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Phantom

The Phantom Smoothed Particle Hydrodynamics code

About

Phantom is a 3D Smoothed Particle Hydrodynamics and Magnetohydrodynamics code for astrophysics. It was written and developed by Daniel Price with contributions from many others (see AUTHORS). It is designed to be a fast 3D SPH code with a low memory footprint, for production runs. It is not a code for testing algorithms (use NDSPMHD instead).

Status

buildtestmpimcfostDocumentation

Links

Code structure

The Phantom source code is structured as follows:

build/Makefilemain Makefile for compiling Phantom and all utilities
src/mainsource for main code
src/setupsource for Phantomsetup utility
src/testssource for unit tests and the Phantom testsuite
src/utilssource for optional utilities and analysis

Getting help

If you need help, please try the following, in order:

  1. Check the documentation.
  2. If you encounter a bug, file an issue
  3. If you want to request a feature, start a discussion
  4. If you need help on how to use phantom, start a discussion

We welcome general discussion about Phantom, Smoothed Particle Hydrodynamics, and astrophysics at the Phantom Slack. However, please use the github issues for support requests.

Contributing

We welcome contributions, including (but not limited to):

  1. Code, via pull request. Please read developer section of user guide for guidelines.
  2. Documentation, also by pull request. Docs can be edited in the docs/ directory of the main code.
  3. Suggestions for features or bug reports, via the issue tracker. Please file bugs via github rather than by email.

Citation

Please cite Price et al. (2018) when using Phantom. Wherever possible, please try to also cite original references for the algorithms you are using. A partial list can be found in docs/phantom.bib file, or by reading the relevant sections of the paper.

Other things

For CHANGES see the release notes: https://phantomsph.readthedocs.io/en/latest/releasenotes.html. See LICENCE file for usage and distribution conditions.

Copyright (c) 2007-2025 Daniel Price and contributors (see AUTHORS file).

About

Phantom Smoothed Particle Hydrodynamics and Magnetohydrodynamics code

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0 stars

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0 watching

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, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Add copy buttons to all
 blocks\n(function() {\n function addCopyButtons() {\n document.querySelectorAll('pre code').forEach(function(codeBlock) {\n if (codeBlock.parentElement.hasAttribute('data-copy-added')) return;\n codeBlock.parentElement.setAttribute('data-copy-added', 'true');\n \n var btn = document.createElement('button');\n btn.textContent = 'Copy';\n btn.style.cssText = 'position:absolute;top:4px;right:4px;padding:2px 8px;font-size:11px;background:#4ecdc4;border:none;border-radius:4px;color:#1a1a2e;cursor:pointer;opacity:0.7;transition:opacity 0.2s;';\n btn.onmouseover = function() { this.style.opacity = '1'; };\n btn.onmouseout = function() { this.style.opacity = '0.7'; };\n btn.onclick = function() {\n navigator.clipboard.writeText(codeBlock.textContent).then(function() {\n btn.textContent = 'Copied!';\n setTimeout(function() { btn.textContent = 'Copy'; }, 1500);\n });\n };\n codeBlock.parentElement.style.position = 'relative';\n codeBlock.parentElement.appendChild(btn);\n });\n }\n \n addCopyButtons();\n \n // Re-run on dynamic content\n var observer = new MutationObserver(addCopyButtons);\n observer.observe(document.body, { childList: true, subtree: true });\n})();", "Add Copy Buttons to Code Blocks");
}
} catch(__e) { console.warn('[Userscript:Add Copy Buttons to Code Blocks]', __e); }
})();
(function(){
try {
var __m = "github.com";
var __re = new RegExp('^' + "github\\.com" + '
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Repository files navigation

Phantom

The Phantom Smoothed Particle Hydrodynamics code

About

Phantom is a 3D Smoothed Particle Hydrodynamics and Magnetohydrodynamics code for astrophysics. It was written and developed by Daniel Price with contributions from many others (see AUTHORS). It is designed to be a fast 3D SPH code with a low memory footprint, for production runs. It is not a code for testing algorithms (use NDSPMHD instead).

