugate: ∂ψ/∂t = (1/(i ħ)) ( −ħ²/(2m) ∇²ψ + Vψ ) ∂ψ/∂t = (−1/(i ħ)) ( −ħ²/(2m) ∇²ψ* + Vψ* ) Plug in. The V terms cancel exactly, and what remains can be rearranged into a divergence: ∂ρ/∂t + ∇·j = 0 where the probability current is j = (ħ/(2mi)) ( ψ* ∇ψ − ψ ∇ψ* ) This is the best way to explain ehat ψ is: |ψ|² behaves like a conserved density, and the phase of ψ is what drives the current j. So in this series, ψ isn’t a slogan. It’s the object whose modulus squared is the density, whose phase generates flow, and whose time evolution is fixed (up to V) by matching wave relations to energy bookkeeping: i ħ ∂ψ/∂t = ( -ħ²/(2m) ∇² + V ) ψ #QuantumMechanics #SchrodingerEquation #WaveFunction #BornRule #Physics #MathematicalPhysics

Mathelirium

40,978 Aufrufe • vor 9 Monaten

🔴 URGENTE ⛈️ Sigue la lluvia torrencial en la Región Metropolitana: Se registran inundaciones repentinas (Flash Floods) en Avenida Nueva Providencia y Ricardo Lyon en Providencia 📷 ⛧ENVTUBER⛧ Joe Kerr ⛧𝓔𝓻𝓪 𝓥𝓾𝓵𝓰𝓪𝓻𝓲𝓼⛧🤘😈

🔴 URGENTE ⛈️ Sigue la lluvia torrencial en la Región Metropolitana: Se registran inundaciones repentinas (Flash Floods) en Avenida Nueva Providencia y Ricardo Lyon en Providencia 📷 ⛧ENVTUBER⛧ Joe Kerr ⛧𝓔𝓻𝓪 𝓥𝓾𝓵𝓰𝓪𝓻𝓲𝓼⛧🤘😈

El Hilo Chileno BORA LULA 🇨🇱💚🇧🇷👊

25,051 Aufrufe • vor 18 Stunden

畳み終わると… 現れる悪魔ψ(⃔ ॑꒳ ॑*)⃕ψ↝ちゃん

畳み終わると… 現れる悪魔ψ(⃔ ॑꒳ ॑*)⃕ψ↝ちゃん

ほんわか姉妹(主)

44,894 Aufrufe • vor 3 Monaten

✶ ⛧ ✫ ⋆⁺₊⋆ 🔗 #EVNNE #이븐 #이정현 #LEEJEONGHYEON

✶ ⛧ ✫ ⋆⁺₊⋆ 🔗 #EVNNE #이븐 #이정현 #LEEJEONGHYEON

EVNNE

49,898 Aufrufe • vor 1 Jahr

#cosplay #zzzero #绝区零 #简杜 #絕區零完整版来啦ψ(｀∇´)ψ

#cosplay #zzzero #绝区零 #简杜 #絕區零完整版来啦ψ(｀∇´)ψ

柠好不好

392,065 Aufrufe • vor 2 Jahren