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quarknova.ca

quark nova project

QNP | Quark Nova Project

Global rank: #20926867
Daily visitors: 0.16K
Monthly Visits: 4,902
Pageviews per user: 0.02
Registrar Abuse Contact Email: [email protected]
Registrant Phone:
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TLD: ca
IP Address: 216.137.189.153
Organization: A Hosting, Inc.
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quarknova.ca
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Last Updated: 18 day ago
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quark nova project

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quarknova.ca Trust Score

quarknova.ca is probably legit as the trust score is reasonable. Our algorithm rated quarknova.ca a 60. Although our rating of quarknova.ca is medium to low risk, we encourage you to always vote as the evaluation of the site is done automatically.

The trust rating is high. Might be safe.
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Which Sites are Alternatives & Competitors to quarknova.ca?

Explore the top alternatives and rivals of quarknova.ca in September 2024, and assess their data relating to website traffic, SEO, Web Server Information, and Whois. Refer to the list below for the best competitors of quarknova.ca, and simply click on each one to delve into their specific details.

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Mentioned on Their Website:

  • theor.jinr.ru
    Conference 2017

    http://theor.jinr.ru/~hmec/csqcd6/

    Previous Meetings could be found on the website: Quarknova.ca. International Steering Committee: Rachid Ouyed (Chair) (Canada), Prashanth Jaikumar (USA / India), Ignazio Bombaci (Italy), Rodrigo Negreiros (Brazil), David Blaschke (JINR / Poland), Jochen Wambach (Germany), Efrain Ferrer (USA),

  • aas.org
    CSQCD IX: From RHIC to Astrophysics, Probing the …

    https://aas.org/events/2021-07/csqcd-ix-rhic-astrophysics-probing-quark-gluon-plasma

    More information. https://quarknova.ca/CSQCDIX/ The Banff meeting will focus on recent explorations of the quark-gluon phase using colliders (e.g. RHIC and …

  • encyclopedia.pub
    The Macro-Physics of the Quark-Nova | Encyclopedia MDPI

    https://encyclopedia.pub/entry/24522

    Since the 1980s, different groups have sought to elucidate the phenomenology of this energy release. Olinto [ 23] pioneered a hydrodynamic formalism …

  • arxiv.org
    arXiv:1510.06135v1 [astro-ph.HE] 21 Oct 2015

    https://arxiv.org/pdf/1510.06135v1.pdf

    2 Ouyed et al. (2010)). The relativistic QN ejecta has an average Lorentz factor QN ˘10 with a corresponding kinetic energy, E QN, exceeding 1052 erg (Ker anen et al. (2005); Ouyed & Leahy (2009)). Here we focus on a scenario where the QN occurs in …

  • mdpi.com
    The Macro-Physics of the Quark-Nova: Astrophysical Implications …

    https://www.mdpi.com/2218-1997/8/6/322

    A quark-nova is a hypothetical stellar evolution branch where a neutron star converts explosively into a quark star. Here, we discuss the intimate coupling between the micro-physics and macro-physics of the quark-nova and provide a prescription for how to couple the Burn-UD code to the stellar evolution code in order to simulate neutron-star …

  • inspirehep.net
    Simulating Hadronic-to-Quark-Matter with Burn-UD: Recent …

    https://inspirehep.net/files/a222b4a0936797ad213410d712f42b40

    Content from this work may be used under the terms of the CreativeCommonsAttribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.

  • forum.musesframework.io
    Interesting conference: CSQCD IX - General - MUSES

    https://forum.musesframework.io/t/interesting-conference-csqcd-ix/320

    CSQCD IX is an IN-PERSON meeting and will take place at the Banff Centre in Banff, Alberta, Canada from August 1-5, 2022. http://quarknova.ca/CSQCDIX/. …

  • arxiv.org
    arXiv:1502.06892v2 [astro-ph.HE] 16 Sep 2015

    https://arxiv.org/pdf/1502.06892

    2 Ouyed et al. ing efficiency. The CE kinetic energy is found from E QN = E CE,K + E CE,th. where the CE thermal energy is E CE,th. = E CE,gas + E CE,rad., shared between the gas and the radiation. We find that even for extreme