Status

buildtestmpimcfostDocumentation

Links

Code structure

The Phantom source code is structured as follows:

build/Makefilemain Makefile for compiling Phantom and all utilities
src/mainsource for main code
src/setupsource for Phantomsetup utility
src/testssource for unit tests and the Phantom testsuite
src/utilssource for optional utilities and analysis

Getting help

If you need help, please try the following, in order:

  1. Check the documentation.
  2. If you encounter a bug, file an issue
  3. If you want to request a feature, start a discussion
  4. If you need help on how to use phantom, start a discussion

We welcome general discussion about Phantom, Smoothed Particle Hydrodynamics, and astrophysics at the Phantom Slack. However, please use the github issues for support requests.

Contributing

We welcome contributions, including (but not limited to):

  1. Code, via pull request. Please read developer section of user guide for guidelines.
  2. Documentation, also by pull request. Docs can be edited in the docs/ directory of the main code.
  3. Suggestions for features or bug reports, via the issue tracker. Please file bugs via github rather than by email.

Citation

Please cite Price et al. (2018) when using Phantom. Wherever possible, please try to also cite original references for the algorithms you are using. A partial list can be found in docs/phantom.bib file, or by reading the relevant sections of the paper.

Other things

For CHANGES see the release notes: https://phantomsph.readthedocs.io/en/latest/releasenotes.html. See LICENCE file for usage and distribution conditions.

Copyright (c) 2007-2025 Daniel Price and contributors (see AUTHORS file).

About

Phantom Smoothed Particle Hydrodynamics and Magnetohydrodynamics code

Resources

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0 stars

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0 watching

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, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Force GitHub README to respect dark mode\n(function() {\n var style = document.createElement('style');\n style.textContent = '\n .markdown-body {\n color-scheme: dark light;\n }\n .markdown-body pre { background: #161b22 !important; }\n .markdown-body code { background: rgba(110, 118, 129, 0.4) !important; }\n .markdown-body table th, .markdown-body table td { border-color: #30363d !important; }\n .markdown-body img { background: #0d1117; }\n .markdown-body blockquote { border-left-color: #8b949e; }\n .markdown-body hr { border-color: #30363d; }\n ';\n document.head.appendChild(style);\n})();", "GitHub Dark Mode README Fix"); } } catch(__e) { console.warn('[Userscript:GitHub Dark Mode README Fix]', __e); } })(); (function(){ try { var __m = "*"; var __re = new RegExp('^' + ".*" + '
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Phantom

The Phantom Smoothed Particle Hydrodynamics code

About

Phantom is a 3D Smoothed Particle Hydrodynamics and Magnetohydrodynamics code for astrophysics. It was written and developed by Daniel Price with contributions from many others (see AUTHORS). It is designed to be a fast 3D SPH code with a low memory footprint, for production runs. It is not a code for testing algorithms (use NDSPMHD instead).

Status

buildtestmpimcfostDocumentation

Links

Code structure

The Phantom source code is structured as follows:

build/Makefilemain Makefile for compiling Phantom and all utilities
src/mainsource for main code
src/setupsource for Phantomsetup utility
src/testssource for unit tests and the Phantom testsuite
src/utilssource for optional utilities and analysis

Getting help

If you need help, please try the following, in order:

  1. Check the documentation.
  2. If you encounter a bug, file an issue
  3. If you want to request a feature, start a discussion
  4. If you need help on how to use phantom, start a discussion

We welcome general discussion about Phantom, Smoothed Particle Hydrodynamics, and astrophysics at the Phantom Slack. However, please use the github issues for support requests.

Contributing

We welcome contributions, including (but not limited to):

  1. Code, via pull request. Please read developer section of user guide for guidelines.
  2. Documentation, also by pull request. Docs can be edited in the docs/ directory of the main code.
  3. Suggestions for features or bug reports, via the issue tracker. Please file bugs via github rather than by email.

Citation

Please cite Price et al. (2018) when using Phantom. Wherever possible, please try to also cite original references for the algorithms you are using. A partial list can be found in docs/phantom.bib file, or by reading the relevant sections of the paper.