  • ar5iv.labs.arxiv.org
    [1510.06135] Quark-Novae occurring in massive binaries : A …

    https://ar5iv.labs.arxiv.org/html/1510.06135

    In Ouyed et al. (2015a, b) we showed how SLSNe-I light-curves, such as for LSQ14bdq (Nicholl et al. ()), SN 2006oz (Leloudas et al. ()) and DES13S2cmm (Papadopoulos et al. ()) can be fit by a QN in a massive stellar binary.Our binary model (illustrated in Figure 1 in Ouyed et al. ()), has component A (i.e. the more massive component) explode as a …

  • academic.oup.com
    Quark-Novae in massive binaries: a model for double-humped, …

    https://academic.oup.com/mnras/article/454/3/2353/1204567

    Abstract. LSQ14bdq and SN 2006oz are superluminous, hydrogen-poor, SNe with double-humped light curves. We show that a Quark-Nova (QN; explosive transition of the Neutron Star – NS – to a quark star –QS) occurring in a massive binary, experiencing two Common Envelope (CE) phases, can quantitatively explain the light curves of …

  • lowbg.org
    R-process 元素の存在量分布 の研究

    https://www.lowbg.org/ugap/ws/sn2022/slides/Hagi.pdf

    •R-process: 鉄以上の元素の約半分を合成する過程 • 中性子星合体がr-processのサイトとして示された。 • 中性子星合体のdynamical ejectaにおいて、初期条件( )を与えることで、 どのように元素組成が変化するのかを調べている。 • 特に太陽系に存在するU, Thなどの強いr-processの元素合成に着目。

  • researchgate.net
    Nico KONING | astrophysics | The University of Calgary, Calgary …

    https://www.researchgate.net/profile/Nico-Koning

    A quark-nova (QN; the sudden transition from a neutron star into a quark star), which occurs in the second common envelope (CE) phase of a massive binary, gives excellent fits to superluminous ...

  • contacts.ucalgary.ca
    COURSE OUTLINE Course: Requisites: Grading

    https://contacts.ucalgary.ca/info/phas/files/info/unitis/courses/PHYS581/W2020/PHYS581-W2020-syllabus.pdf

    Department of Physics & Astronomy Science B 605 403 220-5385 [email protected] COURSE OUTLINE 1. Course: PHYS 581, Computational Physics III - Winter 2020 Lecture 01: T 11:00 - 11:50 in ST 026

  • aanda.org
    Quark-Nova | Astronomy & Astrophysics (A&A)

    https://www.aanda.org/articles/aa/abs/2002/30/aaee141/aaee141.html

    Quark-Nova. R. Ouyed1, J. Dey2 and M. Dey3. 1 Nordic Institute for Theoretical Physics, Blegdamsvej 17, DK-2100 Copenhagen, Denmark 2 Department of Physics, Maulana …

  • en.wikipedia.org
    Talk:Quark-nova - Wikipedia

    https://en.wikipedia.org/wiki/Talk:Quark-nova

    Main page; Contents; Current events; Random article; About Wikipedia; Contact us; Donate; Help; Learn to edit; Community portal; Recent changes; Upload file

  • researchgate.net
    (PDF) Simulating Hadronic-to-Quark-Matter with Burn-UD

    https://www.researchgate.net/publication/317566147_Simulating_Hadronic-to-Quark-Matter_with_Burn-UD_Recent_work_and_astrophysical_applications

    PDF | We present the new developments in Burn-UD, our in-house hydrodynamic combustion code used to model the phase transition of hadronic-to-quark... | Find, read and cite all the research you ...

  • researchgate.net
    QUARK-NOVAE OCCURRING IN MASSIVE BINARIES: A …

    https://www.researchgate.net/publication/293804462_QUARK-NOVAE_OCCURRING_IN_MASSIVE_BINARIES_A_UNIVERSAL_ENERGY_SOURCE_IN_SUPERLUMINOUS_SUPERNOVAE_WITH_DOUBLE-PEAKED_LIGHT_CURVES

    A quark-nova (QN; the sudden transition from a neutron star into a quark star), which occurs in the second common envelope (CE) phase of a massive binary, …

  • researchgate.net
    (PDF) The Effects of Elemental Abundances on Fitting

    https://www.researchgate.net/publication/360467189_The_Effects_of_Elemental_Abundances_on_Fitting_Supernova_Remnant_Models_to_Data

    Models for supernova remnant (SNR) evolution can be used to determine the energy of the explosion, the age of the SNR, and the density of the surrounding medium by matching observations.

  • indico.yukawa.kyoto-u.ac.jp
    Compact Stars in the QCD Phase diagram (7-October 11, 2024) · …

    https://indico.yukawa.kyoto-u.ac.jp/event/30/timetable/?view=standard_numbered

    QCD phase diagram and heavy ion collisions: overview and research talk Panasonic Hall

  • ascl.net
    ASCL.net - Request Change or Additions to an Existing Code

    https://ascl.net/code/change/212

    Request Change or Additions to an Existing Code. Request changes or additions to a code entry using this form. Your changes will be sent to an editor for consideration and moderation and will appear publicly after approved by an editor.

  • ui.adsabs.harvard.edu
    Quark-novae Occurring in Massive Binaries - NASA/ADS

    https://ui.adsabs.harvard.edu/abs/2016ApJ...818...77O/abstract

    A quark-nova (QN; the sudden transition from a neutron star into a quark star), which occurs in the second common envelope (CE) phase of a massive binary, gives excellent fits to …

  • paperswithcode.com
    Quark-Novae occurring in massive binaries - Papers With Code

    https://paperswithcode.com/paper/quark-novae-occurring-in-massive-binaries-a

    task dataset model metric name metric value global rank remove

  • es.wikipedia.org
    Quark-nova - Wikipedia, la enciclopedia libre

    https://es.wikipedia.org/wiki/Quark-nova

    Una quark-nova es la hipotética explosión violenta resultante de la conversión de una estrella de neutrones en una estrella de quarks. De manera análoga a una supernova …

  • britannica.com
    Quark | Definition, Flavors, & Colors | Britannica

    https://www.britannica.com/science/quark

    quark, any member of a group of elementary subatomic particles that interact by means of the strong force and are believed to be among the fundamental constituents of matter.

  • ar5iv.labs.arxiv.org
    [1505.05764] Quark-Novae in massive binaries : a model for …

    https://ar5iv.labs.arxiv.org/html/1505.05764

    A dual-shock QN (dsQN) happens when the QN occurs days to weeks after the SN explosion of the progenitor star. The time delay means that the QN ejecta catches up and collides with the SN ejecta after it has expanded to large radii (Leahy & Ouyed (); Ouyed & Leahy ()).Effectively, the QN re-energizes the extended SN ejecta causing a re …

  • researchgate.net
    iPTF13ehe in the context of Quark-Novae in massive

    https://www.researchgate.net/publication/283117943_iPTF13ehe_in_the_context_of_Quark-Novae_in_massive_binaries_double-humped_hydrogen-poor_superluminous_Supernovae_as_standard_candles

    A quark-nova (QN; the sudden transition from a neutron star into a quark star), which occurs in the second common envelope (CE) phase of a massive binary, gives excellent fits to superluminous ...

  • apps.aavso.org
    The Hunt for the Quark-Nova; a Call for Observers (Abstract)

    https://apps.aavso.org/jaavso/article/2812/

    (Abstract only) A Quark Nova is the explosive transition from a neutron star to a quark star that is theorized to take place days or weeks after a small fraction of “normal” Type II …

  • foodnetwork.com
    What Is Quark? | Cooking School | Food Network

    https://www.foodnetwork.com/how-to/packages/food-network-essentials/what-is-quark

    Quark is a creamy, soft, fresh cow’s milk cheese that is high in protein and can be low-fat, depending on its milkfat content. Quark’s origins can be traced back to …

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DNS Lookup

DNS entries, such as A, NS, MX, and TXT records, are crucial for the functioning of the Internet. The A record maps a domain name to an IPv4 address, while the NS record specifies authoritative name servers for a domain. The MX record identifies the mail server responsible for receiving email messages for a domain. Additionally, the TXT record allows for the association of any text information with a domain name. These records play a vital role in ensuring proper communication and connectivity across the internet.