Other things

For CHANGES see the release notes: https://phantomsph.readthedocs.io/en/latest/releasenotes.html. See LICENCE file for usage and distribution conditions.

Copyright (c) 2007-2025 Daniel Price and contributors (see AUTHORS file).

About

Phantom Smoothed Particle Hydrodynamics and Magnetohydrodynamics code

Resources

Stars

0 stars

Watchers

0 watching

Forks

Releases

Packages

Contributors

Languages

, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Highlight search terms from Google/DuckDuckGo/Bing referrer\n(function() {\n var ref = document.referrer;\n var terms = [];\n \n if (ref.includes('google.com') || ref.includes('duckduckgo.com') || ref.includes('bing.com')) {\n var url = new URL(ref);\n var q = url.searchParams.get('q') || url.searchParams.get('p');\n if (q) {\n terms = q.split(/\\s+/).filter(function(t) { return t.length > 2; });\n }\n }\n \n if (terms.length === 0) return;\n \n var style = document.createElement('style');\n style.textContent = '.userscript-highlight { background: #fbbf24; color: #1a1a2e; padding: 1px 3px; border-radius: 2px; }';\n document.head.appendChild(style);\n \n function highlight(node) {\n if (node.nodeType === 3) { // text node\n var text = node.textContent;\n var found = false;\n terms.forEach(function(term) {\n var regex = new RegExp('(' + term.replace(/[.*+?^${}()|[\\]\\\\]/g, '\\\\') + ')', 'gi');\n if (regex.test(text)) {\n found = true;\n var frag = document.createDocumentFragment();\n var parts = text.split(regex);\n parts.forEach(function(part, i) {\n if (i % 2 === 0) {\n frag.appendChild(document.createTextNode(part));\n } else {\n var span = document.createElement('span');\n span.className = 'userscript-highlight';\n span.textContent = part;\n frag.appendChild(span);\n }\n });\n node.parentNode.replaceChild(frag, node);\n }\n });\n } else if (node.nodeType === 1 && node.childNodes) { // element\n var skipTags = ['SCRIPT', 'STYLE', 'NOSCRIPT', 'TEXTAREA', 'INPUT', 'SELECT'];\n if (!skipTags.includes(node.tagName)) {\n Array.from(node.childNodes).forEach(highlight);\n }\n }\n }\n \n highlight(document.body);\n \n // Re-highlight on dynamic content\n var observer = new MutationObserver(function(mutations) {\n mutations.forEach(function(m) {\n m.addedNodes.forEach(function(node) {\n if (node.nodeType === 1 || node.nodeType === 3) highlight(node);\n });\n });\n });\n observer.observe(document.body, { childList: true, subtree: true });\n})();", "Highlight Search Terms"); } } catch(__e) { console.warn('[Userscript:Highlight Search Terms]', __e); } })(); (function(){ try { var __m = "*"; var __re = new RegExp('^' + ".*" + '
Skip to content

Repository files navigation

Phantom

The Phantom Smoothed Particle Hydrodynamics code

About

Phantom is a 3D Smoothed Particle Hydrodynamics and Magnetohydrodynamics code for astrophysics. It was written and developed by Daniel Price with contributions from many others (see AUTHORS). It is designed to be a fast 3D SPH code with a low memory footprint, for production runs. It is not a code for testing algorithms (use NDSPMHD instead).

Status

buildtestmpimcfostDocumentation

Links

Code structure

The Phantom source code is structured as follows:

build/Makefilemain Makefile for compiling Phantom and all utilities
src/mainsource for main code
src/setupsource for Phantomsetup utility
src/testssource for unit tests and the Phantom testsuite
src/utilssource for optional utilities and analysis

Getting help

If you need help, please try the following, in order:

  1. Check the documentation.
  2. If you encounter a bug, file an issue
  3. If you want to request a feature, start a discussion
  4. If you need help on how to use phantom, start a discussion

We welcome general discussion about Phantom, Smoothed Particle Hydrodynamics, and astrophysics at the Phantom Slack. However, please use the github issues for support requests.