HostClassTTLTypeData
quarknova.caIN10800Aip: 216.137.189.153
quarknova.caIN10800NStarget: motorhead.easydns.org
quarknova.caIN10800NStarget: rush.easydns.com
quarknova.caIN10800NStarget: nirvana.easydns.net
quarknova.caIN10800SOAmname: rush.easydns.comrname: zone.easydns.comserial: 1681457977refresh: 43200retry: 10800expire: 1209600minimum-ttl: 300
quarknova.caIN10800MXtarget: mxb.mailgun.orgpri: 10
quarknova.caIN10800MXtarget: mxa.mailgun.orgpri: 10
quarknova.caIN10800TXTtxt: v=spf1 include:mailgun.org ~all

quarknova.ca Traffic Analysis

According to global rankings, quarknova.ca holds the position of #20926867. It attracts an approximate daily audience of 0.16K visitors, leading to a total of 276 pageviews. On a monthly basis, the website garners around 4.9K visitors.

Daily Visitors0.16K
Monthly Visits4.9K
Pages per Visit0.02
Visit Duration0:00
Bounce Rate45.05%
Want complete report?Full SEMrush Report >>
Daily Unique Visitors:
163
Monthly Visits:
4902
Pages per Visit:
0.02
Daily Pageviews:
276
Avg. visit duration:
0:00
Bounce rate:
45.05%
Monthly Visits (SEMrush):
5559

Traffic Sources

SourcesTraffic Share
Social:
0.00%
Paid Referrals:
100.00%
Mail:
0.00%
Search:
0.00%
Direct:
0.00%

Visitors by Country

CountryTraffic Share
United States:
19.45%
Thailand:
13.39%
Spain:
12.74%
Germany:
11.83%
Australia:
11.70%

SSL Checker - SSL Certificate Verify

An SSL certificate is a digital certificate that ensures a secure encrypted connection between a web server and a user's browser. It provides authentication and encryption to keep data private and protected during transmission. quarknova.ca supports HTTPS, demonstrating their commitment to providing a secure browsing experience for users.

HTTP Headers

HTTP headers are additional segments of data exchanged between a client (e.g. a web browser) and a server during an HTTP request or response. They serve to provide instructions, metadata, or control parameters for the interaction between the client and server.

N/A.

Where is quarknova.ca hosted?

quarknova.ca is likely hosted in various data centers located across different regions worldwide. The current data center mentioned is just one of many where the website may be hosted.

Whois Information

WHOIS protocol used to get domain/IP info. Common for reg details, ownership of a domain/IP. Check quarknova.ca for reg/admin contact info, owner, org, email, phone, creation, and expiration dates.

Domain Updated Date:2024-02-25
Domain Created Date:2011-03-10
Domain Expiry Date:
Domain Name:
Registrar WHOIS Server:whois.ca.fury.ca
Registrar Abuse Contact Email:[email protected]
Registrar Abuse Contact Phone:+1.4165358672
Domain Registrar:easyDNS Technologies Inc.
Domain Owner:

Domain Name: quarknova.ca

Registry Domain ID: 1187049-CIRA

Registrar WHOIS Server: whois.ca.fury.ca

Registrar URL: www.easydns.ca

Updated Date: 2024-02-25T23:08:52Z

Creation Date: 2011-03-10T18:31:35Z

Registry Expiry Date: 2025-03-10T18:31:35Z

Registrar: easyDNS Technologies Inc.

Registrar IANA ID: not applicable

Registrar Abuse Contact Email: [email protected]

Registrar Abuse Contact Phone: +1.4165358672

Name Server: rush.easydns.com

SEO Analysis

SEO analysis involves examining the performance of a website, including titles, descriptions, keywords, and website speed. It also includes identifying popular keywords and researching competitor websites to understand their strategies. The analysis aims to optimize the website's visibility and improve its ranking on search engines.

Title Tag:
QNP | Quark Nova Project

Length: 24 characters

Title tags are usually best kept short, within 50-70 characters. It's important to note that search engines will typically read the entire title tag even if it exceeds 70 characters, but there is a chance they may cut it off or disregard it.

Meta Description:
Quark Nova Project

Length: 18 characters

When crafting website descriptions, keep in mind that search engines only show the first 150-160 characters in search results. To ensure your entire description is visible, aim for a length of 25-160 characters. If your description is too long, it may get cut off. Conversely, if it's too short, search engines may add text from elsewhere on your page. Additionally, search engines may modify the description you provide to better match the user's search intent. It's best to strike a balance between brevity and relevance for optimal visibility.

Meta Keywords:

No meta keywords found.

In the realm of search engine optimization, the meta keywords tag has become a relic of the past due to its potential for misuse, ultimately leading major search engines to disregard it in their ranking algorithms.