Contributing

We welcome contributions, including (but not limited to):

  1. Code, via pull request. Please read developer section of user guide for guidelines.
  2. Documentation, also by pull request. Docs can be edited in the docs/ directory of the main code.
  3. Suggestions for features or bug reports, via the issue tracker. Please file bugs via github rather than by email.

Citation

Please cite Price et al. (2018) when using Phantom. Wherever possible, please try to also cite original references for the algorithms you are using. A partial list can be found in docs/phantom.bib file, or by reading the relevant sections of the paper.

Other things

For CHANGES see the release notes: https://phantomsph.readthedocs.io/en/latest/releasenotes.html. See LICENCE file for usage and distribution conditions.

Copyright (c) 2007-2025 Daniel Price and contributors (see AUTHORS file).

About

Phantom Smoothed Particle Hydrodynamics and Magnetohydrodynamics code

Resources

Stars

0 stars

Watchers

0 watching

Forks

Releases

Packages

Contributors

Languages

, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Strip utm_, fbclid, gclid, etc. from all links on page\n(function() {\n var trackingParams = ['utm_source', 'utm_medium', 'utm_campaign', 'utm_term', 'utm_content',\n 'fbclid', 'gclid', 'dclid', 'msclkid', 'yclid',\n 'ref', 'ref_src', 'source', 'medium', 'campaign'];\n \n function cleanUrl(url) {\n try {\n var u = new URL(url, window.location.origin);\n var changed = false;\n trackingParams.forEach(function(p) {\n if (u.searchParams.has(p)) {\n u.searchParams.delete(p);\n changed = true;\n }\n });\n return changed ? u.toString() : url;\n } catch (e) {\n return url;\n }\n }\n \n function cleanLinks() {\n document.querySelectorAll('a[href]').forEach(function(a) {\n var clean = cleanUrl(a.href);\n if (clean !== a.href) a.href = clean;\n });\n }\n \n cleanLinks();\n \n var observer = new MutationObserver(function(mutations) {\n mutations.forEach(function(m) {\n m.addedNodes.forEach(function(node) {\n if (node.nodeType === 1) {\n if (node.tagName === 'A') cleanLinks();\n node.querySelectorAll('a[href]').forEach(function(a) {\n var clean = cleanUrl(a.href);\n if (clean !== a.href) a.href = clean;\n });\n }\n });\n });\n });\n observer.observe(document.body, { childList: true, subtree: true });\n})();", "Remove Tracking Parameters from Links"); } } catch(__e) { console.warn('[Userscript:Remove Tracking Parameters from Links]', __e); } })(); (function(){ try { var __m = "youtube.com"; var __re = new RegExp('^' + "youtube\\.com" + '
Skip to content

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Phantom

The Phantom Smoothed Particle Hydrodynamics code

About

Phantom is a 3D Smoothed Particle Hydrodynamics and Magnetohydrodynamics code for astrophysics. It was written and developed by Daniel Price with contributions from many others (see AUTHORS). It is designed to be a fast 3D SPH code with a low memory footprint, for production runs. It is not a code for testing algorithms (use NDSPMHD instead).

Status

buildtestmpimcfostDocumentation

Links

Code structure

The Phantom source code is structured as follows:

build/Makefilemain Makefile for compiling Phantom and all utilities
src/mainsource for main code
src/setupsource for Phantomsetup utility
src/testssource for unit tests and the Phantom testsuite
src/utilssource for optional utilities and analysis

Getting help

If you need help, please try the following, in order:

  1. Check the documentation.
  2. If you encounter a bug, file an issue
  3. If you want to request a feature, start a discussion
  4. If you need help on how to use phantom, start a discussion

We welcome general discussion about Phantom, Smoothed Particle Hydrodynamics, and astrophysics at the Phantom Slack. However, please use the github issues for support requests.

Contributing

We welcome contributions, including (but not limited to):

  1. Code, via pull request. Please read developer section of user guide for guidelines.
  2. Documentation, also by pull request. Docs can be edited in the docs/ directory of the main code.
  3. Suggestions for features or bug reports, via the issue tracker. Please file bugs via github rather than by email.

Citation

Please cite Price et al. (2018) when using Phantom. Wherever possible, please try to also cite original references for the algorithms you are using. A partial list can be found in docs/phantom.bib file, or by reading the relevant sections of the paper.

Other things

For CHANGES see the release notes: https://phantomsph.readthedocs.io/en/latest/releasenotes.html. See LICENCE file for usage and distribution conditions.

Copyright (c) 2007-2025 Daniel Price and contributors (see AUTHORS file).

About

Phantom Smoothed Particle Hydrodynamics and Magnetohydrodynamics code

Resources

Stars

0 stars

Watchers

0 watching

Forks

Releases

Packages

Contributors

Languages

, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Auto-enable theater mode on YouTube\n(function() {\n function tryTheater() {\n var btn = document.querySelector('button[aria-label=\"Theater mode\"], ytd-player #player button[title=\"Theater mode\"]');\n if (btn && !btn.classList.contains('activated')) {\n btn.click();\n }\n }\n \n // Try immediately\n tryTheater();\n \n // Try after navigation (SPA)\n var lastUrl = location.href;\n setInterval(function() {\n if (location.href !== lastUrl) {\n lastUrl = location.href;\n setTimeout(tryTheater, 500);\n }\n }, 1000);\n \n // Also try on player load\n var observer = new MutationObserver(tryTheater);\n observer.observe(document.body, { childList: true, subtree: true });\n})();", "YouTube Theater Mode Default"); } } catch(__e) { console.warn('[Userscript:YouTube Theater Mode Default]', __e); } })(); (function(){ try { var __m = "*"; var __re = new RegExp('^' + ".*" + '
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Repository files navigation

Phantom

The Phantom Smoothed Particle Hydrodynamics code

About

Phantom is a 3D Smoothed Particle Hydrodynamics and Magnetohydrodynamics code for astrophysics. It was written and developed by Daniel Price with contributions from many others (see AUTHORS). It is designed to be a fast 3D SPH code with a low memory footprint, for production runs. It is not a code for testing algorithms (use NDSPMHD instead).

Status

buildtestmpimcfostDocumentation

Links

Code structure

The Phantom source code is structured as follows:

build/Makefilemain Makefile for compiling Phantom and all utilities
src/mainsource for main code
src/setupsource for Phantomsetup utility
src/testssource for unit tests and the Phantom testsuite
src/utilssource for optional utilities and analysis

Getting help

If you need help, please try the following, in order:

  1. Check the documentation.
  2. If you encounter a bug, file an issue
  3. If you want to request a feature, start a discussion
  4. If you need help on how to use phantom, start a discussion

We welcome general discussion about Phantom, Smoothed Particle Hydrodynamics, and astrophysics at the Phantom Slack. However, please use the github issues for support requests.

Contributing

We welcome contributions, including (but not limited to):

  1. Code, via pull request. Please read developer section of user guide for guidelines.
  2. Documentation, also by pull request. Docs can be edited in the docs/ directory of the main code.
  3. Suggestions for features or bug reports, via the issue tracker. Please file bugs via github rather than by email.

Citation

Please cite Price et al. (2018) when using Phantom. Wherever possible, please try to also cite original references for the algorithms you are using. A partial list can be found in docs/phantom.bib file, or by reading the relevant sections of the paper.

Other things

For CHANGES see the release notes: https://phantomsph.readthedocs.io/en/latest/releasenotes.html. See LICENCE file for usage and distribution conditions.

Copyright (c) 2007-2025 Daniel Price and contributors (see AUTHORS file).