Keywords Cloud:
Term Count Density
quark 89 3.19%
star 52 1.87%
neutron 44 1.58%
stars 42 1.51%
nova 29 1.04%

A crucial factor in search engine optimization is keyword density, which refers to the proportion of a particular keyword present in the text of a webpage. In order to achieve high rankings on search engine results pages, it is essential to maintain the appropriate keyword density for your primary keyword.

Headings:
<H1>
0
<H2>
10
<H3>
43
<H4>
0
<H5>
0
<H6>
0
<h2>Recent Papers</h2>
<h2>Q & A</h2>
<h2>Software</h2>
<h2>About Us</h2>
<h2>Twitter Feed</h2>
<h2>Get in Touch</h2>
<h2>Multimedia</h2>
<h2>Our Work</h2>
<h2>Research Interests</h2>
<h2>Links</h2>
<h3> SirOp</h3>
<h3>Animations, pod-casts and photo albums</h3>
<h3> SHAPE</h3>
<h3> r-Java</h3>
<h3> Quark Nova Feature Animation</h3>
<h3> Slacker Astronomy Podcast</h3>
<h3> Quark Nova Binary System Animation</h3>
<h3> JetGet</h3>
<h3>Questions</h3>
<h3>Contact Details</h3>
<h3>News, Questions, Discussion...</h3>
<h3>Places on the web we think you might find interesting...</h3>
<h3>Answers to some of your Quark Nova related questions</h3>
<h3> SNRPy</h3>
<h3> Burn-UD</h3>
<h3>Camille Charignon</h3>
<h3> RoLo</h3>
<h3> DIGIGET</h3>
<h3>Amir Ouyed</h3>
<h3> Relevant Papers</h3>
<h3> Relevant Papers</h3>
<h3> Relevant Papers</h3>
<h3> Relevant Papers</h3>
<h3> Relevant Papers</h3>
<h3> Relevant Papers</h3>
<h3>Topics</h3>
<h3> What is the Quark Nova Project</h3>
<h3> Our Research Motivation</h3>
<h3> QN in the Media</h3>
<h3> Going Wherever the Quark Nova Takes Us</h3>
<h3> Relevant Papers</h3>
<h3> Relevant Papers</h3>
<h3>Jan Staff</h3>
<h3>Prashanth Jaikumar</h3>
<h3>Wolfgang Steffen</h3>
<h3>Zachary Shand</h3>
<h3>Brian Niebergal</h3>
<h3>Mathew Kostka</h3>
<h3>Learn About our Team.</h3>
<h3>Rachid Ouyed</h3>
<h3>Denis Leahy</h3>
<h3>Nico Koning</h3>
<h3>Luis Welbanks </h3>

In SEO, the primary focus is placed on keywords within the content. The title of the page holds the highest importance, followed by heading tags such as h1, h2, and h3. The h1 heading should be the largest on the page, while the h2 heading should be slightly smaller, and the h3 heading even smaller. This hierarchical structure is crucial for optimizing search engine rankings.

Image Alt Attribute:
47 images found in your page, and 24 images are without "ALT" text.

What is the issue about?
The tag does not have an ALT attribute defined. As a general rule, search engines do not interpret the content of image files. The text provided in the attribute enables the site owner to provide relevant information to the search engine and to the end user. Alt text is helpful to end users if they have images disabled or if the image does not properly load. In addition, the Alt text is utilized by screen readers. Make sure that your Alt text is descriptive and accurately reflects what the image represents and supports the content on the page.

How to fix?
Use the <img alt> attribute to write descriptive content for the image: <img source='pic.gif' alt='Accurate and descriptive keyword text that represents the image.' />.

Website Speed Test (Desktop):
0.15 seconds

Website speed is a measurement of how fast the content on your page loads. Website speed is one of many factors involved in the discipline of search engine optimization (SEO), but it is not the only one. In a recent study, the average load time for a web page was 3.21s.

Top Organic Search Terms:
Term Search Volume Traffic Traffic (%)
resonaances 210 0 0%

CO-Hosted

CoHosted refers to a situation where multiple domain names (websites) are using the same IP address to point to their respective web servers. They could be owned by different individuals or organizations and may serve entirely different purposes.

quarknova.ca

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Total reviews: 2
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Very positive reviews

rating 5

Total reviews: 2
Average score: 5 stars

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