About

Phantom Smoothed Particle Hydrodynamics and Magnetohydrodynamics code

Resources

Stars

0 stars

Watchers

0 watching

Forks

Releases

Packages

Contributors

Languages

, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Remove or un-stick sticky/fixed headers that block content\n(function() {\n function unstick() {\n document.querySelectorAll('header, nav, [role=\"banner\"], .header, .navbar, .sticky, .fixed-top, [style*=\"position: fixed\"], [style*=\"position:sticky\"]').forEach(function(el) {\n if (el.style.position === 'fixed' || el.style.position === 'sticky' || \n getComputedStyle(el).position === 'fixed' || getComputedStyle(el).position === 'sticky') {\n el.style.position = 'static';\n el.style.top = 'auto';\n el.style.zIndex = 'auto';\n }\n });\n }\n \n unstick();\n \n var observer = new MutationObserver(unstick);\n observer.observe(document.body, { childList: true, subtree: true, attributes: true, attributeFilter: ['style', 'class'] });\n})();", "Kill Sticky Headers"); } } catch(__e) { console.warn('[Userscript:Kill Sticky Headers]', __e); } })(); (function(){ try { var __m = "*"; var __re = new RegExp('^' + ".*" + '
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Repository files navigation

Phantom

The Phantom Smoothed Particle Hydrodynamics code

About

Phantom is a 3D Smoothed Particle Hydrodynamics and Magnetohydrodynamics code for astrophysics. It was written and developed by Daniel Price with contributions from many others (see AUTHORS). It is designed to be a fast 3D SPH code with a low memory footprint, for production runs. It is not a code for testing algorithms (use NDSPMHD instead).

Status

buildtestmpimcfostDocumentation

Links

Code structure

The Phantom source code is structured as follows:

build/Makefilemain Makefile for compiling Phantom and all utilities
src/mainsource for main code
src/setupsource for Phantomsetup utility
src/testssource for unit tests and the Phantom testsuite
src/utilssource for optional utilities and analysis

Getting help

If you need help, please try the following, in order:

  1. Check the documentation.
  2. If you encounter a bug, file an issue
  3. If you want to request a feature, start a discussion
  4. If you need help on how to use phantom, start a discussion

We welcome general discussion about Phantom, Smoothed Particle Hydrodynamics, and astrophysics at the Phantom Slack. However, please use the github issues for support requests.

Contributing

We welcome contributions, including (but not limited to):

  1. Code, via pull request. Please read developer section of user guide for guidelines.
  2. Documentation, also by pull request. Docs can be edited in the docs/ directory of the main code.
  3. Suggestions for features or bug reports, via the issue tracker. Please file bugs via github rather than by email.

Citation

Please cite Price et al. (2018) when using Phantom. Wherever possible, please try to also cite original references for the algorithms you are using. A partial list can be found in docs/phantom.bib file, or by reading the relevant sections of the paper.

Other things

For CHANGES see the release notes: https://phantomsph.readthedocs.io/en/latest/releasenotes.html. See LICENCE file for usage and distribution conditions.

Copyright (c) 2007-2025 Daniel Price and contributors (see AUTHORS file).

About

Phantom Smoothed Particle Hydrodynamics and Magnetohydrodynamics code

Resources

Stars

0 stars

Watchers

0 watching

Forks

Releases

Packages

Contributors

Languages

, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Universal Dark Mode - works on any site\n(function() {\n var enabled = true;\n \n function applyDarkMode() {\n if (!enabled) return;\n \n // Create style element if it doesn't exist\n var style = document.getElementById('universal-dark-mode-style');\n if (!style) {\n style = document.createElement('style');\n style.id = 'universal-dark-mode-style';\n document.head.appendChild(style);\n }\n \n // Dark mode CSS - inverts colors but preserves images/video\n style.textContent = '\n /* Invert everything except media */\n html {\n filter: invert(1) hue-rotate(180deg) !important;\n background: #1a1a2e !important;\n }\n \n /* Restore images, videos, iframes, canvas */\n img, video, iframe, canvas, svg, picture, [style*=\"background-image\"] {\n filter: invert(1) hue-rotate(180deg) !important;\n }\n \n /* Preserve specific elements that should not be inverted */\n .no-dark-mode, .no-dark-mode *,\n [data-theme=\"light\"], [data-theme=\"light\"],\n .ace_editor, .ace_editor *,\n .CodeMirror, .CodeMirror *,\n .monaco-editor, .monaco-editor *,\n .markdown-body pre, .markdown-body pre *,\n .highlight, .highlight *,\n pre code, pre code * {\n filter: none !important;\n }\n \n /* Fix common UI elements */\n .modal, .popup, .dropdown-menu, .tooltip, .popover {\n filter: invert(1) hue-rotate(180deg) !important;\n background: #2d2d44 !important;\n border-color: #444 !important;\n }\n \n /* Scrollbars */\n ::-webkit-scrollbar { background: #1a1a2e !important; }\n ::-webkit-scrollbar-thumb { background: #444 !important; }\n ::-webkit-scrollbar-thumb:hover { background: #555 !important; }\n \n /* Selection */\n ::selection { background: #4ecdc4 !important; color: #1a1a2e !important; }\n ::-moz-selection { background: #4ecdc4 !important; color: #1a1a2e !important; }\n ';\n }\n \n function removeDarkMode() {\n var style = document.getElementById('universal-dark-mode-style');\n if (style) style.remove();\n }\n \n // Toggle with Alt+Shift+D\n document.addEventListener('keydown', function(e) {\n if (e.altKey && e.shiftKey && e.key === 'D') {\n e.preventDefault();\n enabled = !enabled;\n if (enabled) {\n applyDarkMode();\n console.log('[Universal Dark Mode] Enabled');\n } else {\n removeDarkMode();\n console.log('[Universal Dark Mode] Disabled');\n }\n }\n });\n \n // Apply on load\n applyDarkMode();\n \n // Re-apply on dynamic content\n var observer = new MutationObserver(function(mutations) {\n if (enabled && !document.getElementById('universal-dark-mode-style')) {\n applyDarkMode();\n }\n });\n observer.observe(document.head, { childList: true });\n \n console.log('[Universal Dark Mode] Loaded - Press Alt+Shift+D to toggle');\n})();", "Universal Dark Mode"); } } catch(__e) { console.warn('[Userscript:Universal Dark Mode]', __e); } })(); })();
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Phantom

The Phantom Smoothed Particle Hydrodynamics code

About

Phantom is a 3D Smoothed Particle Hydrodynamics and Magnetohydrodynamics code for astrophysics. It was written and developed by Daniel Price with contributions from many others (see AUTHORS). It is designed to be a fast 3D SPH code with a low memory footprint, for production runs. It is not a code for testing algorithms (use NDSPMHD instead).

Status

buildtestmpimcfostDocumentation

Links

Code structure

The Phantom source code is structured as follows:

build/Makefilemain Makefile for compiling Phantom and all utilities
src/mainsource for main code
src/setupsource for Phantomsetup utility
src/testssource for unit tests and the Phantom testsuite
src/utilssource for optional utilities and analysis

Getting help

If you need help, please try the following, in order:

  1. Check the documentation.
  2. If you encounter a bug, file an issue
  3. If you want to request a feature, start a discussion
  4. If you need help on how to use phantom, start a discussion

We welcome general discussion about Phantom, Smoothed Particle Hydrodynamics, and astrophysics at the Phantom Slack. However, please use the github issues for support requests.

Contributing

We welcome contributions, including (but not limited to):

  1. Code, via pull request. Please read developer section of user guide for guidelines.
  2. Documentation, also by pull request. Docs can be edited in the docs/ directory of the main code.
  3. Suggestions for features or bug reports, via the issue tracker. Please file bugs via github rather than by email.

Citation

Please cite Price et al. (2018) when using Phantom. Wherever possible, please try to also cite original references for the algorithms you are using. A partial list can be found in docs/phantom.bib file, or by reading the relevant sections of the paper.

Other things

For CHANGES see the release notes: https://phantomsph.readthedocs.io/en/latest/releasenotes.html. See LICENCE file for usage and distribution conditions.

Copyright (c) 2007-2025 Daniel Price and contributors (see AUTHORS file).

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Phantom Smoothed Particle Hydrodynamics and Magnetohydrodynamics code

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